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spectra Research

Working paper · September 2026

Cylindrical Yield-Curve Dynamics and the Arbitrage-Free Class

Zeyu Cao1 and Shaosai Huang2

Working paper. Comments welcome.

1 Independent Researcher, Long Island City, USA · [email protected]

2 Kspectra Research Inc., Toronto, Canada · [email protected]

Abstract

Finite-factor term-structure models assign no independent risk to exposures between their factors, although desks treat them as risks of their own. The cylindrical term-structure model of [13] gives each maturity an independent shock, but specifies real-world dynamics, leaving the link to arbitrage pricing open. This paper settles that question for every finite truncation of the deformation at fixed spread intensity, and then restores the stochastic spread in two conventions. The key observation is that the deformation’s damped sine modes are imaginary parts of complex exponentials, so the smallest shift-invariant family containing them is a doubled sine–cosine envelope whose added coordinates carry no noise. On this envelope, whether the factor drift is arbitrage-free reduces to one polynomial divisibility, which the model’s maturity diffusion fails on every mode. Because the failure sits in the noiseless coordinates, no change of measure removes it. No such truncation admits an equivalent martingale measure; for generic maturities an explicit arbitrage uses one bond more than there are modes; and the defect grows with resolution. Giving those coordinates noise of their own turns the impossibility into a market price of risk that diverges with resolution. Adjoining those coordinates, keeping the model’s noise and correcting only the drift makes every truncation arbitrage-free. The required convexity has an exact limit under refinement, with a short-end jump resolved in a boundary layer at the resolution scale. Bond-level volatilities converge, but forward-curve distributions do not: within this construction, maturity-local noise, no-arbitrage at every resolution and a curve-valued limit cannot coexist. The short-end value survives the stochastic spread. It is conserved at every vol-of-vol in the uncorrelated affine convention, and recovered at zero vol-of-vol in the bilinear quadratic–Gaussian convention under a recovery normalization, where each truncation has an exact existence criterion. The consistency test and the arbitrage construction extend beyond this model.

Contents
  1. 1Introduction
  2. 2The arbitrage-free class
    1. 2.1State space and curve dynamics
    2. 2.2The drift condition, with proof
    3. 2.3Quasi-exponential structure
    4. 2.4Arbitrage-free affine realisations
  3. 3The cylindrical SPDE, rigorously
    1. 3.1Model and spectral data
    2. 3.2Well-posedness under cylindrical noise
    3. 3.3Pointwise regularity: forward rates are not semimartingales
  4. 4The obstruction: symbol, witness, and magnitude
    1. 4.1The invariant envelope doubles
    2. 4.2The generator comparison is exact on the envelope
    3. 4.3Spectral locking and factor autocovariance
    4. 4.4A finite-bond witness
    5. 4.5The size of the obstruction
    6. 4.6The infinite model: an energy obstruction
    7. 4.7When the silent coordinates are loaded: a market-price-of-risk cost
  5. 5The arbitrage-free completion and its singular limit
    1. 5.1The minimal completion and the exact limit
    2. 5.2No curve-valued limit
    3. 5.3The long end
  6. 6The cost survives the stochastic spread
    1. 6.1The affine completion and its closure
    2. 6.2The short-end cost under stochastic intensity
    3. 6.3Existence, and what the surrogate costs
    4. 6.4Where complex spectrum may not live
    5. 6.5The bilinear channel: quadratic–Gaussian family and normalization
    6. 6.6What the normalization forces
    7. 6.7Finite-truncation existence
  7. 7Conclusion
    1. 7.1What has been shown
    2. 7.2Economic interpretation
    3. 7.3Limitations and open problems
  8. References
  9. How to cite

Keywords. Term structure of interest rates; Heath–Jarrow–Morton drift condition; finite-dimensional realisations; quasi-exponential curves; complex spectrum; maturity-white risk; bond arbitrage; quadratic–Gaussian models.

MSC 2020. 91G30, 60H15, 91G80. JEL. C65, E43, G12, G13.

1Introduction

A finite-factor term-structure model assigns no independent risk to exposures that fall between its factors. For a symmetric butterfly, the modelled exposure is only the second difference of smooth factor loadings, so it vanishes quadratically as the wings are brought in towards the centre maturity. Desks nevertheless hedge and charge for the position as though it carried local risk of its own. In practice, this gap is managed rather than eliminated. Factor truncation, tenor buckets, proxy hedges, convexity overlays and basis-risk reserves make a finite production system workable. They are operational accommodations: they do not specify how the residual maturity risk should enter a common dynamic pricing model.

Turning that residual-risk problem into a production pricing model requires answers to two separate questions. Finite implementation asks what a finite truncation preserves and what depends on its maturity resolution. Pricing consistency asks whether deterministic maturity roll-down and the Heath–Jarrow–Morton (HJM) convexity drift remain inside the volatility span, so that the truncation admits an equivalent local martingale measure. The first question concerns representation; the second concerns no-arbitrage.

The cylindrical method [13] addresses the risk representation first: one innovation is assigned to each maturity, rather than imposing smooth interpolation across neighbouring tenors. Write θ[0,θ]\theta \in [0,\theta ^*] for time to maturity up to the maximum modelled maturity θ\theta ^*. The forward curve is carried by a deformation field XX,

ft(θ)=rt+st[Y(θ)+Xt(θ)],f_t(\theta )=r_t+s_t\bigl [Y(\theta )+X_t(\theta )\bigr ],

with rtr_t a short rate, sts_t a scalar stochastic spread and YY a deterministic shape, and XX solves the second-order stochastic evolution equation

dXt=[θ+κ2θ2]Xtdt+σ0dBt,Xt(0)=Xt(θ)=0.dX_t=\Bigl [\partial _\theta +\frac \kappa 2\partial _\theta ^2\Bigr ]X_t\,dt+\sigma _0\,d\mathcal B_t, \qquad X_t(0)=X_t(\theta ^*)=0 .

Here θ\partial _\theta transports the curve as calendar time passes, κ2θ2\frac \kappa 2\partial _\theta ^2 diffuses shocks along the maturity axis at scale κ\kappa. The noise B\mathcal B is a cylindrical Brownian motion on H=L2([0,θ],e2θ/κdθ)H=L^2([0,\theta ^*],e^{2\theta /\kappa }d\theta ) of intensity σ0\sigma _0: one independent innovation per maturity, which is the whole point of the construction. The Dirichlet realisation of that generator has orthonormal eigenbasis

en(θ)=2/θeθ/κsinωnθ,ωn=nπθ,λn=1+κ2ωn22κ,e_n(\theta )=\sqrt {2/\theta ^*}\,e^{-\theta /\kappa }\sin \omega _n\theta , \qquad \omega _n=\frac {n\pi }{\theta ^*}, \qquad \lambda _n=\frac {1+\kappa ^2\omega _n^2}{2\kappa },

with eigenvalues λn-\lambda _n, so the coordinates xn=Xt,enHx_n=\langle X_t,e_n\rangle _H are independent Ornstein–Uhlenbeck processes reverting at rate λn\lambda _n. Each ene_n is a damped sine of maturity frequency ωn\omega _n and common damping scale κ\kappa. Equivalently, it is the imaginary part of a complex exponential with exponent 1/κ+iωn-1/\kappa +i\omega _n: the real sine–cosine pair carries the conjugate pair, and forward rates and bond prices remain real. These shapes belong to the class associated with finite-dimensional arbitrage-free realisations [619]. The dynamics, however, are specified under the real-world probability measure P\Pm, while the link to the risk-neutral pricing measure Q\Q is left open. With the spread held fixed, the link cannot be supplied as written: no finite sine truncation of the deformation admits an equivalent local martingale measure with its own volatility. That is the problem solved first; §6 then restores the stochastic spread.

We call XX the cylindrical deformation field and the displayed specification the source model. Unqualified, “the model” means the source model. In §§35, where the spread is held fixed, it means that model’s deformation sector, truncated to its first NN sine modes. “The completion” means the arbitrage-free construction of §5; each stochastic-spread family is named by the assumption and convention that defines it.

What makes the question answerable. To carry the analysis past the point at which the link to Q\Q was left open we start from the standard route: consistency is decided on finite-dimensional shift-invariant families of curve shapes [6719], in the invariant-manifold form of [21]. Here that route is compulsory rather than convenient. Under cylindrical noise the forward rate at a fixed maturity is not a semimartingale (§3), so the drift condition cannot be posed maturity by maturity at all. On the curve the comparison is not merely hard but ill-posed; finite-dimensional invariant subspaces are where the question can be made rigorous.

The route is blocked at its first step. It asks for a shift-invariant family, and the model has none. Its NN sine modes span no invariant space, so there is nothing for the realisation machinery to act on — which is where the matter had rested.

The block dissolves once the spectrum is read as complex. Each mode eθ/κsinωnθe^{-\theta /\kappa }\sin \omega _n\theta is the imaginary part of e(1/κ+iωn)θe^{(-1/\kappa +i\omega _n)\theta }. A conjugate pair admits no one-dimensional real invariant subspace, so the smallest invariant space containing one mode is two-dimensional. The model’s span therefore completes to the 2N2N-dimensional sine–cosine envelope, and it is on that envelope — not on the model’s own state space — that the comparison can be made. This is the step the rest of the paper rests on, and it pays twice over. It supplies the invariant family the standard route was asking for. And the coordinates it adjoins carry no noise, while the missing rotation ωn\omega _n acts precisely on them: what would have looked, on the model’s own span, like a correctable disagreement about drift is revealed as an obstruction that no change of measure can remove. Complexification is the mechanism here, not a change of notation.

The remaining steps follow from the envelope. On it the deformation and the arbitrage-free transport both act by matrices, so the comparison of drifts becomes algebra. A generator with symbol pp induces the factor drift p(M)p(M)^\top where no-arbitrage requires MM^\top, and the two agree exactly when mMpzm_M\mid p-z: the comparison is settled by one polynomial divisibility, and the convexity that HJM adds is carried by the deterministic sector. The envelope is also an ordinary finite-dimensional family, so the obstruction can be repaired rather than merely reported. Keeping the model’s loadings and its noise and correcting only the drift turns every truncation into an arbitrage-free model, and the refinement limit of those models fixes the resulting convexity exactly.

What this paper establishes. The deformation generator θ+κ2θ2\partial _\theta +\frac \kappa 2\partial _\theta ^2 has symbol p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2, so the symbol test fails on every decaying or oscillatory block; inside the weighted state space the tolerated class is the constants alone (§4). The doubling has a second consequence. The adjoined cosine partners violate the Dirichlet conditions, so the envelope leaves the domain of the closed generator (Proposition 4.1); the comparison is therefore a tangency statement about the formal symbol, which is precisely why no formulation inside the original domain is available. For the sine truncations at fixed intensity the failure is exact and measure-invariant at every order. No such truncation admits an equivalent local martingale measure (Remark 4.4); the witness construction exhibits the failure as a bond arbitrage (Theorem 4.6); and the obstruction modulus shows the unreachable part of the drift to be extensive rather than washed out by refinement (Proposition 4.8). For the infinite model the repairing shift fails the Girsanov finite-energy condition (Proposition 4.10), and the fully infinite bond-market statement is posed as open. When the silent coordinates are given noise of their own (§4.7), the impossibility becomes a price: every truncation then admits an equivalent measure, at a Sharpe cost growing like N3/2N^{3/2}, and the infinite factor laws are mutually singular (Proposition 4.11). Pointwise rates are not semimartingales (§3), so the finite-dimensional route is the rigorous one. The minimal completion has exact first-span interior limit q=σ022e2τ/κq^\infty =\frac {\sigma _0^2}2e^{-2\tau /\kappa }, a boundary layer on the scale θ/N\theta ^*/N with first-layer profile peak 1.455×σ02/21.455\times \sigma _0^2/2, and a short-end jump σ02/2\sigma _0^2/2 that is the drift cost of that completion. No curve-valued limit exists (Proposition 5.4). In the uncorrelated case, the cost survives the CIR-intensity extension at every vol-of-vol and the quadratic–Gaussian one on its η=0\eta =0 slice. For CIR intensity, the infinite-span surrogate exists precisely when λησ0κ/2\lambda \ge \eta \sigma _0\sqrt {\kappa /2}6.1); and the quadratic–Gaussian bilinear channel, under a stated recovery normalization, has an exact finite-NN existence criterion (Proposition 6.16).

In the table below, NN is the number of retained maturity modes and θ/N\theta ^*/N is their maturity-resolution scale. For each fixed NN, the original truncation and its completion are ordinary finite-factor bond markets; refinement in NN measures sensitivity to maturity resolution.

Issue

Common operational patch

Maturity-local method

Resolution in this paper

Finite
implementation

Variance-ranked factors, tenor buckets and local convexity overlays. These make a finite system usable, but leave resolution as an economically meaningful modelling choice.

One innovation per maturity restores local risk before truncation, but the cylindrical state itself is infinite-rank and cannot be evolved exactly by a production system.

For every NN, an ordinary finite HJM completion; an exact first-span convexity limit and θ/N\theta ^*/N boundary layer; and non-tight curve laws under refinement (Theorem 5.2, Proposition 5.4).

    

Pricing
consistency

Proxy hedges in nearby bonds, bucketed greeks, and basis-risk reserves and limits. They manage residual P&L, but do not themselves impose a joint martingale measure.

The real sine modes capture maturity-local shocks under P\Pm, while deterministic roll-down generates missing cosine directions outside the original shock span.

An exact range obstruction; a generic (N+1)(N+1)-bond arbitrage witness; an extensive stationary defect; and a completion that adjoins the roll-down states and required HJM convexity (Theorem 4.3, Theorem 4.6, Proposition 4.8).

These columns answer different questions. Operational patches manage portfolios in a finite system; the maturity-local method supplies a richer statistical risk field; the completion determines whether each finite truncation can price bonds without arbitrage and quantifies the cost of doing so.

Once a volatility and the minimal envelope have been selected, HJM consistency determines the drift uniquely within that completion. That drift is the cost quantified below; the premium a market attaches to the original unspanned risk is a separate question, which no-arbitrage alone does not settle.

Methodological contributions: four tools. The paper is organised so that four of its results can be lifted out of the instance that motivates them.

(i) A symbol test for consistency (Theorem 4.3(a)). The criterion is not tied to this instance. For any constant-coefficient generator with symbol pp and any shift-invariant block with generating matrix MM, the arbitrage-free drift is carried if and only if mMpzm_M\mid p-z. For diagonalisable MM this says that the symbol must fix the block’s spectrum pointwise, which is the form in which it is usually easiest to apply.

(ii) A constructive arbitrage witness (Theorem 4.6, Remark 4.7). From a state-linear drift discrepancy lying outside the volatility range, an explicit self-financing admissible arbitrage in N+1N+1 fixed-maturity bonds, on an open dense set of maturity tuples. The construction needs only analytic loadings, a Girsanov-unreachable discrepancy, and a nondegenerate state — and it exhibits the portfolio, where the fundamental theorem of asset pricing gives only existence.

(iii) A quantitative obstruction modulus (Proposition 4.8). The quotient distance from the discrepancy to the volatility range, with its exact stationary law: not whether a model violates no-arbitrage but by how much, and whether refinement attenuates the violation. Asking that question is not new: it is what the Hansen–Jagannathan distance asks in stochastic-discount-factor space [24]. This modulus is a narrower, model-internal object — a quotient distance in declared factor coordinates whose stationary law is exact. In that normalization it is a diagnostic, not a price.

(iv) Minimal completion as a repair, with a recoverable cost 5, §§6.16.5). The repair above, stated as a method rather than a computation: faced with a model that fails no-arbitrage, complete its state to the minimal shift-invariant hull, correct only the drift, and read the cost off the refinement limit instead of recording the failure and stopping. Repairing rather than discarding an inconsistent curve family is the move of the affine arbitrage-free Nelson–Siegel class [9], which keeps the Nelson–Siegel loadings and restores consistency through an explicit yield-adjustment term. What differs here is that the family is forced rather than given — the minimal hull of a state space possessing none — and that the cost is read off a refinement limit rather than at a fixed factor count. With the sine-only noise kept, the same short-end coefficient reappears in the uncorrelated affine convention at every vol-of-vol and in the bilinear convention on its zero-vol-of-vol slice. Across completions the cost can move: isotropic loading doubles the jump and smoothed cutoffs alter the overshoot (Remark 5.3(iii)). The positive-vol-of-vol bilinear case is not established.

Related work. The drift restriction is [25] in the parametrisation of [36]. Which curve families admit finite-dimensional arbitrage-free realisations was settled by Björk–Christensen, Björk–Svensson and Filipović [671920], with the invariant-manifold formulation in [21]. That classification is indifferent to whether the generating spectrum is real, and this paper takes up the half of it that term-structure practice has left unused. On a complex block the invariant family is two-dimensional, so a model built from sine modes alone is not merely inconvenient but incomplete; the coordinate its completion adjoins is where the obstruction turns out to live. Where the classification gives a condition to be verified family by family, Theorem 4.3(a) gives a decision procedure for the factor drift: one divisibility of polynomials.

Random-field term structures with smooth spatial covariance [332239] carry a drift condition written in terms of the covariance kernel. Cylindrical noise is the singular limit of that family: the kernel degenerates to a delta and the kernel-level drift condition is no longer available. Theorem 5.2 supplies what replaces it, and Remark 5.3(i) shows the resulting convexity to be exactly the half-delta that heuristic predicts — now with a boundary layer, a rate, and an exact constant. The analytic background for infinite-dimensional formulations is [815], and the pointwise regularity of §3 transcribes stochastic-heat-equation results [4140]. The use made of them here is one those results are not usually asked to support: the pointwise drift condition is unavailable, so the finite-dimensional route is forced rather than chosen. Against the long-end constraint [1627], Proposition 5.5 separates the two effects: complexification neither causes nor cures the classical pathology.

The equivalence–singularity dichotomy of §4.7 rests on a classical engine: Kakutani’s theorem for product measures [30] and, for Gaussian evolution equations, the criteria of Huebner and Rozovskii [28] (surveyed in [11]), under which the laws generated by two drift operators are equivalent or mutually singular according to the order of the operators’ difference. What is new is the financial reading. The invariant that decides the dichotomy is a market-price-of-risk energy, and the model sits on the singular side by a margin that grows like the cube of the truncation order. This bears on a question raised by [3], who study parabolic perturbations of the Musiela equation with the model in view and ask for the amount of arbitrage such a perturbation introduces to be quantified. Their metric is the pricing error of the perturbed curve; the defect energy of §4.7 is a complementary one, and on the envelope it answers as follows: every nonzero parabolic coefficient makes the infinite-envelope energy infinite, while every fixed finite truncation remains equivalent after tilting, at a Sharpe cost that grows with the truncation order. The heat-modulated model of [32] moves the Laplacian out of the drift and into the covariance process precisely in order to stay inside the HJM class; Proposition 4.11(c) shows that a nonzero second-order term cannot remain in the factor drift while preserving equivalence to the arbitrage-free infinite-envelope factor law.

The affine and quadratic–Gaussian classes of §§6.16.5 are [1814] and [23410], where solvability of the loading Riccati over the maturity range of interest is typically assumed. Here it is decided: for the affine surrogate by the exponential-moment criterion of [4] (Theorem 6.5), and for the quadratic–Gaussian channel at every fixed truncation by a conjugate-point criterion (Proposition 6.16), whose consequences uniform in NN are developed in the companion manuscript [42]. That finitely many factors need not span fixed-income risk is an established empirical theme [1226], and [17] bounds which spectral statements are testable under P\Pm. The framework of [35] is the natural one in which to relax deterministic factor volatility, and Markovian lifts of rough volatility [1] generate the same quasi-exponential structure on a different curve.

Set against that background, what this paper contributes begins at a single observation: the coordinate the doubled envelope adjoins is silent, and the obstruction lives precisely there. The decision procedure, the bond witness and the modulus are what that observation makes usable; the exact completion limit with its boundary layer (Theorem 5.2), and the failure of the repaired family to converge as a curve model (Proposition 5.4), are what it costs. We have not found the finite-portfolio construction elsewhere.

Organization. §2 assembles the yardstick: the state space and curve dynamics, the drift restriction with proof, the quasi-exponential classification, and the consistent affine realisations. §3 states the model and closes the pointwise route: under cylindrical noise, forward rates are not semimartingales, so the comparison is conducted on finite-dimensional invariant subspaces. §4 conducts it at three levels — the symbol test in factor coordinates, the bond-market witness, and the obstruction modulus — asks what survives in the infinite model, and prices the obstruction once the silent coordinates are loaded. §5 builds the completion, computes its singular limit and its drift cost, shows that no curve-valued limit exists, and disposes of the long end. §6 restores the stochastic spread in its two conventions, affine and bilinear, and shows that the short-end cost survives it — at every vol-of-vol in the affine convention, on the zero-vol-of-vol slice in the bilinear one. §7 concludes: it answers the two questions above, gives the financial reading of the answers, and states what remains open.

Companion material. The boundary theory of the quadratic–Gaussian existence region is developed separately in [42]. The fixed-NN criterion and the principal financial conclusions proved here are self-contained; the uniform-in-NN positive-vol-of-vol region quoted after Proposition 6.16 is a result of the companion manuscript.

Scope relative to the source model. The source construction models real-world dynamics, states that the arbitrage link is future work, and truncates the maturity domain at finite θmax\theta _{\max } explicitly to avoid the θ\theta \to \infty pathologies of Dybvig–Ingersoll–Ross type [13]. Nothing here identifies an error in that statistical construction; the question is what it costs to turn the method into a model under Q\Q, and the answer has exact structure.

AI-use disclosure. The authors used Anthropic Claude Code and OpenAI Codex as interactive research and writing tools. They assisted with exploratory discussion, testing and refinement of ideas, literature and source organization, code development and verification, mathematical error checking, and editorial revision.

2The arbitrage-free class

The introduction posed the question and wrote down the model; before the model can be measured, the standard has to be fixed. This section assembles that yardstick. Four ingredients are fixed once and used everywhere: the state space and the curve dynamics; the no-arbitrage drift restriction, with proof; the classification of curve shapes compatible with finite-dimensional arbitrage-free realisations; and the characterisation of the consistent realisations themselves. Nothing here is specific to the cylindrical model. A reader who has the HJM drift condition and the quasi-exponential class at hand may skim to §3.

2.1State space and curve dynamics

Everything is set on one Hilbert space of curves, chosen so that maturity roll-down is a strongly continuous semigroup and evaluation at a maturity is continuous.

State space and shift semigroup. Fix a weight w:R+[1,)w:\R _+\to [1,\infty ), nondecreasing, with 0w1/3<\int _0^\infty w^{-1/3}<\infty, and let HwH_w be the Filipović space [19] of absolutely continuous h:R+Rh:\R _+\to \R with

hw2:=|h(0)|2+0|h(τ)|2w(τ)dτ<.\|h\|_w^2:=|h(0)|^2+\int _0^\infty |h'(\tau )|^2\,w(\tau )\,d\tau <\infty .

HwH_w is a separable Hilbert space of continuous curves; point evaluations are continuous; the shift semigroup (Sth)(τ):=h(τ+t)(S_th)(\tau ):=h(\tau +t) is strongly continuous on HwH_w with generator τ\partial _\tau on its natural domain. Membership of a quasi-exponential is an additional integrability requirement, not a consequence of Reλ0\operatorname {Re}\lambda \le 0: a term p(τ)eλτp(\tau )e^{\lambda \tau } belongs to HwH_w precisely when its derivative is square-integrable against ww. In particular constants belong to HwH_w, whereas undamped oscillations and nonconstant polynomials do not (because w1w\ge 1). Finitely many strictly damped modes belong to HwH_w whenever ww is chosen to grow slowly enough relative to their damping; this includes the model’s modes, for example with w(τ)=eaτw(\tau )=e^{a\tau } and 0<a<2/κ0<a<2/\kappa. The model’s curves live on [0,θ][0,\theta ^*]; its eigenmodes extend uniquely to R+\R _+ by their quasi-exponential expressions, and all comparisons below are made on these extensions. The role of the Dirichlet boundary conditions is treated separately in Proposition 4.1.

Whenever an envelope or completion is read as an HwH_w-valued curve model, we also impose the damping-compatible condition

(1)Cw:=0e2τ/κw(τ)dτ<,\begin{equation}\label {eq:modeweight} C_w:=\int _0^\infty e^{-2\tau /\kappa }w(\tau )\,d\tau <\infty , \end{equation}

which the exponential weight above satisfies. The condition is used only where loading blocks are embedded as curves in HwH_w; statements made in factor coordinates, and the product-law statements of §4.7, stand without it.

HJMM dynamics. Under a measure Q\Q carrying a dd-dimensional Brownian motion W\W, the forward curve rtHwr_t\in H_w follows the Heath–Jarrow–Morton–Musiela dynamics

(2)drt=(τrt+αt)dt+σtdWt,\begin{equation}\label {eq:hjmm} dr_t=\bigl (\partial _\tau r_t+\alpha _t\bigr )\,dt+\sigma _t\,d\W _t, \end{equation}

interpreted in the mild sense rt=Str0+0tStsαsds+0tStsσsdWsr_t=S_tr_0+\int _0^tS_{t-s}\alpha _s\,ds+\int _0^tS_{t-s}\sigma _s\,d\W _s. Here α:Ω×R+×R+R\alpha :\Omega \times \R _+\times \R _+\to \R and σ\sigma is row-vector valued; both are jointly measurable, adapted and locally integrable in the appropriate norms. (See [1915] for the existence theory; none of the delicate cases arise for the affine models used here, whose solutions are explicit.)

2.2The drift condition, with proof

The restriction below is the Heath–Jarrow–Morton no-arbitrage condition [25] in the Musiela parametrisation [36]; we record it with proof because every later statement is an instance of it.

Lemma 2.1 (HJM drift restriction) . Let bond prices be P(t,T)=exp(0Ttrt(u)du)P(t,T)=\exp \bigl (-\int _0^{T-t}r_t(u)\,du\bigr ) and let the savings account be Bt=exp(0trs(0)ds)B_t=\exp \bigl (\int _0^t r_s(0)\,ds\bigr ). Suppose rr solves (2) and that, on every bounded maturity triangle, the integrability conditions for stochastic Fubini and Itô’s formula hold. Assume also that, for Qdt\Q \otimes dt-a.e. (ω,t)(\omega ,t), the maturity maps ταt(τ)\tau \mapsto \alpha _t(\tau ) and τσt(τ)\tau \mapsto \sigma _t(\tau ) are locally integrable, so their maturity integrals are absolutely continuous. Then P(,T)/BP(\cdot ,T)/B is a local Q\Q-martingale for every TT if and only if

(3)αt(τ)=σt(τ)0τσt(u)dufor a.e. τ, Qdt-a.e.\begin{equation}\label {eq:driftcond} \alpha _t(\tau )=\sigma _t(\tau )\int _0^\tau \sigma _t(u)^\top du \qquad \text {for a.e.\ }\tau ,\ \Q \otimes dt\text {-a.e.} \end{equation}
Under the physical measure P\Pm the same computation gives αt(τ)=σt(τ)(0τσt(u)du+γt)\alpha _t(\tau )=\sigma _t(\tau )\bigl (\int _0^\tau \sigma _t(u)^\top du+\gamma _t\bigr ) with γ\gamma the market price of risk, which is the form quoted in [13], Eq. (2); a proof is included for completeness.

Proof.Work in the HJM parametrisation f(t,T)=rt(Tt)f(t,T)=r_t(T-t), so that df(t,T)=αH(t,T)dt+σH(t,T)dWtdf(t,T)=\alpha ^{\mathrm H}(t,T)\,dt+\sigma ^{\mathrm H}(t,T)\,d\W _t with αH(t,T)=αt(Tt)\alpha ^{\mathrm H}(t,T)=\alpha _t(T-t), σH(t,T)=σt(Tt)\sigma ^{\mathrm H}(t,T)=\sigma _t(T-t); the τ\partial _\tau term in (2) is absorbed by the reparametrisation. Let Yt:=logP(t,T)=tTf(t,u)duY_t:=\log P(t,T)=-\int _t^Tf(t,u)\,du. By stochastic Fubini,

dYt=f(t,t)dttTdf(t,u)du=(rt(0)A(t,T))dtΣ(t,T)dWt,dY_t=f(t,t)\,dt-\int _t^T df(t,u)\,du=\Bigl (r_t(0)-A(t,T)\Bigr )dt-\Sigma (t,T)\,d\W _t,
with A(t,T)=tTαH(t,u)duA(t,T)=\int _t^T\alpha ^{\mathrm H}(t,u)\,du and Σ(t,T)=tTσH(t,u)du\Sigma (t,T)=\int _t^T\sigma ^{\mathrm H}(t,u)\,du. Itô on P=eYP=e^Y:
dP(t,T)P(t,T)=(rt(0)A(t,T)+12|Σ(t,T)|2)dtΣ(t,T)dWt.\frac {dP(t,T)}{P(t,T)}=\Bigl (r_t(0)-A(t,T)+\tfrac 12|\Sigma (t,T)|^2\Bigr )dt-\Sigma (t,T)\,d\W _t.
The discounted bond is a local martingale iff the drift equals rt(0)r_t(0), i.e. A(t,T)=12|Σ(t,T)|2A(t,T)=\frac 12|\Sigma (t,T)|^2 for all TT. Differentiating in TT gives αH(t,T)=σH(t,T)Σ(t,T)\alpha ^{\mathrm H}(t,T)=\sigma ^{\mathrm H}(t,T)\Sigma (t,T)^\top, which is (3) in Musiela coordinates τ=Tt\tau =T-t. Reversing the steps gives the converse. Under P\Pm, replace “local martingale” by “local martingale after the Girsanov tilt dWQ=dWP+γtdtd\W ^\Q =d\W ^\Pm +\gamma _t\,dt.”

The condition is on the drift given the volatility; the volatility itself — and in particular its spectrum in the sense of §2.3 — is unconstrained. The rest of the paper exploits this division of labour.

2.3Quasi-exponential structure

In Musiela coordinates, calendar time rolls every factor loading down the maturity axis. A finite-state term-structure model is closed only when that roll-down remains inside the chosen loading span. This is the financial meaning of shift invariance.

Definition 2.2. QE:={ipi(τ)eλiτ:piC[τ], λiC}\mathrm {QE}:=\bigl \{\sum _i p_i(\tau )e^{\lambda _i\tau }\,:\,p_i\in \C [\tau ],\ \lambda _i\in \C \bigr \}, real elements understood as those equal to their conjugates.

Theorem 2.3 (Finite-dimensional shift-invariant subspaces) . Let VC1(R+,R)V\subset C^1(\R _+,\R ) be finite-dimensional with τVV\partial _\tau V\subseteq V (elements are then automatically CC^\infty). Let MM be the matrix of τ|V\partial _\tau |_V in a basis B=(b1,,bn)\B =(b_1,\dots ,b_n)^\top, i.e. B=MB\B '=M\B. Then:

  1. B(τ)=eMτB(0)\B (\tau )=e^{M\tau }\B (0), and every vVv\in V satisfies the constant-coefficient ODE χM(τ)v=0\chi _M(\partial _\tau )v=0, where χM\chi _M is the characteristic polynomial of MM; hence VQEV\subseteq \mathrm {QE} with exponents specM\operatorname {spec}M and polynomial degrees bounded by the sizes of the Jordan blocks. Conversely a finite-dimensional quasi-exponential space is shift-invariant when, for each exponent λ\lambda, it contains complete downward-closed Jordan chains {eλτ,τeλτ,,τmλ1eλτ}\{e^{\lambda \tau },\tau e^{\lambda \tau },\ldots ,\tau ^{m_\lambda -1}e^{\lambda \tau }\} (and the conjugate chains in the real case). An arbitrary subspace of QE\mathrm {QE} need not be shift-invariant.
  2. (Real form.) Rn\R ^n decomposes into MM-invariant blocks on which MM is either a real Jordan block or, for a nonreal pair μ±iω\mu \pm i\omega, a real Jordan block with diagonal 2×22\times 2 cells C=(μωωμ)C=\bigl (\begin {smallmatrix}\mu& \omega \\-\omega& \mu \end {smallmatrix}\bigr ) and identity super-cells. On a semisimple complex cell,

    (4)eCτ=eμτR(ωτ),R(ϕ)=(cosϕsinϕsinϕcosϕ),\begin{equation}\label {eq:precession} e^{C\tau }=e^{\mu \tau }R(\omega \tau ),\qquad R(\phi )=\begin {pmatrix}\cos \phi &\sin \phi \\-\sin \phi &\cos \phi \end {pmatrix}, \end{equation}
    so the basis pair is eμτ(cosωτ, sinωτ)e^{\mu \tau }(\cos \omega \tau ,\ \sin \omega \tau ): exponential decay times rotation — precession.
  3. (Integration.) I(τ):=0τB(u)du=(0τeMudu)B(0)\Iv (\tau ):=\int _0^\tau \B (u)\,du=\bigl (\int _0^\tau e^{Mu}\,du\bigr )\B (0), where on the invertible part of MM, 0τeMudu=M1(eMτ1)\int _0^\tau e^{Mu}\,du=M^{-1}(e^{M\tau }-\one ), and on the nilpotent part (M=NM=N, Nm=0N^m=0), 0τeNudu=k=0m1τk+1(k+1)!Nk\int _0^\tau e^{Nu}\,du=\sum _{k=0}^{m-1}\frac {\tau ^{k+1}}{(k+1)!}N^k. In particular QE\mathrm {QE} is closed under 0τ\int _0^\tau, at the price of raising polynomial degree on the kernel of MM.
  4. (Products.) p1eλ1τp2eλ2τ=p1p2e(λ1+λ2)τp_1e^{\lambda _1\tau }\cdot p_2e^{\lambda _2\tau } =p_1p_2\,e^{(\lambda _1+\lambda _2)\tau }, so QE\mathrm {QE} is closed under multiplication, with exponent set closed under addition.

Part (a) is the algebraic core of the Björk–Christensen consistency classification [619], and (d) underlies the exponent-doubling phenomenon in strict finite-dimensional realisations [7].

Proof.(a) B=MB\B '=M\B is a linear constant-coefficient system, so B(τ)=eMτB(0)\B (\tau )=e^{M\tau }\B (0); entries of eMτe^{M\tau } are quasi-exponentials by the Jordan form. By Cayley–Hamilton, χM(τ)\chi _M(\partial _\tau ) annihilates every component of B\B, hence every element of VV; the solution space of χM(τ)v=0\chi _M(\partial _\tau )v=0 is exactly the stated quasi-exponential space. Conversely, differentiation maps each complete chain into itself because τ(τkeλτ)=(kτk1+λτk)eλτ\partial _\tau (\tau ^ke^{\lambda \tau })=(k\tau ^{k-1}+\lambda \tau ^k)e^{\lambda \tau }; downward closure is essential (for example, span{τeτ}\operatorname {span}\{\tau e^{-\tau }\} is not invariant). (b) Standard real Jordan theory. For (4): 1\one and JJ commute and J2=1J^2=-\one, so eCτ=eμτeωτJe^{C\tau }=e^{\mu \tau }e^{\omega \tau J}, and splitting the series of eωτJe^{\omega \tau J} into even and odd powers gives cos(ωτ)1+sin(ωτ)J=R(ωτ)\cos (\omega \tau )\one +\sin (\omega \tau )J=R(\omega \tau ). (c) Termwise integration of the exponential series; the two displayed cases are the semisimple-invertible and nilpotent extremes and combine by primary decomposition and direct sum. (d) Immediate.

Lemma 2.4 (Spanning == controllability) . span{B(τ):τ0}=span{MkB(0):k0}\operatorname {span}\{\B (\tau ):\tau \ge 0\}=\operatorname {span}\{M^k\B (0):k\ge 0\} (the Krylov space of the pair (M,B(0))(M,\B (0))). Hence the curve family spans Rn\R ^n iff (M,B(0))(M,\B (0)) is controllable; otherwise the model reduces to the Krylov subspace, which is the minimal realisation.

Proof.τB(τ)\tau \mapsto \B (\tau ) is analytic; its span equals the span of all derivatives at 00, which is the Krylov space, an MM-invariant subspace containing B(0)\B (0) and contained in any such.

Remark 2.5 (Complex spectrum is not an extension) . Theorem 2.3 makes the conceptual point of this whole program precise: the class forced by shift-invariance has exponents ranging over C\C with no further restriction. Real-eigenvalue bases (Nelson–Siegel [37], Svensson, exponential factor models) are the real slice; the precession blocks (4) are the rest of a class that was always inside the arbitrage-free theory. The eigenmodes, being Ime(1/κ+iωn)θ\operatorname {Im}e^{(-1/\kappa +i\omega _n)\theta } up to normalisation, sit in the complex slice. Complex spectrum is only a compact representation of real sine–cosine factor pairs; it does not make rates or security values complex-valued.

2.4Arbitrage-free affine realisations

The class has now been described by the shapes it admits and the drift it requires; what remains is to say which finite-dimensional models belong to it. The following standing assumption fixes the realisations against which the model will be measured.

Assumption 2.6. The curve is rt(τ)=φt(τ)+B(τ)Xtr_t(\tau )=\varphi _t(\tau )+\B (\tau )^\top \X _t with B,XtRn\B ,\X _t\in \R ^n, where φ\varphi is deterministic, tφtt\mapsto \varphi _t is C1C^1 into HwH_w, and tφtt\mapsto \varphi _t is continuous into D(τ)D(\partial _\tau ) equipped with its graph norm. Moreover B=MB\B '=M\B with (M,B(0))(M,\B (0)) controllable (Lemma 2.4). The factors follow dXt=KXtdt+ΣtdWtd\X _t=K\X _t\,dt+\Sigma _t\,d\W _t with a dd-dimensional Brownian motion and a deterministic, locally continuous ΣtRn×d\Sigma _t\in \R ^{n\times d}; write Ct:=ΣtΣtC_t:=\Sigma _t\Sigma _t^\top. The realisation is required to be consistent: (3) holds for every initial factor state X0=xRn\X _0=x\in \R ^n, so the drift identity is an identity in (x,τ)(x,\tau ), not merely a property of one realised path. (For the infinite-dimensional analytic background to this finite-dimensional setting, see [815].)

Proposition 2.7 (Characterisation) . Under Assumption 2.6, the model is consistent — (3) holds for every initial state — if and only if

(5)K=Mandφ˙t(τ)=φt(τ)+qt(τ),qt(τ):=B(τ)CtI(τ),\begin{equation}\label {eq:KM} K=M^\top \qquad \text {and}\qquad \dot \varphi _t(\tau )=\varphi _t'(\tau )+q_t(\tau ),\qquad q_t(\tau ):=\B (\tau )^\top C_t\,\Iv (\tau ), \end{equation}
with I\Iv as in Theorem 2.3(c); when MM is invertible, qt(τ)=B(τ)CtM1(B(τ)B(0))q_t(\tau )=\B (\tau )^\top C_tM^{-1}(\B (\tau )-\B (0)). The transport equation for φ\varphi has the explicit solution
(6)φt(τ)=φ0(τ+t)+0tqs(τ+ts)ds.\begin{equation}\label {eq:transport} \varphi _t(\tau )=\varphi _0(\tau +t)+\int _0^t q_s(\tau +t-s)\,ds. \end{equation}

Proof.Volatility matching in (2) gives σt(τ)=B(τ)Σt\sigma _t(\tau )=\B (\tau )^\top \Sigma _t, whence

αt(τ)=B(τ)Σt0τΣtB(u)du=B(τ)CtI(τ)=qt(τ).\alpha _t(\tau )=\B (\tau )^\top \Sigma _t\int _0^\tau \Sigma _t^\top \B (u)\,du =\B (\tau )^\top C_t\Iv (\tau )=q_t(\tau ).
The model’s actual drift is φ˙t(τ)+B(τ)KXt\dot \varphi _t(\tau )+\B (\tau )^\top K\X _t, while (2) requires
τrt(τ)+αt(τ)=φt(τ)+B(τ)MXt+qt(τ),\partial _\tau r_t(\tau )+\alpha _t(\tau ) =\varphi _t'(\tau )+\B (\tau )^\top M^\top \X _t+q_t(\tau ),
using τ(BX)=(MB)X=BMX\partial _\tau (\B ^\top \X )=(M\B )^\top \X =\B ^\top M^\top \X. Now equate the two for every initial state and all τ\tau. (At t=0t=0 the state is X0=x\X _0=x; at t>0t>0 one has Xt=eKtx+0teK(ts)ΣsdWs\X _t=e^{Kt}x+\int _0^te^{K(t-s)}\Sigma _s\,d\W _s with eKte^{Kt} invertible, so for each fixed noise path Xt\X _t still sweeps all of Rn\R ^n as xx does. Consistency therefore makes the identity hold for every xRnx\in \R ^n.) The X\X-linear parts give B(τ)(KM)=0\B (\tau )^\top (K-M^\top )=0 for all τ\tau, hence K=MK=M^\top by Lemma 2.4; the deterministic parts give the transport equation. For (6), set gt(x):=φt(xt)g_t(x):=\varphi _t(x-t); then g˙t(x)=φ˙tφt=qt(xt)\dot g_t(x)=\dot \varphi _t-\varphi _t'=q_t(x-t), integrate, and substitute back. Note qtq_t must be deterministic for φ\varphi to absorb it, which is where deterministic Σt\Sigma _t enters; a state-dependent Σ\Sigma exits the class (cf. [35] for the framework; §6.1 constructs the affine relaxation).

Remark 2.8 (Support versus consistency; a counterexample) . The quantifier in Proposition 2.7 matters. If (3) is required only along the realised process, the X\X-linear identity is tested only on the support of Xt\X _t, and controllability of (M,B(0))(M,\B (0)) does not make that support full. Take

B(τ)=(eτe2τ),M=diag(1,2),Σ=(σ0),K=diag(1,7),X0=0.\B (\tau )=\begin {pmatrix}e^{-\tau }\\ e^{-2\tau }\end {pmatrix},\quad M=\operatorname {diag}(-1,-2),\quad \Sigma =\begin {pmatrix}\sigma \\0\end {pmatrix},\quad K=\operatorname {diag}(-1,\,7),\quad \X _0=0 .
Then X2,t0X_{2,t}\equiv 0, so BKX=BX\B ^\top K\X =\B '^\top \X along the support although KMK\neq M^\top; taking q(τ)=σ2(eτe2τ)q(\tau )=\sigma ^2(e^{-\tau }-e^{-2\tau }) and φ\varphi the solution (6) of φ˙t=φt+q\dot \varphi _t=\varphi _t'+q, the pathwise drift condition holds. There are three ways to make the identification K=MK=M^\top rigorous. One may require consistency for every initial state, as in Proposition 2.7 and in the standard finite-dimensional-realisation formulation [619]; one may assume the controllability Gramian of (K,Σ)(K,\Sigma ) is positive definite, which gives full support at every t>0t>0; or one may state the conclusion only on the reachable subspace. All completions constructed in this paper also satisfy the second condition: per block, {Σ-column, KΣ-column}\{\Sigma \text {-column},\ K\Sigma \text {-column}\} spans whenever ωn0\omega _n\neq 0, so for them the pathwise and consistent formulations coincide at positive times.

Remark 2.9 (Ho–Lee benchmark) . n=1n=1, b1b\equiv 1, M=0M=0, Σt=σ\Sigma _t=\sigma: then I(τ)=τ\Iv (\tau )=\tau, q(τ)=σ2τq(\tau )=\sigma ^2\tau, and (6) gives φt(τ)=φ0(τ+t)+σ20t(τ+ts)ds=φ0(τ+t)+σ2(tτ+t22)\varphi _t(\tau )=\varphi _0(\tau +t)+\sigma ^2\int _0^t(\tau +t-s)\,ds =\varphi _0(\tau +t)+\sigma ^2\bigl (t\tau +\frac {t^2}2\bigr ), which is precisely the Ho–Lee forward curve f(t,T)=f(0,T)+σ2t(Tt2)+σWtf(t,T)=f(0,T)+\sigma ^2t\bigl (T-\frac t2\bigr )+\sigma W_t in Musiela coordinates. The zero eigenvalue illustrates Theorem 2.3(c): integration on kerM\ker M raises polynomial degree, and the convexity accumulates quadratically in the deterministic sector. This is an algebraic sanity check on a compact maturity interval (or in a larger state space), not an instance of Assumption 2.6 on the present infinite-horizon HwH_w. Although b1Hwb\equiv 1\in H_w, the convexity q(τ)=σ2τq(\tau )=\sigma ^2\tau and the resulting nonconstant polynomial deterministic sector are not in HwH_w.

Remark 2.10 ( P\Pm versus Q\Q ; essentially affine prices of risk) . (5) constrains the Q\Q-drift. Under P\Pm,

dXt=(MXt+Σtγt)dt+ΣtdWtP.d\X _t=(M^\top \X _t+\Sigma _t\gamma _t)\,dt+\Sigma _t\,d\W _t^\Pm .
If γ\gamma is constant (completely affine), the P\Pm- and Q\Q-drift matrices coincide, although their deterministic drift intercepts may differ, and every spectral statement below applies to historical dynamics as well. If γt=γ0+Γ1Xt\gamma _t=\gamma _0+\Gamma _1\X _t (essentially affine, empirically the relevant case [17]), then
KtP=M+ΣtΓ1.K_t^\Pm =M^\top +\Sigma _t\Gamma _1.
When ΣtΣ\Sigma _t\equiv \Sigma is constant this is a fixed matrix KP=M+ΣΓ1K^\Pm =M^\top +\Sigma \Gamma _1, and the tests below restrict the distortion ΣΓ1\Sigma \Gamma _1 (and Γ1\Gamma _1 only to the extent that it is identified through Σ\Sigma). This matters because the source model is estimated under P\Pm [13].

Remark 2.11 (Strict realisations and exponent doubling) . If one additionally demands that φt\varphi _t itself stay in a finite-dimensional family (a strict finite-dimensional realisation in the sense of [7]), then by Theorem 2.3(d) the family must contain the products entering qq: exponents close under addition. For complex pairs λj±iωj-\lambda _j\pm i\omega _j this generates beat frequencies ωj±ωk\omega _j\pm \omega _k at decay λj+λk\lambda _j+\lambda _k: convexity lives at sums and differences of the basis frequencies. Because integration also introduces a zero-exponent term, qq can retain the original exponents as well as their pairwise sums. On the model’s lattice ωn=nπ/θ\omega _n=n\pi /\theta ^* the beat frequencies remain on the lattice, although their decay exponents need not coincide with those of the original loadings. This is a small structural felicity of the equally spaced spectrum.

The yardstick is assembled: the shapes the class admits, the drift it requires, and the realisations that satisfy both. What remains is to place the model against it.

3The cylindrical SPDE, rigorously

The model enters here, and so does the reason the comparison cannot be made pointwise: under cylindrical noise the field is too rough for the drift condition to be posed maturity-by-maturity. This section makes both statements exact — the model well-posed, the pointwise route closed — which is what forces the diagnosis onto finite-dimensional invariant subspaces, where the next section conducts it.

3.1Model and spectral data

Throughout, θ>0\theta ^*>0, κ>0\kappa >0 and σ0>0\sigma _0>0; these standing assumptions are used from here on without further mention. They are load-bearing rather than cosmetic. With κ<0\kappa <0 the sign of every λn\lambda _n reverses and (7) becomes a backward heat equation; with σ0=0\sigma _0=0 there is no noise, and both the variance bound of Proposition 3.3(a) and the nondegeneracy step of Theorem 4.6 use σ0>0\sigma _0>0.

On [0,θ][0,\theta ^*] (after translating θmin\theta _{\min } to 00), the deformation field solves

(7)dXt=[θ+κ2θ2]=:A~Xtdt+σ0dBt,Xt(0)=Xt(θ)=0,\begin{equation}\label {eq:contspde} dX_t=\underbrace {\Bigl [\partial _\theta +\frac \kappa 2\partial _\theta ^2\Bigr ]}_{=:\widetilde A} X_t\,dt+\sigma _0\,d\mathcal B_t,\qquad X_t(0)=X_t(\theta ^*)=0, \end{equation}

where B\mathcal B is a cylindrical Brownian motion on H=L2([0,θ],e2θ/κdθ)H=L^2([0,\theta ^*],e^{2\theta /\kappa }d\theta ): a family of centred Gaussian random functionals with E[Bt(ϕ)Bs(ψ)]=(ts)ϕ,ψH\E [\mathcal B_t(\phi )\mathcal B_s(\psi )]=(t\wedge s)\langle \phi ,\psi \rangle _H [15]. Two objects must be kept apart throughout: the formal differential expression A~:=θ+κ2θ2\widetilde A:=\partial _\theta +\frac \kappa 2\partial _\theta ^2, which acts on any smooth function, and its closed realization AA in HH on the Dirichlet domain D(A)={hH2:h(0)=h(θ)=0}D(A)=\{h\in H^2:h(0)=h(\theta ^*)=0\}, which generates the semigroup and the mild solution. The distinction is not pedantry — it is exactly where the model’s difficulty lives, since the shift-invariant envelope of §4 leaves D(A)D(A) while remaining inside the domain of A~\widetilde A. The closed operator AA has orthonormal eigenbasis

(8)Aen=λnen,en(θ)=2θsin(ωnθ)eθ/κ,ωn=nπθ,λn=12κ(1+κ2ωn2),\begin{equation}\label {eq:eigen} Ae_n=-\lambda _ne_n,\qquad e_n(\theta )=\sqrt {\tfrac 2{\theta ^*}}\sin (\omega _n\theta )e^{-\theta /\kappa },\qquad \omega _n=\frac {n\pi }{\theta ^*},\qquad \lambda _n=\frac 1{2\kappa }\bigl (1+\kappa ^2\omega _n^2\bigr ), \end{equation}

and coordinates xn(t)=Xt,enHx_n(t)=\langle X_t,e_n\rangle _H are independent OU processes dxn=λnxndt+σ0dWtndx_n=-\lambda _nx_n\,dt+\sigma _0\,dW_t^n.

Proposition 3.1 (Symbol) . For zCz\in \C, A~ezθ=p(z)ezθ\widetilde Ae^{z\theta }=p(z)e^{z\theta } with p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2. This is an identity for the formal expression: apart from the sine combinations selected below, these characters are not in D(A)D(A). The map zp(z)z\mapsto p(z) is real-valued exactly on R{Rez=1/κ}\R \cup \{\operatorname {Re}z=-1/\kappa \}; on the critical line 1κ+iω-\frac 1\kappa +i\omega it takes the value λ(ω)=1+κ2ω22κ-\lambda (\omega )=-\frac {1+\kappa ^2\omega ^2}{2\kappa }. The closed Dirichlet operator has the real spectrum spec(A)={λn:n1}\operatorname {spec}(A)=\{-\lambda _n:n\ge 1\}. For each operator eigenvalue λn-\lambda _n, the spatial characteristic equation p(z)=λnp(z)=-\lambda _n has the conjugate roots 1/κ±iωn-1/\kappa \pm i\omega _n. These characteristic exponents lie on the critical line, the axis of symmetry of the parabola pp; equivalently, they form the spectrum of the maturity-generator block MnM_n introduced in Proposition 4.1.

Proof.Termwise, A~ezθ=(z+κ2z2)ezθ=p(z)ezθ\widetilde Ae^{z\theta }=(z+\frac \kappa 2z^2)e^{z\theta }=p(z)e^{z\theta }. For the reality locus write z=x+iyz=x+iy: Imp(z)=y+κ22xy=y(1+κx)\operatorname {Im}p(z)=y+\frac \kappa 2\cdot 2xy=y(1+\kappa x), which vanishes iff y=0y=0 or x=1/κx=-1/\kappa. Centering on the critical line, z=1κ+wz=-\frac 1\kappa +w gives

p(1κ+w)=1κ+w+κ2(1κ22wκ+w2)=12κ+κ2w2,p\bigl (-\tfrac 1\kappa +w\bigr ) =-\tfrac 1\kappa +w+\tfrac \kappa 2\Bigl (\tfrac 1{\kappa ^2}-\tfrac {2w}\kappa +w^2\Bigr ) =-\tfrac 1{2\kappa }+\tfrac \kappa 2w^2,
even in ww: the line is the parabola’s axis of symmetry. At w=iωw=i\omega the value is 1+κ2ω22κ=λ(ω)-\frac {1+\kappa ^2\omega ^2}{2\kappa }=-\lambda (\omega ), and p(z)=λnp(z)=-\lambda _n becomes κ2w2=κ2ωn2\frac \kappa 2w^2=-\frac \kappa 2\omega _n^2, i.e. w=±iωnw=\pm i\omega _n: the conjugate pair 1κ±iωn-\frac 1\kappa \pm i\omega _n. The Dirichlet conditions select from each root pair the combination Ime(1/κ+iω)θeθ/κsinωθ\operatorname {Im}e^{(-1/\kappa +i\omega )\theta }\propto e^{-\theta /\kappa }\sin \omega \theta vanishing at 00, and vanishing at θ\theta ^* quantises ω\omega to ωn=nπ/θ\omega _n=n\pi /\theta ^* — which is (8).

This is the reason the eigenfunctions are damped sines with a common damping rate. The imaginary part of pp vanishes on the critical line, so both members of each conjugate pair — sine and cosine alike — are formal eigenfunctions of A~\widetilde A with the same real eigenvalue; only the sine combination satisfies the Dirichlet conditions and so lies in D(A)D(A). That observation does the heavy lifting in §4.

3.2Well-posedness under cylindrical noise

Before the model can be compared with anything it has to exist as a function-valued process, and under cylindrical noise that is not automatic. The operator that secures it is the one that will later break the drift condition.

Proposition 3.2 (Function-valued solutions) . For deterministic X0HX_0\in H, the mild solution

Xt=etAX0+σ00te(ts)AdBsX_t=e^{tA}X_0+\sigma _0\int _0^te^{(t-s)A}\,d\mathcal B_s
of (7) is a well-defined HH-valued Gaussian process with a continuous modification, and the stationary variance VarX(θ)=σ02nen(θ)22λn\operatorname {Var}X_\infty (\theta )=\sigma _0^2\sum _n\frac {e_n(\theta )^2}{2\lambda _n} is finite pointwise and in HH. The second-order term is essential: with the shift generator alone, the semigroup is not Hilbert–Schmidt-improving and the stochastic convolution with cylindrical noise has no HH-valued version [15]. (This is a different operator, not the singular substitution κ=0\kappa =0 in the eigenfunctions (8).) For an arbitrary HH-valued initial condition independent of the future noise, the same existence and path-continuity conclusions hold, but the solution need not be Gaussian.

Proof.Diagonalise. From (8), esAen=eλnsene^{sA}e_n=e^{-\lambda _ns}e_n, so the semigroup is Hilbert–Schmidt on HH for every s>0s>0, with esAHS2=ne2λns\|e^{sA}\|_{\mathrm {HS}}^2=\sum _ne^{-2\lambda _ns} and

0tesAHS2ds=n1e2λnt2λn12nλn1<.\int _0^t\|e^{sA}\|_{\mathrm {HS}}^2\,ds =\sum _n\frac {1-e^{-2\lambda _nt}}{2\lambda _n} \le \frac 12\sum _n\lambda _n^{-1}<\infty .
By the theory of linear equations with additive noise [15, Ch. 5], the stochastic convolution is therefore a well-defined centred HH-valued Gaussian process with trace-class covariance Qt=σ02n1e2λnt2λnenenQ_t=\sigma _0^2\sum _n\frac {1-e^{-2\lambda _nt}}{2\lambda _n}\, e_n\otimes e_n; adding etAX0e^{tA}X_0 gives the mild solution. It has a continuous HH-valued modification by the factorization method [15, §5.3]: for 0<α<140<\alpha <\frac 14,
0Ts2αesAHS2dsΓ(12α)n(2λn)2α1<,\int _0^Ts^{-2\alpha }\|e^{sA}\|_{\mathrm {HS}}^2\,ds \le \Gamma (1-2\alpha )\sum _n(2\lambda _n)^{2\alpha -1}<\infty ,
since λnn2\lambda _n\asymp n^2 and 2(2α1)<12(2\alpha -1)<-1 — the same exponent 14\frac 14 that resurfaces as the temporal Hölder threshold in Proposition 3.3(b). In coordinates the solution is the OU family below (8); the stationary variances σ02/(2λn)\sigma _0^2/(2\lambda _n) are summable, and supθen(θ)22/θ\sup _\theta e_n(\theta )^2\le 2/\theta ^* makes σ02nen(θ)2/(2λn)\sigma _0^2\sum _ne_n(\theta )^2/(2\lambda _n) converge uniformly on [0,θ][0,\theta ^*]: the stationary field exists pointwise and in HH.

For the pure shift, drop the diffusion term. The generator θ\partial _\theta (a first-order operator admits one endpoint condition; take the one at θ\theta ^*) generates the killed shift (Tsϕ)(θ)=ϕ(θ+s)1{θ+sθ}(T_s\phi )(\theta )=\phi (\theta +s)\one _{\{\theta +s\le \theta ^*\}}. In H=L2(e2θ/κdθ)H=L^2(e^{2\theta /\kappa }d\theta ) its adjoint is (Tsψ)(θ)=e2s/κψ(θs)1{θs}(T_s^*\psi )(\theta )=e^{-2s/\kappa }\psi (\theta -s)\one _{\{\theta \ge s\}}, so TsTsT_sT_s^* is multiplication by e2s/κ1[0,θs]e^{-2s/\kappa }\one _{[0,\theta ^*-s]}, a strictly positive multiple of a projection with infinite-dimensional range. Hence TsHS2=tr(TsTs)=\|T_s\|_{\mathrm {HS}}^2=\operatorname {tr}(T_sT_s^*)=\infty for every s<θs<\theta ^*: no smoothing, no Hilbert–Schmidt improvement. The would-be covariance of the stochastic convolution is multiplication by gt(θ)=σ02κ2(1e2(t(θθ))/κ)g_t(\theta )=\sigma _0^2\frac \kappa 2\bigl (1-e^{-2(t\wedge (\theta ^*-\theta ))/\kappa }\bigr ), which is bounded below on sets of positive measure. A multiplication operator with such a multiplier has infinite trace, since its quadratic form dominates a positive multiple of an infinite-rank projection. No HH-valued Gaussian vector has this covariance, so the convolution admits no HH-valued version [15, Ch. 5]: transported without smoothing, cylindrical noise stays cylindrical.

So the local-deformation operator κ2θ2\frac \kappa 2\partial _\theta ^2 is what makes “one source of randomness per maturity” mathematically possible at all. The same operator will turn out to be exactly what breaks the drift condition (Theorem 4.3); that is the precise form of the tension in [13].

3.3Pointwise regularity: forward rates are not semimartingales

Existence in HH does not make individual forward rates tractable. The next result closes the pointwise route: at a fixed maturity the rate is too rough for the drift condition of Lemma 2.1 to be posed at all, which is what sends the comparison onto finite-dimensional invariant subspaces.

Proposition 3.3. Let XX solve (7) either from its stationary law or from a deterministic X0HX_0\in H, and fix θ(0,θ)\theta \in (0,\theta ^*). In the stationary case let I=[0,T]I=[0,T], while in the deterministic-initial case let I=[t,t+T](0,)I=[t_*,t_*+T]\subset (0,\infty ). Then:

  1. uniformly for t,t+hIt,t+h\in I and sufficiently small h>0h>0, there are 0<cθ,ICθ,I<0<c_{\theta ,I}\le C_{\theta ,I}<\infty such that

    cθ,IhVar(Xt+h(θ)Xt(θ))Cθ,Ih;c_{\theta ,I}\sqrt h \le \operatorname {Var}\bigl (X_{t+h}(\theta )-X_t(\theta )\bigr ) \le C_{\theta ,I}\sqrt h;
  2. tXt(θ)t\mapsto X_t(\theta ) has a modification that is locally Hölder of every order <14<\frac 14 on II;
  3. along the uniform partitions of II into mm subintervals, the quadratic-variation sums QmQ_m satisfy EQmm\E Q_m\asymp \sqrt m\to \infty and, for all sufficiently large mm,

    P(QmcIm)112\Pm \bigl (Q_m\ge c_I\sqrt m\bigr )\ge \frac 1{12}
    for some cI>0c_I>0. Hence (Qm)(Q_m) is not tight and cannot converge in probability to a finite limit; in particular, tXt(θ)t\mapsto X_t(\theta ) is not a semimartingale.

Cf. [4140] for the analogous statements for the stochastic heat equation, including the finiteness of the quartic variation, of which (a)–(c) are the drift-augmented transcription.

Proof.(a) Var(Xt+h(θ)Xt(θ))=σ02nλn1(1eλnh)en(θ)2\operatorname {Var}(X_{t+h}(\theta )-X_t(\theta )) =\sigma _0^2\sum _n\lambda _n^{-1}\bigl (1-e^{-\lambda _nh}\bigr )e_n(\theta )^2 by the OU covariances. With en(θ)2=2θsin2(ωnθ)e2θ/κ2θe_n(\theta )^2=\frac 2{\theta ^*}\sin ^2(\omega _n\theta )e^{-2\theta /\kappa }\le \frac 2{\theta ^*} and λnn2\lambda _n\asymp n^2, split at n=h1/2n_*=\lceil h^{-1/2}\rceil: the sum is nnh+n>nn2h\lesssim \sum _{n\le n_*}h+\sum _{n>n_*}n^{-2}\asymp \sqrt h. For the lower bound, sin2(nπθ/θ)\sin ^2(n\pi \theta /\theta ^*) has positive lower density bounded away from zero (for irrational θ/θ\theta /\theta ^* by Weyl equidistribution with mean 12\frac 12; for rational p/qp/q the values are qq-periodic and vanish only when qnq\mid n), so a positive-density subsequence contributes h\gtrsim \sqrt h. (b) Gaussianity plus (a) gives E|Xt+hXt|2pCphp/2\E |X_{t+h}-X_t|^{2p}\le C_ph^{p/2} and Kolmogorov’s criterion yields Hölder <14<\frac 14. (c) EQm=iVar(ΔiX)mT/m=Tm\E Q_m=\sum _i\operatorname {Var}(\Delta _iX)\asymp m\cdot \sqrt {T/m}=\sqrt {Tm}. For jointly Gaussian increments, VarQm=2i,jCov(Δi,Δj)22(iVarΔi)2=2(EQm)2\operatorname {Var}Q_m=2\sum _{i,j}\operatorname {Cov}(\Delta _i,\Delta _j)^2 \le 2\bigl (\sum _i\operatorname {Var}\Delta _i\bigr )^2=2(\E Q_m)^2, so EQm23(EQm)2\E Q_m^2\le 3(\E Q_m)^2 and Paley–Zygmund gives P(Qm12EQm)(EQm)24EQm2112\Pm \bigl (Q_m\ge \tfrac 12\E Q_m\bigr )\ge \frac {(\E Q_m)^2}{4\E Q_m^2}\ge \frac 1{12}. A continuous semimartingale has QmQ_m converging in probability to its finite quadratic variation and hence has a tight sequence of quadratic-variation sums. Here, for every R<R<\infty and all sufficiently large mm,

P(Qm>R)P(Qm12EQm)112,\Pm (Q_m>R)\ge \Pm \left (Q_m\ge \tfrac 12\E Q_m\right )\ge \frac 1{12},
because EQm\E Q_m\to \infty. Thus (Qm)(Q_m) is not tight, a contradiction.

Deterministic initial data. Write Xt=etAX0+ZtX_t=e^{tA}X_0+Z_t with ZZ the stochastic convolution, which for t>0t>0 is defined pointwise (etAe^{tA} is analytic, so etAX0e^{tA}X_0 is smooth and deterministic). Only ZZ is random, and its modal variances are vn(t)=σ022λn(1e2λnt)v_n(t)=\frac {\sigma _0^2}{2\lambda _n}(1-e^{-2\lambda _nt}), giving the exact increment law

Var(Zt+h(θ)Zt(θ))=nen(θ)2[vn(t)(1eλnh)2+σ022λn(1e2λnh)].\operatorname {Var}\bigl (Z_{t+h}(\theta )-Z_t(\theta )\bigr ) =\sum _n e_n(\theta )^2\Bigl [v_n(t)\bigl (1-e^{-\lambda _nh}\bigr )^2 +\frac {\sigma _0^2}{2\lambda _n}\bigl (1-e^{-2\lambda _nh}\bigr )\Bigr ].
The second bracket alone reproduces the two-sided h\sqrt h estimate of (a), uniformly for tIt\in I, by the same split at n=h1/2n_*=\lceil h^{-1/2}\rceil. The first is nonnegative and bounded by σ022λn(1eλnh)2\frac {\sigma _0^2}{2\lambda _n}(1-e^{-\lambda _nh})^2, which the same split bounds by O(h)O(\sqrt h). Thus the preceding Gaussian argument applies to ZZ on every I=[t,t+T](0,)I=[t_*,t_*+T]\subset (0,\infty ): if QmZQ_m^Z denotes its quadratic-variation sum, then EQmZm\E Q_m^Z\asymp \sqrt m and
P(QmZ12EQmZ)112.\Pm \left (Q_m^Z\ge \frac 12\E Q_m^Z\right )\ge \frac 1{12}.
Put Dt:=(etAX0)(θ)D_t:=(e^{tA}X_0)(\theta ). Analytic smoothing makes DD continuously differentiable with bounded derivative on II, and therefore its quadratic-variation sum satisfies
QmD:=i(ΔiD)2T2msupsI|Ds|2=O(m1).Q_m^D:=\sum _i(\Delta _iD)^2 \le \frac {T^2}{m}\sup _{s\in I}|D_s'|^2=O(m^{-1}).
Regarding the increment vectors as elements of Rm\R ^m, the triangle inequality gives
QmXQmZQmD.\sqrt {Q_m^X}\ge \sqrt {Q_m^Z}-\sqrt {Q_m^D}.
Consequently, on the preceding Paley–Zygmund event and for all sufficiently large mm, QmX14QmZmQ_m^X\ge \frac 14Q_m^Z\gtrsim \sqrt m. Moreover, since the increments of ZZ are centred and DD is deterministic,
EQmX=EQmZ+QmDm.\E Q_m^X=\E Q_m^Z+Q_m^D\asymp \sqrt m.
This proves (b)–(c) for deterministic initial data without requiring a pointwise value of X0X_0 at time zero.

Remark 3.4 (Where the drift condition can live) . Proposition 3.3 means the pointwise HJM computation of Lemma 2.1 is not even well-posed for (7): individual forward rates are not Itô processes. Pairings Xt,ϕ\langle X_t,\phi \rangle with ϕD(A)\phi \in D(A^*) are semimartingales (weak formulation). On the finite maturity interval the bond integral X0uX(θ)dθX\mapsto \int _0^uX(\theta )\,d\theta is a bounded functional on H=L2([0,θ],e2θ/κdθ)H=L^2([0,\theta ^*],e^{2\theta /\kappa }d\theta ), with HH-representer e2θ/κ1[0,u](θ)e^{-2\theta /\kappa }\mathbf 1_{[0,u]}(\theta ). This representer is not in D(A)D(A^*): under the unitary conjugacy of Proposition 4.10 it becomes eθ/κ1[0,u]e^{-\theta /\kappa }\mathbf 1_{[0,u]}, which jumps at uu and so is not even H1H^1. That alone does not decide the question that matters — whether traded-bond processes are semimartingales under the fully infinite cylindrical dynamics — which remains open (Proposition 4.10 and the discussion closing §4). The requirement is not special to this model: a state space in which bond prices are to be Itô processes must either make the maturity functionals that define them semimartingale pairings or carry the traded coordinates explicitly. That is the division of labour between the two spaces used here: the arbitrage-free class of §2 lives in HwH_w, where point evaluation is continuous, while the SPDE itself is posed in HH. At every finite truncation the bond processes are ordinary Itô semimartingales, and Theorem 4.6 below constructs an explicit finite-bond witness. The random-field literature [332239] handles this with spatially correlated noise, for which a drift condition in terms of the covariance kernel exists; white-in-maturity noise is exactly the singular case. The rigorous route is therefore the one taken in §§45: diagnose and repair on finite-dimensional invariant subspaces, then control the limit — where the singularity resurfaces in a precisely quantified form (Theorem 5.2).

4The obstruction: symbol, witness, and magnitude

The comparison between the class of §2 and the model of §3 now runs at three increasing levels of concreteness. In factor coordinates, a symbol computation identifies exactly which dynamics the class tolerates and shows that none of the model’s blocks is among them. In traded securities, the failure becomes an explicit arbitrage portfolio (§4.4). In magnitude, a normalized quotient shows that refinement does not attenuate it (§4.5). §4.6 asks what survives in the infinite model, and §4.7 what changes when the silent coordinates are given noise of their own: the impossibility becomes a price.

4.1The invariant envelope doubles

The comparison needs a shift-invariant family, and the model’s sine modes do not form one. The first step is therefore to find the smallest invariant space that contains them.

Proposition 4.1 (Envelope doubling) . Let

Vn:=span{eθ/κsinωnθ,eθ/κcosωnθ}.V_n:=\operatorname {span}\{e^{-\theta /\kappa }\sin \omega _n\theta ,\, e^{-\theta /\kappa }\cos \omega _n\theta \}.
Then VnV_n is the minimal θ\partial _\theta-invariant subspace containing ene_n, with generating matrix
(9)Mn=(1/κωnωn1/κ),specMn={1κ±iωn},detMn=1κ2+ωn2.\begin{equation}\label {eq:Mn} M_n=\begin {pmatrix}-1/\kappa &\omega _n\\-\omega _n&-1/\kappa \end {pmatrix},\qquad \operatorname {spec}M_n=\Bigl \{-\frac 1\kappa \pm i\omega _n\Bigr \},\qquad \det M_n=\frac 1{\kappa ^2}+\omega _n^2. \end{equation}
Consequently the minimal shift-invariant envelope of the NN-mode truncation is
span{e1,,eN}nNVn,\operatorname {span}\{e_1,\dots ,e_N\}\longmapsto \bigoplus _{n\le N}V_n,
of dimension 2N2N. The cosine partners violate the Dirichlet conditions (cos-modes are nonzero at θ=0\theta =0), which is why the model’s state space itself is not shift-invariant.

Economically, the cosine partner is not an additional source of randomness. It is the deterministic roll-down direction generated as a sine loading ages; omitting it prevents the finite state from representing maturity transport.

Proof.Differentiating the pair of characters,

θeθ/κ(sinωnθcosωnθ)=eθ/κ(1/κωnωn1/κ)(sinωnθcosωnθ),\partial _\theta \,e^{-\theta /\kappa } \begin {pmatrix}\sin \omega _n\theta \\ \cos \omega _n\theta \end {pmatrix} =e^{-\theta /\kappa } \begin {pmatrix}-1/\kappa& \omega _n\\-\omega _n&-1/\kappa \end {pmatrix} \begin {pmatrix}\sin \omega _n\theta \\ \cos \omega _n\theta \end {pmatrix},
which is (9). VnV_n is 2-dimensional and invariant; no 1-dimensional invariant subspace contains ene_n because a 1-dimensional invariant subspace is spanned by a real eigenvector of MnM_n, and specMnR=\operatorname {spec}M_n\cap \R =\emptyset. Distinct nn give linearly independent trigonometric characters after dividing by the common exponential, so the envelopes sum directly.

The envelope is the object on which the comparison is made from here on. That it leaves the Dirichlet domain is the first thing the next subsection has to settle.

4.2The generator comparison is exact on the envelope

The domain distinction of §3 decides which object the comparison is about. The cosine partners adjoined in Proposition 4.1 violate the Dirichlet conditions and do not belong to D(A)D(A); on the envelope the relevant operator is therefore the formal expression A~=θ+κ2θ2\widetilde A=\partial _\theta +\frac \kappa 2\partial _\theta ^2, acting on the analytic (quasi-exponential) extensions. The obstruction proved here is therefore a tangency/symbol statement, in the spirit of the invariant-manifold calculus of [21]: the formal symbol acts one way on the invariant envelope and no-arbitrage transport demands another. It concerns the formal expression, not an invariant subspace of the closed Dirichlet operator. The sine truncation itself is invariant under AA; its minimal shift-invariant envelope leaves D(A)D(A) (Proposition 4.1), and the completions built on that envelope are finite-dimensional models in their own right.

Proposition 4.2 (Induced factor drifts: the symbol of a curve dynamics) . Let VV be any finite-dimensional shift-invariant space with basis B\B, B=MB\B '=M\B, and consider curve dynamics d(BXt)=(GBXt)dt+(noise)d(\B ^\top \X _t)=(G\,\B ^\top \X _t)\,dt+\text {(noise)} driven by a generator GG leaving VV invariant.

  1. (Any constant-coefficient generator.) Let G=k=0dakθkG=\sum _{k=0}^{d}a_k\partial _\theta ^k with symbol p(z)=k=0dakzkp(z)=\sum _{k=0}^da_kz^k. Then VV is GG-invariant and the induced factor drift matrix is

    Kdef=p(M)=p(M).K^{\mathrm {def}}=p(M)^\top =p(M^\top ).
    The deformation generator of this paper is the case G=A~=θ+κ2θ2G=\widetilde A=\partial _\theta +\frac \kappa 2\partial _\theta ^2 (the model’s formal expression, per the caveat above), with p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2.
  2. If G=τG=\partial _\tau with the affine inhomogeneity of (2) (arbitrage-free), the required factor drift is KNA=MK^{\mathrm {NA}}=M^\top (Proposition 2.7).
  3. On the model’s blocks (9), p(Mn)=λn12p(M_n)=-\lambda _n\one _2 exactly, consistent with Proposition 3.1: the symbol is real on the critical line, so AA acts isotropically there — decay λn\lambda _n, no rotation.

Proof.(a) B=MB\B '=M\B iterates to B(k)=MkB\B ^{(k)}=M^k\B, so GB=kakB(k)=p(M)BG\B =\sum _ka_k\B ^{(k)}=p(M)\B; in particular VV is GG-invariant. For a curve Bx\B ^\top x, G(Bx)=(p(M)B)x=B(p(M)x)G(\B ^\top x)=(p(M)\B )^\top x=\B ^\top \bigl (p(M)^\top x\bigr ), and since the components of B\B are a basis, coordinate representations are unique: the curve drift GBXtG\,\B ^\top \X _t is carried by the factor drift matrix Kdef=p(M)K^{\mathrm {def}}=p(M)^\top, which equals p(M)p(M^\top ) because transposition fixes polynomials in a single matrix. (b) is Proposition 2.7: under the arbitrage-free dynamics the affine inhomogeneity is absorbed by φ\varphi, and the factor block of τ\partial _\tau is MM^\top. (c) With Mn=1κ1+ωnJM_n=-\frac 1\kappa \one +\omega _nJ and J2=1J^2=-\one, Mn2=(1κ2ωn2)12ωnκJM_n^2=\bigl (\frac 1{\kappa ^2}-\omega _n^2\bigr )\one -\frac {2\omega _n}\kappa J, so

p(Mn)=Mn+κ2Mn2=(1κ+κ2(1κ2ωn2))1+(ωnκ22ωnκ)J=λn1:p(M_n)=M_n+\tfrac \kappa 2M_n^2 =\Bigl (-\tfrac 1\kappa +\tfrac \kappa 2\bigl (\tfrac 1{\kappa ^2}-\omega _n^2\bigr )\Bigr )\one +\bigl (\omega _n-\tfrac \kappa 2\cdot \tfrac {2\omega _n}\kappa \bigr )J =-\lambda _n\one :
the JJ-part cancels identically — the algebraic form of “real symbol on the critical line” (Proposition 3.1): decay λn\lambda _n, no rotation.

Theorem 4.3 (The symbol test; the exact obstruction) . With the notation of Proposition 4.2, let VV be a shift-invariant block with generating matrix MM and let the curve dynamics have symbol pp.

  1. (The test, for any symbol.) The dynamics carries the arbitrage-free factor drift on VV — that is, Kdef=KNAK^{\mathrm {def}}=K^{\mathrm {NA}} — if and only if

     mM(z) | p(z)z \boxed {\ m_M(z)\ \big |\ p(z)-z\ }
    where mMm_M is the minimal polynomial of MM. When MM is diagonalisable this says exactly that the symbol must fix the block’s spectrum pointwise, p(λ)=λp(\lambda )=\lambda for every λspecM\lambda \in \operatorname {spec}M; in general p(z)zp(z)-z must vanish at each eigenvalue to the order of its largest Jordan block. Thus consistency of the factor drift on each finite-dimensional shift-invariant block is reduced to one polynomial divisibility; on the envelope nVn\bigoplus _nV_n the induced drift is block-diagonal, so the condition holds there if and only if it holds on every block.
  2. (The instance.) For p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2 the criterion reads mMκ2z2m_M\mid \frac \kappa 2z^2, i.e.

    Kdef=KNAp(M)=MM2=0Vkerθ2={affine curves a+bθ}.K^{\mathrm {def}}=K^{\mathrm {NA}}\iff p(M)=M\iff M^2=0\iff V\subseteq \ker \partial _\theta ^2=\{\text {affine curves }a+b\theta \}.
    Since specM{Rez=1/κ}\operatorname {spec}M\subset \{\operatorname {Re}z=-1/\kappa \} contains no zero eigenvalue, no block of this model passes: the drift condition fails on every genuinely decaying block (μ0\mu \neq 0) and every oscillatory block (ω0\omega \neq 0). The quantitative discrepancy is p(M)M=κ2M2p(M)-M=\frac \kappa 2M^2, i.e. on the spectrum, p(z)z=κ2z2p(z)-z=\frac \kappa 2z^2. In HwH_w the affine sliver is thinner still: since w1w\ge 1 is nondecreasing, 0w=\int _0^\infty w=\infty and a+bθw<\|a+b\theta \|_w<\infty forces b=0b=0, so inside the state space the tolerated class is the constants alone. For the model’s blocks the two induced dynamics are
    Kndef=λn12vsKnNA=Mn=(1/κωnωn1/κ),K_n^{\mathrm {def}}=-\lambda _n\one _2\qquad \text {vs}\qquad K_n^{\mathrm {NA}}=M_n^\top =\begin {pmatrix}-1/\kappa& -\omega _n\\\omega _n&-1/\kappa \end {pmatrix},
    differing in exactly two ways: the decay mismatch κλn=12(1+κ2ωn2)\kappa \lambda _n=\frac 12(1+\kappa ^2\omega _n^2), equal to 11 only if the lattice contains an index satisfying κωn=1\kappa \omega _n=1. Such an index exists precisely when θ/(πκ)N\theta ^*/(\pi \kappa )\in \mathbb N; otherwise θ/(πκ)\theta ^*/(\pi \kappa ) is only the continuous crossing location. The second discrepancy is the missing rotation ±ωn\pm \omega _n. Separately and non-spectrally, the convexity qtq_t of (5) is absent from (7).

Proof.(a) Kdef=p(M)K^{\mathrm {def}}=p(M)^\top and KNA=MK^{\mathrm {NA}}=M^\top; transposing, equality is p(M)=Mp(M)=M, i.e. q(M)=0q(M)=0 for q:=pidq:=p-\mathrm {id}. A polynomial annihilates MM precisely when it is divisible by the minimal polynomial, which is the stated criterion; the spectral form is the standard reading of mMqm_M\mid q (simple roots when MM is diagonalisable, root multiplicities equal to the largest Jordan-block sizes in general). (b) Here q=κ2z2q=\frac \kappa 2z^2, so q(M)=0q(M)=0 reads κ2M2=0\frac \kappa 2M^2=0. On a 2×22\times 2 rotation–decay cell M=μ1+ωJM=\mu \one +\omega J, M2=(μ2ω2)1+2μωJ=0M^2=(\mu ^2-\omega ^2)\one +2\mu \omega J=0 forces μ=ω=0\mu =\omega =0; a nilpotent Jordan cell (0100)\bigl (\begin {smallmatrix}0&1\\0&0\end {smallmatrix}\bigr ) also satisfies M2=0M^2=0 and spans {1,θ}\{1,\theta \}. Since B=M2B\B ''=M^2\B and the components of B\B form a basis, M2=0M^2=0 is equivalent to Vkerθ2V\subseteq \ker \partial _\theta ^2. The displayed block pair is Kndef=p(Mn)=λn12K_n^{\mathrm {def}}=p(M_n)^\top =-\lambda _n\one _2 (Proposition 4.2(c)) against KnNA=MnK_n^{\mathrm {NA}}=M_n^\top (Proposition 2.7); the mismatch ratio κλn=12(1+κ2ωn2)\kappa \lambda _n=\frac 12(1+\kappa ^2\omega _n^2) restates (8).

Remark 4.4 (The obstruction is measure-invariant) . The discrepancy of Theorem 4.3 is not a market price of risk. On the Brownian filtration every equivalent measure change is a Girsanov tilt dWQ=dW+γtdtd\W ^\Q =d\W +\gamma _t\,dt, so it changes the factor drift by Σγt-\Sigma \gamma _t and therefore can move it only within the range of the volatility. With the sine-only loading, rangeΣ\operatorname {range}\Sigma is the sine coordinates, while per block

KndefKnNA=λn12Mn=(1κλnωnωn1κλn)K_n^{\mathrm {def}}-K_n^{\mathrm {NA}} =-\lambda _n\one _2-M_n^\top =\begin {pmatrix}\frac 1\kappa -\lambda _n&\omega _n\\[2pt]-\omega _n&\frac 1\kappa -\lambda _n \end {pmatrix}
has cosine row (ωn, 1κλn)0\bigl (-\omega _n,\ \frac 1\kappa -\lambda _n\bigr )\neq 0: the missing rotation acts on the noiseless coordinate, which no tilt γ\gamma — adapted, state-dependent, or otherwise — can reach. (Even when a matched lattice index nn^* with κωn=1\kappa \omega _{n^*}=1 exists, so the decay entry 1κλn=(κωn1)(κωn+1)2κ\frac 1\kappa -\lambda _n=-\frac {(\kappa \omega _n-1)(\kappa \omega _n+1)}{2\kappa } vanishes, the rotation entry ωn-\omega _{n^*} does not.) The missing convexity is likewise unreachable: qq contains an original-frequency term at decay 1/κ1/\kappa, together with a zero-frequency term and 2ωn2\omega _n beat terms at decay 2/κ2/\kappa (Remark 2.11); the latter components lie outside the sine-only volatility range. Consequently the envelope realisation equipped with the induced dynamics admits no equivalent local martingale measure, for every NN: at each truncation order the verdict is not “wrong Q\Q-drift” but “no Q\Q exists.” This sharpens Remark 2.10: the P\Pm-freedom bought by an essentially affine price of risk is exactly ΣΓ1\Sigma \Gamma _1, the sine rows, and the deviation exits it identically. And it is visible only on the doubled envelope; the cosine partners adjoined in Proposition 4.1 are what expose it. Theorem 4.6 below turns this factor-range statement into an explicit arbitrage using finitely many traded zero-coupon bonds.

4.3Spectral locking and factor autocovariance

Theorem 4.3 was stated for the model. Its characterisation half, Proposition 2.7, has a consequence for every consistent model that is worth recording on its own, because it is testable and the model violates it maximally.

Corollary 4.5 (Spectral locking) . In a consistent arbitrage-free model of Assumption 2.6 (Proposition 2.7), specK=specM\operatorname {spec}K=\operatorname {spec}M with multiplicities. Moreover, if ΣtΣ\Sigma _t\equiv \Sigma is constant with C=ΣΣC=\Sigma \Sigma ^\top, RespecM<0\operatorname {Re}\operatorname {spec}M<0, and the factor process is initialised at (or has relaxed to) its stationary law, then the stationary covariance VV_\infty solves the Lyapunov equation MV+VM+C=0M^\top V_\infty +V_\infty M+C=0 and the stationary autocovariance is

R(h):=Cov(Xt+h,Xt)=eMhV.R(h):=\operatorname {Cov}(\X _{t+h},\X _t)=e^{M^\top h}V_\infty .
On a semisimple complex block with spectrum λ±iω-\lambda \pm i\omega this equals eλhR(ωh)Ve^{-\lambda h}R(\omega h)^\top V_\infty by (4): on every stochastically excited such block, the nonzero covariance entries of its rows are damped sinusoids with the maturity frequency ω\omega and decay rate λ\lambda. On a complex Jordan chain of length m>1m>1 the frequency and the decay rate are the same, but the entries are eλhe^{-\lambda h} times sine–cosine combinations with polynomial coefficients of degree at most m1m-1: it is the pure-sinusoid shape, not the spectral content, that requires semisimplicity. Thus a maturity ripple of wavelength 2π/ω2\pi /\omega corresponds, on that block, to a calendar-time cycle of period 2π/ω2\pi /\omega.

Proof.Proposition 2.7 gives K=MK=M^\top, which is similar to MM, so the Jordan structure — in particular the spectrum with multiplicities — coincides. With constant Σ\Sigma and RespecM<0\operatorname {Re}\operatorname {spec}M<0, the factor OU system dX=MXdt+ΣdWd\X =M^\top \X \,dt+\Sigma \,d\W has stationary law N(0,V)N(0,V_\infty ) with V=0eMsCeMsdsV_\infty =\int _0^\infty e^{M^\top s}Ce^{Ms}\,ds; the integral converges, and

MV+VM=0dds(eMsCeMs)ds=C,M^\top V_\infty +V_\infty M =\int _0^\infty \frac {d}{ds}\bigl (e^{M^\top s}Ce^{Ms}\bigr )\,ds=-C,
which is the Lyapunov equation, uniquely solvable because specMspec(M)=\operatorname {spec}M^\top \cap \operatorname {spec}(-M)=\emptyset. For h0h\ge 0, Xt+h=eMhXt+tt+heM(t+hu)ΣdWu\X _{t+h}=e^{M^\top h}\X _t+\int _t^{t+h}e^{M^\top (t+h-u)}\Sigma \,d\W _u with the integral independent of Ft\mathcal F_t, so under stationarity R(h)=Cov(Xt+h,Xt)=eMhVR(h)=\operatorname {Cov}(\X _{t+h},\X _t)=e^{M^\top h}V_\infty. Work in coordinates adapted to the real Jordan form (the completions’ coordinates already are). On a semisimple cell Mb=λ1+ωJM_b=-\lambda \one +\omega J, (4) gives the block rows eMbh=eλhR(ωh)e^{M_b^\top h}=e^{-\lambda h}R(\omega h)^\top, so for every column jj
R(h)1j=eλh(cos(ωh)(V)1jsin(ωh)(V)2j),R(h)2j=eλh(sin(ωh)(V)1j+cos(ωh)(V)2j),\begin{align*} R(h)_{1j}&=e^{-\lambda h}\bigl (\cos (\omega h)(V_\infty )_{1j}-\sin (\omega h)(V_\infty )_{2j}\bigr ),\\ R(h)_{2j}&=e^{-\lambda h}\bigl (\sin (\omega h)(V_\infty )_{1j}+\cos (\omega h)(V_\infty )_{2j}\bigr ), \end{align*}

i.e. R(h)ij=ρijeλhcos(ωhϕij)R(h)_{ij}=\rho _{ij}\,e^{-\lambda h}\cos (\omega h-\phi _{ij}) with amplitude ρij=((V)1j2+(V)2j2)1/2\rho _{ij}=\bigl ((V_\infty )_{1j}^2+(V_\infty )_{2j}^2\bigr )^{1/2}: every nonvanishing entry in those rows is a damped sinusoid at frequency exactly ω\omega and decay exactly λ\lambda. The block is stochastically excited — some ρij0\rho _{ij}\neq 0 — whenever its rows Σb\Sigma _b of Σ\Sigma are nonzero: the block-diagonal of VV_\infty is then the controllability Gramian 0eMbsΣbΣbeMbsds\int _0^\infty e^{M_b^\top s}\Sigma _b\Sigma _b^\top e^{M_bs}\,ds, positive definite because {v,(λ1ωJ)v}\{v,\,(-\lambda \one -\omega J)v\} spans R2\R ^2 for every v0v\neq 0 when ω0\omega \neq 0 (JvvJv\perp v). For a chain of length mm the real Jordan block is Mb=(1mC)+(N12)M_b=(\one _m\otimes C)+(N\otimes \one _2) with NN the nilpotent shift; the two summands commute, so eMbh=eλhk<mhkk!(N)kR(ωh)e^{M_b^\top h}=e^{-\lambda h}\sum _{k<m}\frac {h^k}{k!}(N^\top )^k\otimes R(\omega h)^\top, which is the stated polynomial-times-sinusoid form. A concrete instance: C=21+ωJC=-2\one +\omega J with ω=1\omega =1, m=2m=2, V=14V_\infty =\one _4 and ΣΣ=(M+M)0\Sigma \Sigma ^\top =-(M^\top +M)\succ 0 satisfies every hypothesis and has entries ±he2hsinh\pm h\,e^{-2h}\sin h, which are not pure sinusoids.

At the reference calibration (κ,θ)=(4,30)(\kappa ,\theta ^*)=(4,30), the required and proposed decay rates already cross between modes 2 and 3, after which the mismatch grows quadratically with mode number. With the essentially-affine caveat of Remark 2.10, this gives a direct restriction on the joint maturity and time spectra. The cylindrical model violates it maximally: its maturity spectrum has constant real part and nonzero imaginary parts; its time spectrum is real with n2n^2-growing magnitude (Figure 1b, Figure 2a).

Figure 1: (a) The model’s first three eigenmodes: damped oscillatory quasi-exponentials with
envelope \(e^{-\theta /\kappa }\) . (b) The two spectra: maturity-domain \(-1/\kappa \pm i\omega _n\) (vertical line) versus the model’s time-domain
OU rates \(-\lambda _n\) (real axis); arrows mark the pairing no-arbitrage would identify — the time spectrum
is the image of the maturity spectrum under the symbol \(p\) , collapsed to the real axis because
the model’s spectral line is the symmetry axis of the parabola. (c) The mismatch ratio \(\kappa \lambda _n\) against
the arbitrage-free requirement (dashed).
Figure 1. (a) The model’s first three eigenmodes: damped oscillatory quasi-exponentials with envelope eθ/κe^{-\theta /\kappa }. (b) The two spectra: maturity-domain 1/κ±iωn-1/\kappa \pm i\omega _n (vertical line) versus the model’s time-domain OU rates λn-\lambda _n (real axis); arrows mark the pairing no-arbitrage would identify — the time spectrum is the image of the maturity spectrum under the symbol pp, collapsed to the real axis because the model’s spectral line is the symmetry axis of the parabola. (c) The mismatch ratio κλn\kappa \lambda _n against the arbitrage-free requirement (dashed).

Remark 4.4 is a statement about factor coordinates. The remainder of the section turns it into two statements one can act on. At every truncation the defect is exposed by a finite panel of traded bonds (§4.4), and its size does not wash out under refinement (§4.5). §4.6 then asks what survives in the infinite model, where the sine system is complete and no coordinate is silent: an energy obstruction does. §4.7 closes by giving the silent coordinates noise of their own, which turns the unreachable drift into a price.

4.4A finite-bond witness

The range defect is not merely a coordinate-level failure. At every finite truncation it can be separated by a finite panel of traded bonds. For the statement, put

bns(τ):=2θeτ/κsin(ωnτ),bnc(τ):=2θeτ/κcos(ωnτ),b_n^s(\tau ):=\sqrt {\frac 2{\theta ^*}}e^{-\tau /\kappa }\sin (\omega _n\tau ), \qquad b_n^c(\tau ):=\sqrt {\frac 2{\theta ^*}}e^{-\tau /\kappa }\cos (\omega _n\tau ),

and define the integrated sine loading and the integrated state-drift defect by

(10)Fn(τ):=0τbns(u)du,Hn(τ):=bns(τ)+λnFn(τ),\begin{equation}\label {eq:FH-bond} F_n(\tau ):=\int _0^\tau b_n^s(u)\,du, \qquad H_n(\tau ):=b_n^s(\tau )+\lambda _nF_n(\tau ), \end{equation}

and write qN(τ):=σ02nNbns(τ)Fn(τ)q^N(\tau ):=\sigma _0^2\sum _{n\le N}b^s_n(\tau )F_n(\tau ) for the truncation’s own convexity, so that 0τqN=12σ02nFn(τ)2\int _0^\tau q^N=\frac 12\sigma _0^2\sum _nF_n(\tau )^2. (This is BCI\B ^\top C\,\Iv of Proposition 2.7 evaluated on the sine-only data, and agrees with the completion’s convexity in Definition 5.1.)

With NN Brownian shocks, N+1N+1 bonds generically leave one instantaneous zero-volatility portfolio. In the inconsistent truncation that portfolio retains nonzero discounted drift. The proof chooses its sign from the observed state and stops before the sign can reverse, turning the rank defect into an admissible arbitrage.

Theorem 4.6 (A finite-bond witness of the obstruction) . Fix N1N\ge 1 and consider the actual NN-sine truncation

(11)rt(τ)=φt(τ)+n=1Nbns(τ)xn,t,dxn,t=λnxn,tdt+σ0dWtn,\begin{equation}\label {eq:sine-truncation-bond} r_t(\tau )=\varphi _t(\tau )+\sum _{n=1}^Nb_n^s(\tau )x_{n,t}, \qquad dx_{n,t}=-\lambda _nx_{n,t}\,dt+\sigma _0\,dW_t^n, \end{equation}
with deterministic initial state and a deterministic, jointly C1C^1 sector φ(t,τ)\varphi (t,\tau ). Let Bt=exp(0trs(0)ds)B_t=\exp (\int _0^tr_s(0)\,ds) and P~(t,T)=P(t,T)/Bt\widetilde P(t,T)=P(t,T)/B_t.

For every nonempty open interval J(0,θ)J\subset (0,\theta ^*), define the ordered simplex

JN+1:={(τ1,,τN+1)JN+1:τ1<<τN+1}.J_\uparrow ^{N+1}:= \{(\tau _1,\ldots ,\tau _{N+1})\in J^{N+1}:\tau _1<\cdots <\tau _{N+1}\}.
An open dense subset of full Lebesgue measure in JN+1J_\uparrow ^{N+1} has the following property. At every deterministic t0>0t_0>0, the fixed-calendar-maturity bonds Tj=t0+τjT_j=t_0+\tau _j, together with the savings account, support an admissible self-financing strategy with zero initial wealth, nonnegative wealth at all times, and strictly positive terminal wealth almost surely. Thus the finite bond market violates NA (hence NFLVR) and admits no equivalent local martingale measure.

The count is generically minimal for this instantaneous zero-volatility construction: N+1N+1 denotes N+1N+1 risky bonds, in addition to the savings account.

Proof.Write

a0(t,τ):=0τ(φ˙t(u)φt(u)qN(u))du.a_0(t,\tau ):=\int _0^\tau \bigl (\dot \varphi _t(u)-\varphi _t'(u)-q^N(u)\bigr )\,du.
With Fn,HnF_n,H_n as in (10), the state-linear difference between the model’s drift and HJM transport in (11) is
n=1N[(1κλn)bns(τ)ωnbnc(τ)]xn,t.\sum _{n=1}^N \left [\left (\frac 1\kappa -\lambda _n\right )b_n^s(\tau ) -\omega _nb_n^c(\tau )\right ]x_{n,t}.
Since (bns)=κ1bns+ωnbnc(b_n^s)'=-\kappa ^{-1}b_n^s+\omega _nb_n^c, its maturity integral is Hn-H_n. The bond calculation in Lemma 2.1, including 0τqN=12σ02nFn(τ)2\int _0^\tau q^N=\frac 12\sigma _0^2\sum _nF_n(\tau )^2, therefore gives
(12)dP~(t,T)P~(t,T)=[a0(t,Tt)+n=1NHn(Tt)xn,t]dtσ0n=1NFn(Tt)dWtn.\begin{equation}\label {eq:bondwitness-return} \frac {d\widetilde P(t,T)}{\widetilde P(t,T)} =\left [-a_0(t,T-t)+\sum _{n=1}^NH_n(T-t)x_{n,t}\right ]dt -\sigma _0\sum _{n=1}^NF_n(T-t)\,dW_t^n. \end{equation}
The deterministic HJM defect enters as the intercept a0a_0.

Fix any kNk\le N. The analytic functions F1,,FN,HkF_1,\ldots ,F_N,H_k are linearly independent on every open JJ. Indeed, differentiation first proves independence of the FnF_n from that of the distinct sine modes. If HkH_k lay in their span, differentiating would put

Hk=(λk1κ)bks+ωkbkcH_k'=\left (\lambda _k-\frac 1\kappa \right )b_k^s+\omega _kb_k^c
in the finite sine span, impossible because ωk>0\omega _k>0 and the sine–cosine characters are linearly independent on every open interval. The elementary evaluation lemma for linearly independent functions now supplies distinct τ1,,τN+1J\tau _1,\ldots ,\tau _{N+1}\in J such that
(13)det[F1(τ1)FN(τ1)Hk(τ1)F1(τN+1)FN(τN+1)Hk(τN+1)]0.\begin{equation}\label {eq:bond-evaluation-det} \det \left [ \begin {array}{cccc} F_1(\tau _1)&\cdots &F_N(\tau _1)&H_k(\tau _1)\\ \vdots &&\vdots &\vdots \\ F_1(\tau _{N+1})&\cdots &F_N(\tau _{N+1})&H_k(\tau _{N+1}) \end {array}\right ]\ne 0. \end{equation}
For completeness, the evaluation lemma follows by induction: if no final evaluation point made the determinant nonzero, the last function would be a fixed linear combination of the preceding ones. The determinant in (13) is a nonzero real-analytic function of the maturity tuple, so its nonzero set is open and dense in the ordered simplex. Since the zero set of a nonvanishing real-analytic function is Lebesgue-null, that set also has full measure, as the theorem asserts.

Set Tj=t0+τjT_j=t_0+\tau _j and, for tt near t0t_0, define

Fjn(t):=Fn(Tjt),j(t):=(1)j+N+1detF(j)(t),\mathsf F_{jn}(t):=F_n(T_j-t), \qquad \ell _j(t):=(-1)^{j+N+1}\det \mathsf F^{(j)}(t),
where F(j)\mathsf F^{(j)} deletes row jj. Laplace expansion gives (t)F(t)=0\ell (t)^\top \mathsf F(t)=0. By (13) and continuity, there is a deterministic ε>0\varepsilon >0 with t0+ε<minjTjt_0+\varepsilon <\min _jT_j such that rankF(t)=N\operatorname {rank}\mathsf F(t)=N and
(14)(t)(Hk(T1t),,Hk(TN+1t))0\begin{equation}\label {eq:cofactor-H} \ell (t)^\top \bigl (H_k(T_1-t),\ldots ,H_k(T_{N+1}-t)\bigr )^\top \ne 0 \end{equation}
throughout [t0,t0+ε][t_0,t_0+\varepsilon ].

Let μ(t)\mu (t) be the vector of discounted relative drifts in (12) and put gt:=(t)μ(t)g_t:=\ell (t)^\top \mu (t). By (14), the coefficient of xk,t0x_{k,t_0} in gt0g_{t_0} is nonzero. Since

Var(xn,t0)=σ022λn(1e2λnt0)>0,\operatorname {Var}(x_{n,t_0}) =\frac {\sigma _0^2}{2\lambda _n}\bigl (1-e^{-2\lambda _nt_0}\bigr )>0,
gt0g_{t_0} is a nondegenerate affine Gaussian, even in the presence of the deterministic intercept a0a_0, and hence P(gt0=0)=0\Pm (g_{t_0}=0)=0.

Set ζ:=sgn(gt0)\zeta :=\operatorname {sgn}(g_{t_0}) and

ϱ:=inf{tt0:ζgt12|gt0|}(t0+ε).\varrho :=\inf \left \{t\ge t_0: \zeta g_t\le \tfrac 12|g_{t_0}|\right \}\wedge (t_0+\varepsilon ).
Here gt=(t)μ(t)g_t=\ell (t)^\top \mu (t) is jointly continuous in (t,ω)(t,\omega ): \ell and a0a_0 are deterministic and continuous, and μ\mu is affine in the continuous state Xt\X _t with continuous deterministic coefficients. Since ζgt0=|gt0|>0\zeta g_{t_0}=|g_{t_0}|>0 a.s., continuity of tζgtt\mapsto \zeta g_t gives ϱ>t0\varrho >t_0 almost surely. Use the predictable discounted dollar exposures
hj(t):=ζj(t)1(t0,ϱ](t),h_j(t):=\zeta \ell _j(t)\mathbf 1_{(t_0,\varrho ]}(t),
equivalently the bond units
ϑj(t):=ζj(t)P~(t,Tj)1(t0,ϱ](t).\vartheta _j(t):= \frac {\zeta \ell _j(t)}{\widetilde P(t,T_j)} \mathbf 1_{(t_0,\varrho ]}(t).
Here ζ\zeta is Ft0\mathcal F_{t_0}-measurable, and the continuous hitting time ϱ\varrho is predictable, so the exposures are predictable. Because every P~(,Tj)\widetilde P(\cdot ,T_j) is strictly positive and continuous and \ell is deterministic and continuous, the bond units are locally bounded and hence semimartingale-integrable. Their discounted gain, started from zero, satisfies exactly
dGt=j=1N+1ϑj(t)dP~(t,Tj)=ζgt1(t0,ϱ](t)dt,dG_t=\sum _{j=1}^{N+1}\vartheta _j(t)\,d\widetilde P(t,T_j) =\zeta g_t\mathbf 1_{(t_0,\varrho ]}(t)\,dt,
because F=0\ell ^\top \mathsf F=0. It has no Brownian term and
Gt0,Gt0+ε=Gϱ12|gt0|(ϱt0)>0a.s.G_t\ge 0, \qquad G_{t_0+\varepsilon }=G_\varrho \ge \tfrac 12|g_{t_0}|(\varrho -t_0)>0 \quad \text {a.s.}
The risky positions are financed through the discounted cash holding
ϑt0:=Gtjϑj(t)P~(t,Tj).\vartheta _t^0:=G_t-\sum _j\vartheta _j(t)\widetilde P(t,T_j).
After ϱ\varrho the positive wealth is left in cash. This defines a self-financing admissible arbitrage. Finally, for mNm\le N generic bonds the m×Nm\times N evaluation matrix of the independent FnF_n has row rank mm, hence no nonzero left-null portfolio. This proves the generic-minimality claim.

Remark 4.7 (What the construction needs: a recipe, not a computation) . The proof used three properties of the model and nothing else, so the route generalises. Let a factor term-structure model have (i) loadings real-analytic on some open maturity interval JJ; (ii) a state-linear discrepancy ncn(τ)xn,t\sum _nc_n(\tau )x_{n,t} between its drift and HJM transport, whose maturity integral 0ck\int _0^\cdot c_k fails to lie in the span of the integrated volatility loadings {0σn}nN\{\int _0^\cdot \sigma _n\}_{n\le N} as functions on JJ — equivalently, a discrepancy no Girsanov tilt can reach; and (iii) a state making the surviving drift functional gt0=(t0)μ(t0)g_{t_0}=\ell (t_0)^\top \mu (t_0) nondegenerate, in the sense that its law is atom-free at 00. Nondegeneracy of the individual coordinates is not enough: if the cofactor pairing leaves the combination a=(1,1)a=(1,-1) while x1,t0=x2,t0x_{1,t_0}=x_{2,t_0} almost surely, both coordinates are nondegenerate and aXt0a^\top \X _{t_0} vanishes identically. A state law with positive-definite covariance on the relevant coordinates — as in Theorem 4.6, where the xnx_n are independent with positive variance — is a convenient sufficient condition. Then the evaluation-determinant argument supplies an open dense set of maturity tuples, the cofactor portfolio annihilates the volatility matrix identically, and the sign-and-stopping argument converts the surviving drift into an admissible arbitrage in N+1N+1 bonds. Nothing in this uses the sine basis, the cylindrical noise, or the particular symbol. The passage from “the drift condition fails in a direction outside rangeΣ\operatorname {range}\Sigma” to an explicit finite portfolio is therefore available for any such model. And it is constructive, where the fundamental theorem of asset pricing would give only existence.

4.5The size of the obstruction

The next result measures the size of the unreachable drift. Its quotient class is intrinsic; the displayed scalar uses the model’s own normalization of the coordinates, and Remark 4.9 says what it does and does not measure.

Proposition 4.8 (Normalized-coordinate size of the unspanned drift) . Order the nnth envelope state as (sn,cn)(s_n,c_n), with the sine coordinate first, and let

KNC:=n=1N(λn12),MN:=n=1NMn,ΣN:=σ0(e1s,,eNs).K_N^{\mathrm C}:=\bigoplus _{n=1}^N(-\lambda _n\one _2), \qquad M_N:=\bigoplus _{n=1}^NM_n, \qquad \Sigma _N:=\sigma _0(\mathbf e_1^s,\ldots ,\mathbf e_N^s).
The invariant object is the quotient class
oN(x):=[(KNCMN)x]R2N/rangeΣN.\mathfrak o_N(x):= \big [(K_N^{\mathrm C}-M_N^\top )x\big ] \in \R ^{2N}/\operatorname {range}\Sigma _N.
In the canonically normalized sine–cosine coordinates above, equip the quotient with the induced Euclidean norm and put dn:=κ1λnd_n:=\kappa ^{-1}-\lambda _n. Then
(15)dN(x)2:=infγRN(KNCMN)xΣNγ22=n=1N(ωnsn+dncn)2.\begin{equation}\label {eq:obstruction-size} \mathfrak d_N(x)^2 :=\inf _{\gamma \in \R ^N} \left \|(K_N^{\mathrm C}-M_N^\top )x-\Sigma _N\gamma \right \|_2^2 =\sum _{n=1}^N(-\omega _ns_n+d_nc_n)^2. \end{equation}
For the stationary embedded sine truncation, cn=0c_n=0 and the sns_n are independent centred Gaussians with variance σ02/(2λn)\sigma _0^2/(2\lambda _n). Thus, for independent standard normal variables ZnZ_n,
(16)dN(X)2 =d n=1Nσ02κωn21+κ2ωn2Zn2,\begin{equation}\label {eq:obstruction-law} \mathfrak d_N(X)^2\ \stackrel {d}{=}\ \sum _{n=1}^N \frac {\sigma _0^2\kappa \omega _n^2}{1+\kappa ^2\omega _n^2}\,Z_n^2, \end{equation}
and consequently, from (16),
(17)EdN(X)2=σ02κ[Nn=1N11+κ2ωn2](18)=σ02κNσ022κ[θκcoth(θκ)1]+O(N1).\begin{align} \E \,\mathfrak d_N(X)^2 &=\frac {\sigma _0^2}{\kappa } \left [N-\sum _{n=1}^N\frac 1{1+\kappa ^2\omega _n^2}\right ] \label {eq:mean-obstruction}\\ &=\frac {\sigma _0^2}{\kappa }N -\frac {\sigma _0^2}{2\kappa } \left [\frac {\theta ^*}{\kappa }\coth \!\left (\frac {\theta ^*}{\kappa }\right )-1\right ] +O(N^{-1}). \label {eq:mean-obstruction-asymp} \end{align}

Under the natural nested coupling of the stationary coordinates,

(19)dN(X)2Nσ02κalmost surely and in L2.\begin{equation}\label {eq:obstruction-lln} \frac {\mathfrak d_N(X)^2}{N}\longrightarrow \frac {\sigma _0^2}{\kappa } \qquad \text {almost surely and in }L^2. \end{equation}
Thus the normalized squared obstruction is extensive: it approaches σ02/κ\sigma _0^2/\kappa per retained mode rather than disappearing with refinement.

Proof.On block nn,

KnCMn=(dnωnωndn).K_{n}^{\mathrm C}-M_n^\top =\begin {pmatrix}d_n&\omega _n\\-\omega _n&d_n\end {pmatrix}.
The volatility range is exactly the sine coordinate in every block. Minimization over γn\gamma _n removes the first row and leaves ωnsn+dncn-\omega _ns_n+d_nc_n, proving (15). In stationarity,
E(ωn2sn2)=σ02ωn22λn=σ02κ(111+κ2ωn2),\E (\omega _n^2s_n^2) =\frac {\sigma _0^2\omega _n^2}{2\lambda _n} =\frac {\sigma _0^2}{\kappa } \left (1-\frac 1{1+\kappa ^2\omega _n^2}\right ),
which gives (17). The identity
n=111+(κπn/θ)2=12[θκcoth(θκ)1]\sum _{n=1}^{\infty }\frac 1{1+(\kappa \pi n/\theta ^*)^2} =\frac 12\left [ \frac {\theta ^*}{\kappa }\coth \!\left (\frac {\theta ^*}{\kappa }\right )-1\right ]
and its O(N1)O(N^{-1}) tail give (18). Finally the independent summands ωn2sn2\omega _n^2s_n^2 have uniformly bounded variances and means converging to σ02/κ\sigma _0^2/\kappa. Kolmogorov’s strong law gives the almost-sure limit in (19); the same variance bound gives L2L^2 convergence.

Remark 4.9 (What the modulus does and does not measure) . The quotient class oN\mathfrak o_N and its nonvanishing are invariant under invertible factor changes; the Euclidean number dN\mathfrak d_N is tied to the normalized sine–cosine coordinates and changes under a non-orthogonal rescaling. It quantifies only the state-linear drift component outside the Girsanov range, not the deterministic convexity defect. It is therefore neither a market price of risk, a Sharpe ratio, a hedging loss, nor a monetary reserve. A security-output norm would additionally require a declared maturity panel and portfolio metric; Theorem 4.6 supplies the invariant fact needed here, namely that a generic finite panel separates the quotient class.

That completes the finite-NN diagnosis. What survives it in the infinite model is the next question.

4.6The infinite model: an energy obstruction

In the infinite cylindrical model the sine system is complete in the state space, so no literal “noiseless coordinate” survives the limit and Remark 4.4 does not upgrade termwise. What survives is an energy obstruction.

Proposition 4.10 (The infinite model: no square-integrable Girsanov repair) . (i) The stationary field’s maturity increments obey E(Xt(θ+h)Xt(θ))2=σ02κe2θ/κ|h|+O(h2)\E \bigl (X_t(\theta +h)-X_t(\theta )\bigr )^2 =\frac {\sigma _0^2}{\kappa }e^{-2\theta /\kappa }|h|+O(h^2) at every interior θ\theta. The field is Brownian-rough in maturity, hence a.s. nowhere differentiable in θ\theta, and XtC1X_t\notin C^1 a.s. (ii) On the completed natural filtration of the driving cylindrical Brownian motion, every equivalent change of measure is represented by a predictable Girsanov density γ\gamma satisfying

0TγtH2dt<a.s.,\int _0^T\|\gamma _t\|_H^2\,dt<\infty \qquad \text {a.s.},
together with the condition that its stochastic exponential is a true martingale. Thus the relevant integrand space is the pathwise space L2([0,T];H)L^2([0,T];H), not L2([0,T];Hw)L^2([0,T];H_w). For the stationary solution, and also for every deterministic X0HX_0\in H independent of the future noise, at each t>0t>0
(20)n1ωn4|xn(t)|2=a.s.\begin{equation}\label {eq:notH2} \sum _{n\ge 1}\omega _n^4|x_n(t)|^2=\infty \qquad \text {a.s.} \end{equation}
Consequently θ2XtH\partial _\theta ^2X_t\notin H a.s. for every t>0t>0, and with probability one this holds for Lebesgue-a.e. t(0,T)t\in (0,T). Hence there is no predictable γL2([0,T];H)\gamma \in L^2([0,T];H) for which
σ0γt=(A~θ)Xtqt=κ2θ2Xtqt\sigma _0\gamma _t=(\widetilde A-\partial _\theta )X_t-q_t =\frac \kappa 2\partial _\theta ^2X_t-q_t
holds distributionally for a.e. tt, whenever the proposed convexity term qtq_t is HH-valued. In particular, an equivalent measure change cannot implement this repair even if the drift identity is required only against the test core Cc(0,θ)C_c^\infty (0,\theta ^*). The spatial assertion in (i) is the stationary stochastic-heat regularity; see [4133]. Part (ii) is proved below.

Proof.The map U:HL2(0,θ)U:H\to L^2(0,\theta ^*), (Uf)(θ)=eθ/κf(θ)(Uf)(\theta )=e^{\theta /\kappa }f(\theta ), is unitary and Uen=ϕn:=2/θsin(ωnθ)Ue_n=\phi _n:=\sqrt {2/\theta ^*}\sin (\omega _n\theta ). In stationarity, the coefficients of Y:=UXY:=UX have variances

σ022λn=σ02κ(ωn2+κ2).\frac {\sigma _0^2}{2\lambda _n} =\frac {\sigma _0^2}{\kappa (\omega _n^2+\kappa ^{-2})}.
Therefore
Cov(Y(θ),Y(u))=σ02κGθ2+κ2D(θ,u),\operatorname {Cov}(Y(\theta ),Y(u)) =\frac {\sigma _0^2}{\kappa } G^D_{-\partial _\theta ^2+\kappa ^{-2}}(\theta ,u),
where GDG^D is the Dirichlet Green kernel. Its first derivative has the unit diagonal jump, so the covariance increment identity gives E[(Y(θ+h)Y(θ))2]=(σ02/κ)|h|+O(h2)\E [(Y(\theta +h)-Y(\theta ))^2]=(\sigma _0^2/\kappa )|h|+O(h^2). Since X(θ)=eθ/κY(θ)X(\theta )=e^{-\theta /\kappa }Y(\theta ), part (i)’s displayed asymptotic follows. The Gaussian process YY is the massive Brownian (Ornstein–Uhlenbeck) bridge in the spatial coordinate; its quadratic variation is (σ02/κ)dθ(\sigma _0^2/\kappa )d\theta. Thus it, and its product with the positive smooth envelope eθ/κe^{-\theta /\kappa }, is a.s. nowhere differentiable.

For (ii), moreover,

UAU1=κ2θ212κUAU^{-1}=\frac \kappa 2\partial _\theta ^2-\frac 1{2\kappa }
with Dirichlet domain. For deterministic initial data, the independent Gaussian noise parts of xn(t)x_n(t) have variances
vn(t)=σ022λn(1e2λnt)ωn2(t>0,n);v_n(t)=\frac {\sigma _0^2}{2\lambda _n}\bigl (1-e^{-2\lambda _nt}\bigr )\asymp \omega _n^{-2} \qquad (t>0,n\to \infty );
in stationarity, vn=σ02/(2λn)v_n=\sigma _0^2/(2\lambda _n) exactly. Writing xn(t)=mn(t)+vn(t)Znx_n(t)=m_n(t)+\sqrt {v_n(t)}Z_n with independent standard normals, the events |xn(t)|12vn(t)|x_n(t)|\ge \frac 12\sqrt {v_n(t)} have probabilities bounded below uniformly in nn (the centred interval has maximal Gaussian mass when mn(t)=0m_n(t)=0). Independence and the second Borel–Cantelli lemma therefore imply that infinitely many occur. Their terms in nωn4xn(t)2\sum _n\omega _n^4x_n(t)^2 are bounded below by a positive multiple of ωn2\omega _n^2, proving (20).

Zero traces are needed before the sine criterion may be applied, and they do not follow from (20) alone: f1f\equiv 1 has f=0Hf''=0\in H while its sine coefficients are of order n1n^{-1}, so its weighted sum diverges. They do hold here. In stationarity part (i) exhibits Y=UXtY=UX_t as the massive Brownian bridge on [0,θ][0,\theta ^*], which has a continuous modification vanishing at both endpoints; for deterministic X0HX_0\in H, write Xt=etAX0+ZtX_t=e^{tA}X_0+Z_t where Zt:=XtstatetAX0statZ_t:=X^{\mathrm {stat}}_t-e^{tA}X^{\mathrm {stat}}_0 is a version of the stochastic convolution. The semigroup terms lie in D(A)H2H01D(A)\subset H^2\cap H_0^1 for t>0t>0 (AA is self-adjoint and negative after conjugation, hence analytic), and the bridge terms vanish at the endpoints, so XtX_t is continuous with Xt(0)=Xt(θ)=0X_t(0)=X_t(\theta ^*)=0 a.s.

Now suppose θ2XtH\partial _\theta ^2X_t\in H. One-dimensional elliptic regularity then gives XtH2X_t\in H^2, and with the zero traces just established UXtH2H01UX_t\in H^2\cap H_0^1 (multiplication by e±θ/κe^{\pm \theta /\kappa } preserves H2H^2 on a finite interval). The Dirichlet sine characterisation — UXtH2H01UX_t\in H^2\cap H_0^1 if and only if n(1+ωn4)|xn(t)|2<\sum _n(1+\omega _n^4)|x_n(t)|^2<\infty — then contradicts (20). Hence θ2XtH\partial _\theta ^2X_t\notin H. Since this holds with probability one for each t>0t>0, Tonelli’s theorem applied to the indicator of the exceptional H2H^2 event gives the simultaneous statement for Lebesgue-a.e. tt, almost surely. If the displayed weak drift identity held with γt,qtH\gamma _t,q_t\in H, its right-hand side would give an HH representative of θ2Xt\partial _\theta ^2X_t as a distribution, contradicting the preceding conclusion. Finally, on the completed natural Brownian filtration, Girsanov’s theorem requires 0TγtH2dt<\int _0^T\|\gamma _t\|_H^2dt<\infty almost surely, in addition to the true-martingale condition for the density exponential, so such a measure change is unavailable.

That is the obstruction under the model’s own noise. One question remains before the diagnosis is complete, and the next subsection settles it: what changes if the silent coordinates are given noise of their own, so that the defect becomes reachable by a change of measure.

4.7When the silent coordinates are loaded: a market-price-of-risk cost

Remark 4.4 and Proposition 4.10 rest on the same fact: under the model’s sine-only loading the defect leaves the range of the volatility, so no tilt can reach it. Suppose instead that every block is loaded isotropically, with intensities σn>0\sigma _n>0 and nωn2σn2<\sum _n\omega _n^2\sigma _n^2<\infty, and use the damping-compatible weight (1). This loading adds one Brownian source per block: it is a second completion, compared with the sine-only one in Remark 5.3(iii). With it the defect lies inside the volatility range, Girsanov’s theorem applies at every finite order, and the question becomes what the tilt costs and whether the cost stays finite on the infinite envelope. The answer is a dichotomy governed by one number.

For an entire function pp with p(z¯)=p(z)p(\bar z)=\overline {p(z)} the induced drift on block nn is p(Mn)p(M_n)^\top: the proof of Proposition 4.2(a) applies to the power series of pp, which converges on the two-dimensional block. Since Mn=κ11+ωnJM_n=-\kappa ^{-1}\one +\omega _nJ with J2=1J^2=-\one, every entire ff satisfies f(Mn)=Ref(zn)1+Imf(zn)Jf(M_n)=\operatorname {Re}f(z_n)\,\one +\operatorname {Im}f(z_n)\,J with zn:=κ1+iωnz_n:=-\kappa ^{-1}+i\omega _n. Write

(21)δn:=p(zn)zn,kn:=Rep(zn),en:=|δn|2kn,E:=n1en,\begin{equation}\label {eq:defect} \delta _n:=p(z_n)-z_n,\qquad k_n:=-\operatorname {Re}p(z_n),\qquad \mathfrak e_n:=\frac {|\delta _n|^2}{k_n},\qquad \mathcal E:=\sum _{n\ge 1}\mathfrak e_n, \end{equation}

and let Ξn:=p(Mn)Mn\Xi _n:=p(M_n)^\top -M_n^\top be the defect block, the difference between the induced drift and the arbitrage-free drift of Proposition 2.7. Then ΞnΞn=|δn|212\Xi _n^\top \Xi _n=|\delta _n|^2\one _2, and the symmetric part of p(Mn)p(M_n)^\top is kn12-k_n\one _2: knk_n is the mean-reversion rate of block nn under the induced dynamics and κ1\kappa ^{-1} its rate under the arbitrage-free dynamics. We call en\mathfrak e_n the defect energy of block nn and E\mathcal E the defect energy of the envelope. For the model’s symbol p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2 one has p(zn)=λnp(z_n)=-\lambda _n (Proposition 3.1), hence δn=(λn+zn)\delta _n=-(\lambda _n+z_n), |δn|2=dn2+ωn2=λn2|\delta _n|^2=d_n^2+\omega _n^2=\lambda _n^2 with dn=κ1λnd_n=\kappa ^{-1}-\lambda _n as in Proposition 4.8, kn=λnk_n=\lambda _n, en=λn\mathfrak e_n=\lambda _n, and Ξn\Xi _n is the block displayed in Remark 4.4.

All laws below live on the canonical product path space Ω:=n1C([0,T];R2)\Omega :=\prod _{n\ge 1}C([0,T];\R ^2), 0<T<0<T<\infty, with its product σ\sigma-algebra FT\mathcal F_T. The coordinate process is x=(xn)n1x=(x_n)_{n\ge 1} with xn=(sn,cn)x_n=(s_n,c_n); its raw canonical filtration is augmented under each law separately where needed, and FT(N):=σ{xn(s):nN, sT}\mathcal F^{(N)}_T:=\sigma \{x_n(s):n\le N,\ s\le T\} is the σ\sigma-field of the first NN blocks. Writing bns,bncb_n^s,b_n^c for the two components of Bn\B _n, direct differentiation and (1) give

bnsw2+bncw2=2θ[1+(ωn2+κ2)Cw].\|b_n^s\|_w^2+\|b_n^c\|_w^2 =\frac 2{\theta ^*} \left [1+\left (\omega _n^2+\kappa ^{-2}\right )C_w\right ].

Consequently nωn2σn2<\sum _n\omega _n^2\sigma _n^2<\infty makes nBnxn\sum _n\B _n^\top x_n an HwH_w-valued process under the arbitrage-free dynamics. The same is true under the induced dynamics whenever infnkn>0\inf _nk_n>0, since each coordinate variance is then bounded by a constant multiple of σn2\sigma _n^2. Nothing in the proposition itself requires the coordinate sequence to define a curve: its statements concern the two product laws.

Proposition 4.11 (Girsanov energy and the Kakutani dichotomy) . Under the isotropic loading above, let Pdef\Pm ^{\mathrm {def}} and PNA\Pm ^{\mathrm {NA}} be the laws on FT\mathcal F_T, 0<T<0<T<\infty, of the factor process started at the origin, under the induced drift p(M)p(M)^\top and under the arbitrage-free drift MM^\top respectively, with the same noise. Assume kn>0k_n>0 for all nn, except where (c) says otherwise; in (a) this assumption enters only the stationary statement.

  1. (Finite order.) Let PN:=Pdef|FT(N)P_N:=\Pm ^{\mathrm {def}}|_{\mathcal F^{(N)}_T} and QN:=PNA|FT(N)Q_N:=\Pm ^{\mathrm {NA}}|_{\mathcal F^{(N)}_T}. For every NN, PNQNP_N\sim Q_N with

    dQNdPN=exp(nN0Tγn,tdWtn12nN0T|γn,t|2dt),γn,t=σn1Ξn(sn,tcn,t),\frac {dQ_N}{dP_N} =\exp \Bigl (-\sum _{n\le N}\int _0^T\gamma _{n,t}\cdot d\W ^n_t -\tfrac 12\sum _{n\le N}\int _0^T|\gamma _{n,t}|^2dt\Bigr ),\qquad \gamma _{n,t}=\sigma _n^{-1}\,\Xi _n\binom {s_{n,t}}{c_{n,t}},
    where Wn\W ^n is the Pdef\Pm ^{\mathrm {def}}-Brownian motion of block nn. In Pdef\Pm ^{\mathrm {def}}-stationarity EnN|γn,t|2=nNen\E \sum _{n\le N}|\gamma _{n,t}|^2=\sum _{n\le N}\mathfrak e_n, whatever the intensities. The Hellinger affinity of PNP_N and QNQ_N is nNhn\prod _{n\le N}\mathfrak h_n with
    (22)hn=ek¯nTcosh(mnT)+(k¯n/mn)sinh(mnT),k¯n:=12(kn+κ1),mn2:=k¯n2+14|δn|2.\begin{equation}\label {eq:hellinger} \mathfrak h_n=\frac {e^{\bar k_nT}}{\cosh (\mathfrak m_nT)+(\bar k_n/\mathfrak m_n)\sinh (\mathfrak m_nT)}, \qquad \bar k_n:=\tfrac 12\bigl (k_n+\kappa ^{-1}\bigr ),\qquad \mathfrak m_n^2:=\bar k_n^2+\tfrac 14|\delta _n|^2 . \end{equation}
  2. (Infinite envelope.) On FT\mathcal F_T,

    PdefPNAE<n|δn|2<Ξ:=nΞn is Hilbert--Schmidt,\Pm ^{\mathrm {def}}\sim \Pm ^{\mathrm {NA}} \iff \mathcal E<\infty \iff \sum _n|\delta _n|^2<\infty \iff \Xi :=\textstyle \bigoplus _n\Xi _n\ \text {is Hilbert--Schmidt},
    Ξ\Xi acting on 2(N;R2)\ell ^2(\mathbb N;\R ^2); otherwise the two laws are mutually singular, with 0T|γt|2dt=\int _0^T|\gamma _t|^2dt=\infty Pdef\Pm ^{\mathrm {def}}-a.s., where |γt|2:=n1|γn,t|2|\gamma _t|^2:=\sum _{n\ge 1}|\gamma _{n,t}|^2. In the singular case no measure equivalent to Pdef\Pm ^{\mathrm {def}} gives the factor process the dynamics of Proposition 2.7.
  3. Equivalence forces δn0\delta _n\to 0, hence knκ1k_n\to \kappa ^{-1}. It fails for every polynomial symbol of degree at least two. If kn0k_n\le 0 on infinitely many blocks, the two product laws are still defined on Ω\Omega and are mutually singular there, although the coordinate sequence need not then define an HwH_w-valued curve.
  4. (The model.) For p(z)=z+κ2z2p(z)=z+\frac \kappa 2z^2,

    EN:=nNen=nNλn=N2κ+κπ2N(N+1)(2N+1)12θ2,\mathcal E_N:=\sum _{n\le N}\mathfrak e_n=\sum _{n\le N}\lambda _n =\frac N{2\kappa }+\frac {\kappa \pi ^2N(N+1)(2N+1)}{12\,\theta ^{*2}},
    and, with c1:=1212c_1:=\frac 1{\sqrt 2}-\frac 12,
    eTEN/4  nNhn  2Ne(11/2)NT/(2κ)ec1TEN,e^{-T\mathcal E_N/4}\ \le \ \prod _{n\le N}\mathfrak h_n\ \le \ 2^N\,e^{(1-1/\sqrt 2)NT/(2\kappa )}\,e^{-c_1T\mathcal E_N},
    so that lognNhnc1TENc1κπ2TN3/(6θ2)-\log \prod _{n\le N}\mathfrak h_n\sim c_1T\,\mathcal E_N\sim c_1\kappa \pi ^2TN^3/(6\theta ^{*2}). The tilted truncations are therefore equivalent at every order and singular in the limit, and their affinity decays like ecN3e^{-cN^3} on both sides.

Part (d) is the quantitative counterpart of Remark 4.4. With the sine-only loading the two laws are inequivalent at every order because the defect is unreachable; with the isotropic loading they are equivalent at every order, at a cost growing like N3N^3, and inequivalent in the limit. The two loadings agree on the infinite verdict and differ in what they say about truncations: an impossibility against a price.

Proof.(a) On the first NN blocks the drift is linear in the state, so the stochastic exponential of the linear (γn)nN(\gamma _n)_{n\le N} is a true martingale (Beneš’ criterion, [31, Cor. 3.5.16]). Writing the factor equation of those blocks as dx=p(M)xdt+ΣdW=Mxdt+Σ(dW+γdt)dx=p(M)^\top x\,dt+\Sigma \,d\W =M^\top x\,dt+\Sigma \,(d\W +\gamma \,dt) identifies W+γdt\W +\int \gamma \,dt as a 2N2N-dimensional Brownian motion under the tilted measure on FT(N)\mathcal F^{(N)}_T, whose density is the displayed exponential; neither this nor the affinity formula below uses kn>0k_n>0. Block nn of p(M)p(M)^\top is normal with symmetric part kn1-k_n\one, so its stationary covariance solves the Lyapunov equation and equals σn2/(2kn)12\sigma _n^2/(2k_n)\,\one _2; hence E|γn|2=σn2tr(ΞnΞn)σn2/(2kn)=|δn|2/kn=en\E |\gamma _n|^2=\sigma _n^{-2}\operatorname {tr}(\Xi _n^\top \Xi _n)\,\sigma _n^2/(2k_n) =|\delta _n|^2/k_n=\mathfrak e_n. For the affinity let bdefb^{\mathrm {def}}, bNAb^{\mathrm {NA}} be the two drifts and Pmid\Pm ^{\mathrm {mid}} the law with the midpoint drift 12(bdef+bNA)\frac 12(b^{\mathrm {def}}+b^{\mathrm {NA}}). Since 12(|bdef|2+|bNA|2)|12(bdef+bNA)|2=14|bdefbNA|2\frac 12(|b^{\mathrm {def}}|^2+|b^{\mathrm {NA}}|^2)-|\frac 12(b^{\mathrm {def}}+b^{\mathrm {NA}})|^2 =\frac 14|b^{\mathrm {def}}-b^{\mathrm {NA}}|^2, the Girsanov densities against the driftless reference law give dPdefdPNA=dPmidexp(180T|Σ1Ξxt|2dt)\sqrt {d\Pm ^{\mathrm {def}}\,d\Pm ^{\mathrm {NA}}} =d\Pm ^{\mathrm {mid}}\exp \bigl (-\frac 18\int _0^T|\Sigma ^{-1}\Xi x_t|^2dt\bigr ). Block nn of the midpoint drift is normal with symmetric part k¯n1-\bar k_n\one; its skew part rotates (sn,cn)(s_n,c_n) without changing the modulus, so hn=Emidexp(18|δn|20T|yt|2dt)\mathfrak h_n=\E ^{\mathrm {mid}}\exp \bigl (-\frac 18|\delta _n|^2\int _0^T|y_t|^2dt\bigr ) with yy a two-dimensional Ornstein–Uhlenbeck process of rate k¯n\bar k_n and unit intensity started at 00 (the intensity σn\sigma _n cancels). For a one-dimensional such process the Riccati equation for the exponent gives Eexp(ϑ0Tyt2dt)=ek¯T/2(coshmT+(k¯/m)sinhmT)1/2\E \exp (-\vartheta \int _0^Ty_t^2dt)=e^{\bar kT/2}\bigl (\cosh \mathfrak mT +(\bar k/\mathfrak m)\sinh \mathfrak mT\bigr )^{-1/2} with m2=k¯2+2ϑ\mathfrak m^2=\bar k^2+2\vartheta; squaring for the two independent coordinates and putting ϑ=|δn|2/8\vartheta =|\delta _n|^2/8 gives (22).

(b) Under both laws the blocks are independent, so on FT\mathcal F_T both laws are product measures over nn with equivalent factors by (a), and Kakutani’s theorem [30] states that they are equivalent if nhn>0\prod _n\mathfrak h_n>0 and mutually singular otherwise. Sufficiency. By Jensen, hn=EdefdPnNA/dPndefexp(12KLn)\mathfrak h_n=\E ^{\mathrm {def}}\sqrt {d\Pm ^{\mathrm {NA}}_n/d\Pm ^{\mathrm {def}}_n} \ge \exp (-\frac 12\mathrm {KL}_n) with KLn=12Edef0T|γn,t|2dt\mathrm {KL}_n=\frac 12\E ^{\mathrm {def}}\int _0^T|\gamma _{n,t}|^2dt; from the origin Edef|xn,t|2=(σn2/kn)(1e2knt)\E ^{\mathrm {def}}|x_{n,t}|^2=(\sigma _n^2/k_n)(1-e^{-2k_nt}), so KLn=12en[T(1e2knT)/(2kn)]12enT\mathrm {KL}_n=\frac 12\mathfrak e_n\bigl [T-(1-e^{-2k_nT})/(2k_n)\bigr ]\le \frac 12\mathfrak e_nT and 1hn14enT1-\mathfrak h_n\le \frac 14\mathfrak e_nT. Thus E<\mathcal E<\infty gives n(1hn)<\sum _n(1-\mathfrak h_n)<\infty and equivalence. Necessity. By Kakutani’s criterion it suffices to show that E=\mathcal E=\infty forces n(1hn)=\sum _n(1-\mathfrak h_n)=\infty, and this is done block by block. Put Yn:=0T|γn,t|2dtY_n:=\int _0^T|\gamma _{n,t}|^2dt. The midpoint representation in the proof of (a) reads hn=EmideYn/8\mathfrak h_n=\E ^{\mathrm {mid}}e^{-Y_n/8}, so 1hn=Emid(1eYn/8)(1e1)Emidmin(Yn/8,1)1-\mathfrak h_n=\E ^{\mathrm {mid}}(1-e^{-Y_n/8})\ge (1-e^{-1})\,\E ^{\mathrm {mid}}\min (Y_n/8,1). Under Pmid\Pm ^{\mathrm {mid}}, YnY_n is a positive quadratic functional of a centred Gaussian process, hence by the Karhunen–Loève expansion a sum iaiZi2\sum _ia_iZ_i^2 with ai0a_i\ge 0 and independent standard normals ZiZ_i; so EYn23(EYn)2\E Y_n^2\le 3(\E Y_n)^2 and Paley–Zygmund gives Pmid(Yn12EmidYn)112\Pm ^{\mathrm {mid}}(Y_n\ge \frac 12\E ^{\mathrm {mid}}Y_n)\ge \frac 1{12}, the step already used in Proposition 3.3(c); hence Emidmin(Yn/8,1)112min(116EmidYn,1)\E ^{\mathrm {mid}}\min (Y_n/8,1)\ge \frac 1{12}\min (\frac 1{16}\E ^{\mathrm {mid}}Y_n,1). Block nn under Pmid\Pm ^{\mathrm {mid}} is an Ornstein–Uhlenbeck process with symmetric part k¯n1-\bar k_n\one started at the origin, so Emid|xn,t|2=σn2(1e2k¯nt)/k¯n\E ^{\mathrm {mid}}|x_{n,t}|^2=\sigma _n^2(1-e^{-2\bar k_nt})/\bar k_n and

EmidYn=|δn|2k¯nTφ(k¯nT),φ(u):=11e2u2u(0,1),φ(u)13min(u,1),\E ^{\mathrm {mid}}Y_n=\frac {|\delta _n|^2}{\bar k_n}\,T\,\varphi (\bar k_nT),\qquad \varphi (u):=1-\frac {1-e^{-2u}}{2u}\in (0,1),\qquad \varphi (u)\ge \tfrac 13\min (u,1),
φ\varphi increasing. Split the index set at kn12κk_n\ge \frac 1{2\kappa }. If en=\sum \mathfrak e_n=\infty over the blocks with kn12κk_n\ge \frac 1{2\kappa }, then there k¯n34κ\bar k_n\ge \frac 3{4\kappa } and 2knkn+κ123\frac {2k_n}{k_n+\kappa ^{-1}}\ge \frac 23, so EmidYn=2knkn+κ1enTφ(k¯nT)cen\E ^{\mathrm {mid}}Y_n=\frac {2k_n}{k_n+\kappa ^{-1}}\,\mathfrak e_n\,T\varphi (\bar k_nT) \ge c\,\mathfrak e_n with c:=29Tmin(3T4κ,1)c:=\frac 29T\min (\frac {3T}{4\kappa },1), and min(c16en,1)=\sum \min (\frac c{16}\mathfrak e_n,1)=\infty. Otherwise en=\sum \mathfrak e_n=\infty over the blocks with kn<12κk_n<\frac 1{2\kappa }, which are then infinitely many; there |δn|Reδn=κ1kn>12κ|\delta _n|\ge \operatorname {Re}\delta _n=\kappa ^{-1}-k_n>\frac 1{2\kappa } and k¯n(12κ,34κ)\bar k_n\in (\frac 1{2\kappa },\frac 3{4\kappa }), so EmidYnT3κφ(T2κ)>0\E ^{\mathrm {mid}}Y_n\ge \frac T{3\kappa }\varphi (\frac T{2\kappa })>0 on infinitely many blocks. In either case n(1hn)=\sum _n(1-\mathfrak h_n)=\infty, and Kakutani’s dichotomy gives singularity. The pathwise statement follows from the same estimates under Pdef\Pm ^{\mathrm {def}}: the YnY_n are independent and nonnegative with EdefYn=2KLn=enTφ(knT)\E ^{\mathrm {def}}Y_n=2\,\mathrm {KL}_n=\mathfrak e_nT\varphi (k_nT); Paley–Zygmund gives Edefmin(Yn,1)112min(12EdefYn,1)\E ^{\mathrm {def}}\min (Y_n,1)\ge \frac 1{12}\min (\frac 12\E ^{\mathrm {def}}Y_n,1); the same split shows nEdefmin(Yn,1)=\sum _n\E ^{\mathrm {def}}\min (Y_n,1)=\infty (in the second case enφ(knT)|δn|2min(T,kn1)/3min(T,2κ)/(12κ2)\mathfrak e_n\varphi (k_nT)\ge |\delta _n|^2\min (T,k_n^{-1})/3\ge \min (T,2\kappa )/(12\kappa ^2)); and for independent nonnegative summands this is equivalent to nYn=\sum _nY_n=\infty a.s. (the three-series theorem with Borel–Cantelli). The remaining equivalences follow from kn=κ1Reδnκ1+|δn|k_n=\kappa ^{-1}-\operatorname {Re}\delta _n\le \kappa ^{-1}+|\delta _n|, which gives en|δn|2/(κ1+|δn|)\mathfrak e_n\ge |\delta _n|^2/(\kappa ^{-1}+|\delta _n|): E<\mathcal E<\infty forces δn0\delta _n\to 0, then knκ1k_n\to \kappa ^{-1} and enκ|δn|2\mathfrak e_n\asymp \kappa |\delta _n|^2, while ΞHS2=2n|δn|2\|\Xi \|_{\mathrm {HS}}^2=2\sum _n|\delta _n|^2. For the last sentence: under a measure equivalent to Pdef\Pm ^{\mathrm {def}} that gives the factor process the drift MM^\top with the same noise, the law of the factor process would be PNA\Pm ^{\mathrm {NA}}, which is singular to Pdef\Pm ^{\mathrm {def}}.

(c) is contained in (b): for a polynomial pp of degree at least two, |p(zn)|/ωn|p(z_n)|/\omega _n\to \infty, so |δn||p(zn)||zn||\delta _n|\ge |p(z_n)|-|z_n|\to \infty and n|δn|2=\sum _n|\delta _n|^2=\infty. Blocks with kn0k_n\le 0 do not affect the equivalence in (a) or the affinity formula, neither of which uses kn>0k_n>0; only the stationary energy does. If only finitely many such blocks occur, discard them: their factors are equivalent by (a) and do not affect Kakutani’s product, so (b) applied to the remaining blocks decides the dichotomy. When infinitely many occur, the midpoint rate k¯n=12(kn+κ1)\bar k_n=\frac 12(k_n+\kappa ^{-1}) is at most 12κ\frac 1{2\kappa } there, so Emid|xn,t|2=2σn20te2k¯nsds2σn2κ(1et/κ)\E ^{\mathrm {mid}}|x_{n,t}|^2=2\sigma _n^2\int _0^te^{-2\bar k_ns}ds\ge 2\sigma _n^2\kappa (1-e^{-t/\kappa }) and, since |δn|Reδn=κ1knκ1|\delta _n|\ge \operatorname {Re}\delta _n=\kappa ^{-1}-k_n\ge \kappa ^{-1}, EmidYn2κ1[Tκ(1eT/κ)]>0\E ^{\mathrm {mid}}Y_n\ge 2\kappa ^{-1}\bigl [T-\kappa (1-e^{-T/\kappa })\bigr ]>0 on infinitely many blocks; the necessity argument of (b) then gives n(1hn)=\sum _n(1-\mathfrak h_n)=\infty and singularity on Ω\Omega. The product laws exist on Ω\Omega whatever the signs of the knk_n, but their coordinate variances lack uniform dissipative control: they grow linearly in tt when kn=0k_n=0 and exponentially when kn<0k_n<0. Consequently nωn2|xn|2\sum _n\omega _n^2|x_n|^2 need not converge.

(d) Substitute p(zn)=λnp(z_n)=-\lambda _n and sum λn=(1+κ2ωn2)/(2κ)\lambda _n=(1+\kappa ^2\omega _n^2)/(2\kappa ) over nNn\le N; the sum diverges, so (b) gives singularity in the limit. For the affinity write (22) as

hn=2e(k¯nmn)T(1+k¯n/mn)+(1k¯n/mn)e2mnT,\mathfrak h_n=\frac {2\,e^{(\bar k_n-\mathfrak m_n)T}} {(1+\bar k_n/\mathfrak m_n)+(1-\bar k_n/\mathfrak m_n)\,e^{-2\mathfrak m_nT}},
whose denominator lies between 11 and 22 because 0<k¯nmn0<\bar k_n\le \mathfrak m_n; hence e(k¯nmn)Thn2e(k¯nmn)Te^{(\bar k_n-\mathfrak m_n)T}\le \mathfrak h_n\le 2e^{(\bar k_n-\mathfrak m_n)T}. Now mnk¯n=|δn|2/(4(mn+k¯n))\mathfrak m_n-\bar k_n=|\delta _n|^2/\bigl (4(\mathfrak m_n+\bar k_n)\bigr ), with |δn|2=λn2|\delta _n|^2=\lambda _n^2 and k¯n=12(λn+κ1)\bar k_n=\frac 12(\lambda _n+\kappa ^{-1}) for the model. Since mn+k¯n2k¯nλn\mathfrak m_n+\bar k_n\ge 2\bar k_n\ge \lambda _n, one has mnk¯nλn/4\mathfrak m_n-\bar k_n\le \lambda _n/4, whence nNhneTEN/4\prod _{n\le N}\mathfrak h_n\ge e^{-T\mathcal E_N/4}. In the other direction, mn2=12λn2+λn2κ+14κ2(λn2+122κ)2\mathfrak m_n^2=\frac 12\lambda _n^2+\frac {\lambda _n}{2\kappa }+\frac 1{4\kappa ^2} \ge \bigl (\frac {\lambda _n}{\sqrt 2}+\frac 1{2\sqrt 2\,\kappa }\bigr )^2 gives k¯nmnc1λn+(112)12κ\bar k_n-\mathfrak m_n\le -c_1\lambda _n+(1-\frac 1{\sqrt 2})\frac 1{2\kappa } and the displayed upper bound. Finally (mn+k¯n)/λn12+12(\mathfrak m_n+\bar k_n)/\lambda _n\to \frac 1{\sqrt 2}+\frac 12, so (mnk¯n)/λn(4(12+12))1=c1(\mathfrak m_n-\bar k_n)/\lambda _n\to \bigl (4(\frac 1{\sqrt 2}+\frac 12)\bigr )^{-1}=c_1; as loghn-\log \mathfrak h_n differs from (mnk¯n)T(\mathfrak m_n-\bar k_n)T by at most log2\log 2 and ENN3\mathcal E_N\asymp N^3, it follows that lognNhnc1TEN-\log \prod _{n\le N}\mathfrak h_n\sim c_1T\mathcal E_N.

Remark 4.12 (The price, its invariant, and the sequence of tilted markets) . (i) At the reference calibration (κ,θ)=(4,30)(\kappa ,\theta ^*)=(4,30) and T=1T=1 the truncated model has

N5101632EN1.839.6934.8255EN1.353.115.9016.0nNhn0.920.37610321021.\begin {array}{lcccc} N & 5 & 10 & 16 & 32\\ \hline \mathcal E_N & 1.83 & 9.69 & 34.8 & 255\\ \sqrt {\mathcal E_N} & 1.35 & 3.11 & 5.90 & 16.0\\ \prod _{n\le N}\mathfrak h_n & 0.92 & 0.37 & 6\cdot 10^{-3} & 2\cdot 10^{-21} \end {array}.
(ii) At each finite order, |γt||\gamma _t| bounds the instantaneous Sharpe ratio of every self-financing portfolio in the NN-block market: a portfolio with volatility vector vv has excess drift vγv\cdot \gamma, hence Sharpe ratio vγ/|v||γ|v\cdot \gamma /|v|\le |\gamma |, with equality when vγv\parallel \gamma. A panel of 2N2N bonds as in (iv) attains the equality at all but finitely many times of its horizon, since its volatility vectors then span R2N\R ^{2N}. Thus EN\sqrt {\mathcal E_N} is the stationary root-mean-square of the market price of risk |γt||\gamma _t|, equivalently of the maximal instantaneous Sharpe ratio of the NNth market — a continuous-time local analogue of the Hansen–Jagannathan bound [23] — and E=limNEN\sqrt {\mathcal E}=\lim _N\sqrt {\mathcal E_N} is its limit. Unlike dN\mathfrak d_N of Proposition 4.8 (Remark 4.9), EN\mathcal E_N is a market-price-of-risk energy, precisely because under the isotropic loading the defect lies in the range of the volatility. (iii) The invariant is coordinate-free. For a factor generator KK with noise loading Σ\Sigma, possibly rectangular, whose covariance C=ΣΣC=\Sigma \Sigma ^\top is invertible, and with stationary covariance VV, the minimum-norm tilt carrying the induced dynamics to the class is γmin=ΣC1Ξx\gamma _{\min }=\Sigma ^\top C^{-1}\Xi x with Ξ=KM\Xi =K-M^\top, and its stationary energy is E|γmin|2=tr(C1ΞVΞ)=C1/2ΞV1/2HS2\E |\gamma _{\min }|^2=\operatorname {tr}(C^{-1}\Xi V\Xi ^\top ) =\|C^{-1/2}\Xi V^{1/2}\|_{\mathrm {HS}}^2. Finiteness of this quantity is a property of the operator and the noise, invariant under changes of factor coordinates; in the block-diagonal isotropic setting it reduces to E<\mathcal E<\infty, with a value independent of the intensities. (iv) Fix a trading horizon H(0,θ)H\in (0,\theta ^*) and take T=HT=H in (a)–(d). At each order take the market of the bank account and 2N2N bonds with fixed maturities Tj(H,θ)T_j\in (H,\theta ^*), so that every bond is alive on [0,H][0,H] with time to maturity in the modelled range, and let the deterministic sector be transported as in Proposition 2.7. The 2N×2N2N\times 2N volatility matrix has entries σnIns(Tjt)\sigma _nI^s_n(T_j-t) and σnInc(Tjt)\sigma _nI^c_n(T_j-t), t[0,H]t\in [0,H]. The 2N2N functions Ins,IncI^s_n,I^c_n (nNn\le N) are linearly independent real-analytic functions on every open interval, since their derivatives are the distinct characters bns,bncb^s_n,b^c_n; so by the evaluation argument in the proof of Theorem 4.6 the matrix is invertible at t=0t=0 for an open dense set of maturity tuples in (H,θ)2N(H,\theta ^*)^{2N}, and, being real-analytic in tt, it is invertible for all but finitely many t[0,H]t\in [0,H], hence dtdt-a.e. On the natural filtration of the 2N2N Brownian motions the market is therefore complete, with QNQ_N as its unique pricing measure. In the singular case nNhn0\prod _{n\le N}\mathfrak h_n\to 0 by Kakutani’s criterion, so the sequences (PN)(P_N) and (QN)(Q_N) are entirely separated; that separation is the criterion for strong asymptotic arbitrage in the sense of [29] (see also [38]). For the model this holds for every H(0,θ)H\in (0,\theta ^*) by (d), and it is a rigorous finite-sequence form of the infinite statement left open below.

The diagnosis is now complete at every finite order. Every nontrivial finite sine truncation of the envelope, equipped with the induced drift, admits no equivalent local martingale measure; once the silent coordinates are loaded, every truncation admits one, at a price that diverges with the truncation order. In the infinite model the factor-law statement is settled on the loaded side, where the laws are mutually singular (Proposition 4.11(b)). The statement for the traded bonds is the open problem of Remark 3.4: it presupposes traded-bond processes that are semimartingales under the cylindrical dynamics. The next section stops asking whether the model is arbitrage-free and constructs the arbitrage-free model that its envelope and its noise admit.

5The arbitrage-free completion and its singular limit

Section 4 returned a verdict. At every finite sine truncation the deformation drift lies outside its volatility span, the defect is realisable in traded bonds, and it does not fade under refinement; once the silent coordinates are loaded, it carries a price that diverges. This section does what the conclusion of [13] asks and turns the verdict into a construction — keep the model’s basis envelope and its noise, repair the drift, and take NN\to \infty to see where the singularity of maturity-white risk reappears. The repair is exact at every NN. What it costs, and at which level its limit lives, are the two results here: a short-end drift discontinuity with an explicit boundary layer, and a limit for the convexity and the bond-return volatilities but none for the curve. Section 6 then asks whether that cost survives the model’s own stochastic spread.

5.1The minimal completion and the exact limit

The repair is a definition: keep the envelope of Proposition 4.1 and the sine-only noise, and impose the drift that Proposition 2.7 requires.

Definition 5.1 (Completion) . Fix κ,θ,σ0>0\kappa ,\theta ^*,\sigma _0>0 and N1N\ge 1. The NN-block completion is the model of Assumption 2.6 with basis B=nN2θeτ/κ(sinωnτ, cosωnτ)\B =\bigoplus _{n\le N}\sqrt {\frac 2{\theta ^*}}\,e^{-\tau /\kappa } \bigl (\sin \omega _n\tau ,\ \cos \omega _n\tau \bigr )^\top, generating matrix M=nMnM=\bigoplus _nM_n, factor drift K=MK=M^\top, noise loading only on the sine coordinates with intensity σ0\sigma _0 (so C=nσ02diag(1,0)C=\bigoplus _n\sigma _0^2\operatorname {diag}(1,0) — exactly the model’s sources of randomness), and φt\varphi _t transported by (6) with qtN=qNq_t^N=q^N below. By Proposition 2.7 each completion is arbitrage-free.

The cosine coordinates carry no noise but are excited through the rotation in MM^\top; the completion is a 2N2N-dimensional Gaussian factor HJM model. Its convexity is qN(τ)=B(τ)CI(τ)=nNqn(τ)q^N(\tau )=\B (\tau )^\top C\,\Iv (\tau )=\sum _{n\le N}q_n(\tau ). Per block only the sine coordinate is loaded, so qn(τ)=σ02bns(τ)0τbns(u)duq_n(\tau )=\sigma _0^2\,b_n^s(\tau )\int _0^\tau b_n^s(u)\,du with bns(τ)=2/θeτ/κsinωnτb_n^s(\tau )=\sqrt {2/\theta ^*}\,e^{-\tau /\kappa }\sin \omega _n\tau, and the standard exponential–trigonometric integral gives the closed form

(23)qn(τ)=2σ02θeτ/κκ2+ωn2[ωnsinωnτeτ/κκsin2ωnτωneτ/κsinωnτcosωnτ].\begin{equation}\label {eq:qn} q_n(\tau )=\frac {2\sigma _0^2}{\theta ^*}\cdot \frac {e^{-\tau /\kappa }}{\kappa ^{-2}+\omega _n^2} \Bigl [\omega _n\sin \omega _n\tau -\frac {e^{-\tau /\kappa }}\kappa \sin ^2\omega _n\tau -\omega _ne^{-\tau /\kappa }\sin \omega _n\tau \cos \omega _n\tau \Bigr ]. \end{equation}

Theorem 5.2 (Exact completion limit) . For every κ,θ,σ0>0\kappa ,\theta ^*,\sigma _0>0 and every τ(0,θ)\tau \in (0,\theta ^*),

(24) limNqN(τ)=q(τ)=σ022e2τ/κ \begin{equation}\label {eq:limit} \boxed {\ \lim _{N\to \infty }q^N(\tau )=q^\infty (\tau )=\frac {\sigma _0^2}2\,e^{-2\tau /\kappa }\ } \end{equation}
— independent of θ\theta ^* — with convergence uniform on compact subsets of (0,θ)(0,\theta ^*). Meanwhile qN(0)=0q^N(0)=0 for every NN (as any HJM drift must satisfy at τ=0\tau =0), so the limit has a jump q(0+)=σ02/2q^\infty (0^+)=\sigma _0^2/2: the convergence develops a Gibbs boundary layer at the short end with universal profile
(25)qN(uθNπ)  σ02G(u),G(u):=2π[Si(u)12Si(2u)],\begin{equation}\label {eq:profile} q^N\!\Bigl (\frac {u\,\theta ^*}{N\pi }\Bigr )\ \longrightarrow \ \sigma _0^2\,G(u),\qquad G(u):=\frac 2\pi \Bigl [\Si (u)-\tfrac 12\Si (2u)\Bigr ], \end{equation}
uniformly on compacts of [0,)[0,\infty ). The limiting profile has a strict first local maximum at u=πu=\pi, of height
σ02G(π)=2π[Si(π)12Si(2π)]σ02=0.727568σ02=1.45514×q(0+),\sigma _0^2\,G(\pi ) =\frac 2\pi \Bigl [\Si (\pi )-\tfrac 12\Si (2\pi )\Bigr ]\sigma _0^2 =0.727568\,\sigma _0^2=1.45514\times q^\infty (0^+),
in the following precise local sense: for fixed 0<a<π<b<2π0<a<\pi <b<2\pi, every maximiser uNu_N of uqN(uθ/(Nπ))u\mapsto q^N(u\theta ^*/(N\pi )) on [a,b][a,b] satisfies uNπu_N\to \pi, and its value converges to σ02G(π)\sigma _0^2G(\pi ).

Proof.Write Δn=κ2+ωn2\Delta _n=\kappa ^{-2}+\omega _n^2, use sin2=12(1cos2ωnτ)\sin ^2=\frac 12(1-\cos 2\omega _n\tau ), sincos=12sin2ωnτ\sin \cos =\frac 12\sin 2\omega _n\tau, and sum (23) against the three classical series (Fourier expansions of the sawtooth and of hyperbolic functions on the lattice ωn=nπ/θ\omega _n=n\pi /\theta ^*; e.g. Gradshteyn–Ryzhik 1.441–1.445):

S1(x):=n1ωnsinωnxΔn=θsinhθxκ2sinhθκ,S2(x):=n1cosωnxΔn=κθcoshθxκ2sinhθκκ22,S_1(x):=\sum _{n\ge 1}\frac {\omega _n\sin \omega _nx}{\Delta _n} =\frac {\theta ^*\sinh \frac {\theta ^*-x}\kappa }{2\sinh \frac {\theta ^*}\kappa },\qquad S_2(x):=\sum _{n\ge 1}\frac {\cos \omega _nx}{\Delta _n} =\frac {\kappa \theta ^*\cosh \frac {\theta ^*-x}\kappa }{2\sinh \frac {\theta ^*}\kappa }-\frac {\kappa ^2}2,
valid for 0<x<2θ0<x<2\theta ^* (resp. 0x2θ0\le x\le 2\theta ^*), and S3:=S2(0)S_3:=S_2(0). Then
q(τ)=2σ02θeτ/κ[S1(τ)eτ/κ2κ(S3S2(2τ))eτ/κ2S1(2τ)],q^\infty (\tau )=\frac {2\sigma _0^2}{\theta ^*}e^{-\tau /\kappa } \Bigl [S_1(\tau )-\frac {e^{-\tau /\kappa }}{2\kappa }\bigl (S_3-S_2(2\tau )\bigr ) -\frac {e^{-\tau /\kappa }}2S_1(2\tau )\Bigr ],
the doubled arguments requiring τ<θ\tau <\theta ^*. Elementary hyperbolic algebra (set u=τ/κu=\tau /\kappa, y=θ/κy=\theta ^*/\kappa; the sum telescopes to [ey2uey2u]/(4sinhy)\bigl [e^{y-2u}-e^{-y-2u}\bigr ]/(4\sinh y), whose numerator factors as 2e2usinhy2e^{-2u}\sinh y, leaving 12e2u\frac 12e^{-2u}) collapses every θ\theta ^*-dependent term and yields (24). Convergence: after the trigonometric reduction the tails are of two kinds. The absolutely convergent ones have O(Δn1)=O(n2)O(\Delta _n^{-1})=O(n^{-2}) coefficients. The conditionally convergent ones have coefficients ωn/Δn\omega _n/\Delta _n, monotone 0\to 0 after finitely many terms, against sinωnx\sin \omega _nx, whose partial sums are bounded uniformly for xx in compact subsets of (0,2θ)(0,2\theta ^*); Dirichlet’s test then gives uniform convergence on compacts of (0,θ)(0,\theta ^*). At τ=0\tau =0 every term of (23) vanishes; at τ=θ\tau =\theta ^* every sinωnθ=0\sin \omega _n\theta ^*=0, so qN(θ)=0q(θ)q^N(\theta ^*)=0\neq q^\infty (\theta ^{*-}).

(Layer profile.) Put

a:=κ1,h:=πθ,x:=hτ=uN;a:=\kappa ^{-1},\qquad h:=\frac {\pi }{\theta ^*},\qquad x:=h\tau =\frac {u}{N};
thus ωn=hn\omega _n=hn and τ=u/(Nh)\tau =u/(Nh). Fix U<U<\infty and let 0uU0\le u\le U. The elementary bounds
|sin(nx)|nUN,|sin(2nx)|2nUN,|\sin (nx)|\le \frac {nU}{N},\qquad |\sin (2nx)|\le \frac {2nU}{N},
give
nN|ωna2+ωn21ωn|(|sin(nx)|+|sin(2nx)|)3a2Uh3Nn11n2=OU(N1),nNsin2(nx)a2+ωn2U2h2N.\begin{align*} &\sum _{n\le N} \left | \frac {\omega _n}{a^2+\omega _n^2}-\frac 1{\omega _n} \right | \bigl (|\sin (nx)|+|\sin (2nx)|\bigr ) \\ &\hspace {25mm}\le \frac {3a^2U}{h^3N}\sum _{n\ge 1}\frac 1{n^2} =O_U(N^{-1}), \\ &\sum _{n\le N}\frac {\sin ^2(nx)}{a^2+\omega _n^2} \le \frac {U^2}{h^2N}. \end{align*}

Here we used

|ωna2+ωn21ωn|=a2ωn(a2+ωn2)a2h3n3.\left | \frac {\omega _n}{a^2+\omega _n^2}-\frac 1{\omega _n} \right | =\frac {a^2}{\omega _n(a^2+\omega _n^2)} \le \frac {a^2}{h^3n^3}.
Moreover,
|eaτ1|aτaUhN,nN|sin(nx)|+|sin(2nx)|n3U.|e^{-a\tau }-1|\le a\tau \le \frac {aU}{hN}, \qquad \sum _{n\le N}\frac {|\sin (nx)|+|\sin (2nx)|}{n}\le 3U.
Applying these estimates term by term to (23) yields, uniformly for u[0,U]u\in [0,U],
(26)qN(uθNπ)=σ022πnNsin(nu/N)12sin(2nu/N)n+OU(N1).\begin{equation}\label {eq:layerapprox} q^N\!\left (\frac {u\theta ^*}{N\pi }\right ) =\sigma _0^2\,\frac 2\pi \sum _{n\le N}\frac {\sin (nu/N)-\frac 12\sin (2nu/N)}{n} +O_U(N^{-1}). \end{equation}
For
gu(y):={sin(uy)/y,y>0,u,y=0,g_u(y):= \begin {cases} \sin (uy)/y,&y>0,\\ u,&y=0, \end {cases}
the family {gu:0uU}\{g_u:0\le u\le U\} has uniformly bounded first derivatives on [0,1][0,1]. Hence its right Riemann sums satisfy
nNsin(nu/N)n=1NnNgu(n/N)=01gu(y)dy+OU(N1)=Si(u)+OU(N1),\sum _{n\le N}\frac {\sin (nu/N)}n =\frac 1N\sum _{n\le N}g_u(n/N) =\int _0^1g_u(y)\,dy+O_U(N^{-1}) =\Si (u)+O_U(N^{-1}),
uniformly for u[0,U]u\in [0,U]; applying the same argument with 2u2u gives
nNsin(2nu/N)n=Si(2u)+OU(N1).\sum _{n\le N}\frac {\sin (2nu/N)}n =\Si (2u)+O_U(N^{-1}).
Substitution in (26) proves
qN(uθNπ)σ022π[Si(u)12Si(2u)]q^N\!\left (\frac {u\theta ^*}{N\pi }\right ) \longrightarrow \sigma _0^2\,\frac 2\pi \left [\Si (u)-\frac 12\Si (2u)\right ]
uniformly on compact subsets of [0,)[0,\infty ). Since G(u)=2πsinu(1cosu)uG'(u)=\frac 2\pi \,\frac {\sin u\,(1-\cos u)}u is positive on (0,π)(0,\pi ) and negative on (π,2π)(\pi ,2\pi ), u=πu=\pi is the unique maximiser on every fixed interval [a,b][a,b] as in the statement. Uniform convergence and the standard argmax lemma give the asserted convergence of the window-restricted maximisers and values; the conclusion is local to the window [a,b][a,b] of the statement.

The θ\theta ^*-independence of the short-end value has a one-line explanation. In the layer the leading sums are the sawtooth series n1sin(nx)/n=πx2\sum _{n\ge 1}\sin (nx)/n=\frac {\pi -x}2 and n1sin(2nx)/n=π2x2\sum _{n\ge 1}\sin (2nx)/n=\frac {\pi -2x}2 for x(0,π)x\in (0,\pi ), and 2π[πx2π2x4]=12\frac 2\pi \bigl [\frac {\pi -x}2-\frac {\pi -2x}4\bigr ]=\frac 12 identically: the xx-dependence cancels, which is the sawtooth form of the θ\theta ^*-independence of q(0+)q^\infty (0^+).

The two constants deserve comment. The relative first-layer peak 1.455141.45514 exceeds the classical Wilbraham–Gibbs value 2πSi(π)=1.17898\frac 2\pi \Si (\pi )=1.17898 for a plain jump. The reason is that Si(2π)\Si (2\pi ) is the first local minimum of Si\Si: the second harmonic reaches its maximal downward excursion exactly where the first peaks, and the two excursions reinforce rather than cancel. And a corresponding far-end discontinuity is recorded in Remark 6.6: the two one-sided limits at τ=θ\tau =\theta ^* are ±σ022e2θ/κ\pm \frac {\sigma _0^2}2e^{-2\theta ^*/\kappa } — a full jump of size σ02e2θ/κ\sigma _0^2e^{-2\theta ^*/\kappa } — while qN(θ)=0q^N(\theta ^*)=0 for every NN.

Remark 5.3 (Interpretation: the drift cost of the minimal completion) . Three readings of Theorem 5.2. (i) Kennedy’s half-delta is exact at finite span. For a random-field HJM with spatial covariance kernel c(τ1,τ2)c(\tau _1,\tau _2), the formal drift condition is α(τ)=0τc(τ,u)du\alpha (\tau )=\int _0^\tau c(\tau ,u)\,du [332239]. The cylindrical noise has c(τ,u)=σ02e2u/κδ(τu)c(\tau ,u)=\sigma _0^2e^{-2u/\kappa }\delta (\tau -u) distributionally (completeness of (8) in the weighted space), and integrating a boundary delta with half its mass gives exactly σ022e2τ/κ\frac {\sigma _0^2}2e^{-2\tau /\kappa }. The completion theorem turns this formal computation into a rigorous limit statement — and shows the finite-θ\theta ^* corrections cancel identically, which the heuristic does not predict. (ii) The jump is the shadow of Proposition 3.3. The same white-in-maturity noise that destroys pointwise semimartingality shows up, after finite-dimensional repair and passage to the limit, as an irremovable σ02/2\sigma _0^2/2 discontinuity of the short-end drift. Arbitrage-free approximants exist at every NN, but their drifts develop a boundary layer of width θ/N\theta ^*/N rather than converging smoothly. Within this selected completion, maturity-local volatility therefore entails a singular short-end HJM drift cost. (iii) Non-uniqueness of the completion is quantifiable. Loading noise isotropically on both coordinates (C=σ0212C=\sigma _0^2\one _2 per block) gives instead, again as the first-span interior limit on 0<τ<θ0<\tau <\theta ^*,

qiso(τ)=σ02[e2τ/κ+κθ(e2τ/κeτ/κ)].q^{\mathrm {iso}}_\infty (\tau )=\sigma _0^2\left [e^{-2\tau /\kappa } +\frac \kappa {\theta ^*}\left (e^{-2\tau /\kappa }-e^{-\tau /\kappa }\right )\right ].
Indeed, adding the cosine-loaded analogue of (23) to the sine-loaded term and using the same series S1,S2,S3S_1,S_2,S_3 as in the proof of Theorem 5.2 gives
qiso(τ)=2σ02θ{eτ/κ[S1(τ)+κ1S2(τ)]κ1e2τ/κS3}.q^{\mathrm {iso}}_\infty (\tau ) =\frac {2\sigma _0^2}{\theta ^*} \left \{e^{-\tau /\kappa } \left [S_1(\tau )+\kappa ^{-1}S_2(\tau )\right ] -\kappa ^{-1}e^{-2\tau /\kappa }S_3\right \}.
The identities
S1(τ)+κ1S2(τ)=θe(θτ)/κ2sinh(θ/κ)κ2,κ1S3=θ2coth(θ/κ)κ2S_1(\tau )+\kappa ^{-1}S_2(\tau ) =\frac {\theta ^*e^{(\theta ^*-\tau )/\kappa }} {2\sinh (\theta ^*/\kappa )}-\frac \kappa 2, \qquad \kappa ^{-1}S_3 =\frac {\theta ^*}{2}\coth (\theta ^*/\kappa )-\frac \kappa 2
reduce this expression to the displayed formula. It has the doubled short-end jump σ02\sigma _0^2, a genuine O(κ/θ)O(\kappa /\theta ^*) span correction, and changes sign when τ>κlog(1+θ/κ)\tau >\kappa \log (1+\theta ^*/\kappa ). The completion is a choice; the sine-only one is canonical in that it adds no sources of randomness to [13]. The layer profile is likewise a property of the sharp sine cutoff of Definition 5.1: smoothed truncations (Fejér and its relatives) damp or remove the overshoot, so the Gibbs constant belongs to the completion choice, not to the limit.

5.2No curve-valued limit

The convexity density converges; the curve laws do not, and not merely in stationarity. The next statement makes this quantitative, and identifies what does survive: the bond-level functionals.

Proposition 5.4 (No curve-level limit for the equal-intensity completion) . Start each completion from a deterministic factor state, or more generally from an initial state independent of its future Brownian noise. For every fixed t>0t>0 and block nn, the covariance contributed by the stochastic convolution is

Vn(t)=0teKnsCneKnsds=σ02κ4(1e2t/κ)12+Rn(t),Rn(t)=Ot(ωn1).V_n(t)=\int _0^t e^{K_ns}C_ne^{K_n^\top s}\,ds =\frac {\sigma _0^2\kappa }{4}(1-e^{-2t/\kappa })\one _2+R_n(t), \qquad \|R_n(t)\|=O_t(\omega _n^{-1}).
Consequently, at every fixed τ0\tau \ge 0, the stochastic-convolution contribution satisfies
VarconvftN(τ)=σ02κ2θ(1e2t/κ)Ne2τ/κ+Ot(logN)  ,\operatorname {Var}_{\mathrm {conv}}f_t^N(\tau )= \frac {\sigma _0^2\kappa }{2\theta ^*}(1-e^{-2t/\kappa }) N e^{-2\tau /\kappa }+O_t(\log N)\ \longrightarrow \ \infty ,
and, whenever the initial state has a finite second moment, the total variance is at least this quantity, with equality for deterministic initial states. The non-tightness conclusion itself needs no moment assumption — only independence. The point-evaluation laws are therefore not tight, and neither are the curve laws in HwH_w, since evaluation is continuous there. In stationarity the same formulas hold with (1e2t/κ)(1-e^{-2t/\kappa }) replaced by 11. Bond-level functionals survive: Σ(τ)2=|C1/2BI(τ)|2\|\Sigma (\tau )\|^2=|C^{1/2}\B _I(\tau )|^2 is NN-uniformly finite.

Proof.Since Kn=κ112K_n=-\kappa ^{-1}\one _2 plus a skew-symmetric rotation generator, eKnsCneKnse^{K_ns}C_ne^{K_n^\top s} is e2s/κe^{-2s/\kappa } times a rotation of Cn=σ02diag(1,0)C_n=\sigma _0^2\operatorname {diag}(1,0). Its nonoscillatory part is σ022e2s/κ12\frac {\sigma _0^2}{2}e^{-2s/\kappa }\one _2, whose integral gives the displayed scalar term; integration of the sine and cosine terms of frequency 2ωn2\omega _n gives Rn(t)=Ot(ωn1)\|R_n(t)\|=O_t(\omega _n^{-1}). Now Bn(τ)12Bn(τ)=(2/θ)e2τ/κ\B _n(\tau )^\top \one _2\B _n(\tau )=(2/\theta ^*)e^{-2\tau /\kappa } and nNωn1=O(logN)\sum _{n\le N}\omega _n^{-1}=O(\log N). Independence of the initial state and future noise makes covariances additive, proving the variance bound. For the bond-level claim, Ins(τ)=O(ωn1)I_n^s(\tau )=O(\omega _n^{-1}) uniformly on compacts, so n|Ins(τ)|2<\sum _n|I_n^s(\tau )|^2<\infty uniformly in NN. Finally, convolution with a centred Gaussian of variance tending to infinity has concentration on every interval of fixed length tending to zero; therefore no choice of independent initial law can restore pointwise tightness.

Figure 2: (a) Factor autocorrelation on block \(n=2\) ( \(\kappa =4\) , \(\theta ^*=30\) ): the arbitrage-free dynamics \(e^{M_n^\top h}\) spirals (decay \(1/\kappa \) , rotation \(\omega _n\) ), the model’s \(e^{-\lambda _nh}\) decays along a ray. This is Corollary 4.5 in a picture. (b) The
completion’s convexity: partial sums \(q^N\) against the exact limit \(\frac {\sigma _0^2}2e^{-2\tau /\kappa }\) ; every \(q^N\) vanishes at \(\tau =0\) while the
limit jumps to \(\sigma _0^2/2\) ; the Gibbs layer narrows as \(\theta ^*/N\) . The layer has the universal profile \(\sigma _0^2\,G(N\pi \tau /\theta ^*)\) , \(G(u)=\frac 2\pi [\Si (u)-\tfrac 12\Si (2u)]\) , with
reinforced first-layer peak \(1.455\times \sigma _0^2/2\) near \(\tau =\theta ^*/N\) (Theorem 5.2 ). (c) The two arbitrage-free completions of
Remark 5.3 (iii).
Figure 2. (a) Factor autocorrelation on block n=2n=2 (κ=4\kappa =4, θ=30\theta ^*=30): the arbitrage-free dynamics eMnhe^{M_n^\top h} spirals (decay 1/κ1/\kappa, rotation ωn\omega _n), the model’s eλnhe^{-\lambda _nh} decays along a ray. This is Corollary 4.5 in a picture. (b) The completion’s convexity: partial sums qNq^N against the exact limit σ022e2τ/κ\frac {\sigma _0^2}2e^{-2\tau /\kappa }; every qNq^N vanishes at τ=0\tau =0 while the limit jumps to σ02/2\sigma _0^2/2; the Gibbs layer narrows as θ/N\theta ^*/N. The layer has the universal profile σ02G(Nπτ/θ)\sigma _0^2\,G(N\pi \tau /\theta ^*), G(u)=2π[Si(u)12Si(2u)]G(u)=\frac 2\pi [\Si (u)-\tfrac 12\Si (2u)], with reinforced first-layer peak 1.455×σ02/21.455\times \sigma _0^2/2 near τ=θ/N\tau =\theta ^*/N (Theorem 5.2). (c) The two arbitrage-free completions of Remark 5.3(iii).

The mechanism is structural. The arbitrage-free repair replaces the model’s decay λnn2\lambda _n\asymp n^2 by the uniform 1/κ1/\kappa, and with it goes the mode-variance summability that made the cylindrical field function-valued (Proposition 3.2). What converges is the convexity density (Theorem 5.2) and the bond-return volatility structure: the limit lives at the level of bonds, not of the curve. A distribution-valued or bond-level limit model — traded-bond semimartingales, an equivalent martingale measure, cross-maturity consistency — is the natural next object, and is the first open problem of §7.3. Thus, within this equal-amplitude cylindrical sine refinement and its minimal finite-dimensional HJM completion, the calculation exhibits a trilemma: retaining the maturity-local noise, imposing no-arbitrage at every truncation, and obtaining a function-valued refinement limit — any two. For the completion, factor count is therefore economically consequential rather than a numerical grid parameter: bond-return volatility functionals remain controlled, whereas instantaneous forward-curve laws do not stabilize under refinement.

The third corner of the trilemma is not empty, and Proposition 4.11 says what lives there. Give up the maturity-local noise for the isotropic trace-class loading of §4.7. Then the factor drift MM^\top of the completion carries an HwH_w-valued curve, no-arbitrage holds at every resolution, and the question becomes how much of the model’s curvature term can be kept in the historical drift at a finite price. Let D:=τ+κ1\mathfrak D:=\partial _\tau +\kappa ^{-1}, which acts on the block VnV_n as ωnJ\omega _nJ, and for a scale ν>0\nu >0 (in years) consider the mollified generator, as a formal expression on quasi-exponentials,

A~ν:=τ+κ2τ2eν22D2,pν(zn)=zn+ϖn(p(zn)zn),ϖn:=eν2ωn2/2,\widetilde A_\nu :=\partial _\tau +\frac \kappa 2\,\partial _\tau ^2\,e^{\frac {\nu ^2}2\mathfrak D^2}, \qquad p_\nu (z_n)=z_n+\varpi _n\bigl (p(z_n)-z_n\bigr ),\qquad \varpi _n:=e^{-\nu ^2\omega _n^2/2},

with entire symbol pν(z)=z+κ2z2eν22(z+κ1)2p_\nu (z)=z+\frac \kappa 2z^2e^{\frac {\nu ^2}2(z+\kappa ^{-1})^2}. The definition that carries the mathematics is blockwise: Kν:=npν(Mn)K_\nu :=\bigoplus _np_\nu (M_n)^\top, and by the block calculus of §4.7 pν(Mn)=(1ϖn)Mn+ϖnp(Mn)p_\nu (M_n)^\top =(1-\varpi _n)\,M_n^\top +\varpi _n\,p(M_n)^\top, the convex combination of transport and the model’s drift. The multiplier has a reading in the model’s own terms: since κ2D2=A~+12κ\frac \kappa 2\mathfrak D^2=\widetilde A+\frac 1{2\kappa } as formal expressions, eν22D2e^{\frac {\nu ^2}2\mathfrak D^2} is eν2/(2κ2)e^{\nu ^2/(2\kappa ^2)} times the formal flow e(ν2/κ)A~e^{(\nu ^2/\kappa )\widetilde A}, so the curvature penalty is applied to the curve after the cylindrical flow has acted on it for ν2/κ\nu ^2/\kappa years. This is the formal calculus of §3 on the doubled envelope, not the closed Dirichlet semigroup, which does not preserve the cosine partners; on the sine eigenspaces the two agree. In the notation of (21), |δn(ν)|=ϖnλn|\delta _n(\nu )|=\varpi _n\lambda _n and kn(ν)=κ1dnϖnk_n(\nu )=\kappa ^{-1}-d_n\varpi _n, with kn(ν)12κ=1ϖn2κ+κ2ωn2ϖn>0k_n(\nu )-\frac 1{2\kappa }=\frac {1-\varpi _n}{2\kappa }+\frac \kappa 2\omega _n^2\varpi _n>0, so

EN(ν):=nNϖn2λn2κ1dnϖn,E(ν):=limNEN(ν)<(ν>0),\mathcal E_N(\nu ):=\sum _{n\le N}\frac {\varpi _n^2\lambda _n^2}{\kappa ^{-1}-d_n\varpi _n},\qquad \mathcal E(\nu ):=\lim _{N\to \infty }\mathcal E_N(\nu )<\infty \quad (\nu >0),

and

E(ν)κθ22πν3(ν0).\mathcal E(\nu )\sim \frac {\kappa \theta ^*}{2\sqrt {2\pi }}\,\nu ^{-3}\quad (\nu \to 0).

For the asymptotic, write kn(ν)=an+unk_n(\nu )=a_n+u_n with an:=(1ϖn)/κa_n:=(1-\varpi _n)/\kappa and un:=ϖnλnu_n:=\varpi _n\lambda _n; then en=un2/(an+un)\mathfrak e_n=u_n^2/(a_n+u_n) and 0unenmin(an,un)0\le u_n-\mathfrak e_n\le \min (a_n,u_n). The main term nun=κ2nωn2ϖn+12κnϖn\sum _nu_n=\frac \kappa 2\sum _n\omega _n^2\varpi _n+\frac 1{2\kappa }\sum _n\varpi _n is, up to O(ν2)O(\nu ^{-2}), the Riemann sum with spacing π/θ\pi /\theta ^* of the unimodal function κ2ω2eν2ω2/2\frac \kappa 2\omega ^2e^{-\nu ^2\omega ^2/2}, whose integral is κ2π/2ν3\frac \kappa 2\sqrt {\pi /2}\,\nu ^{-3}, plus an O(ν1)O(\nu ^{-1}) term. The remainder is o(ν3)o(\nu ^{-3}): splitting at ω=L/ν\omega =L/\nu, the blocks below contribute at most anν2ωn2/(2κ)=O(L3ν1)\sum a_n\le \sum \nu ^2\omega _n^2/(2\kappa )=O(L^3\nu ^{-1}), and those above at most un\sum u_n, which is ν3\nu ^{-3} times a Gaussian tail integral that vanishes as LL\to \infty. By Proposition 4.11, for every ν>0\nu >0 the infinite factor laws are equivalent. The mollified curvature term is carried entirely by the historical drift, as an essentially affine risk premium in the sense of Remark 2.10; under the pricing measure the factor drift is the completion’s MM^\top. The symbol test of Theorem 4.3 still fails on every block: the defect is the model’s, scaled by ϖn\varpi _n. Its price is EN(ν)\sqrt {\mathcal E_N(\nu )}, the stationary root-mean-square of the maximal Sharpe ratio the premium commands in the NNth truncated market, with E(ν)\sqrt {\mathcal E(\nu )} its limit (Remark 4.12(ii)). What is bought is modest and exactly measurable: the fraction ϖn\varpi _n of the curvature term kept on block nn. At the reference calibration a Sharpe ratio of 0.40.4 corresponds to ν5.7\nu \approx 5.7 years, where ϖn\varpi _n is 0.840.84, 0.490.49 and 0.200.20 on the 6060-, 3030- and 2020-year modes, 0.060.06 on the 1515-year mode and below 0.020.02 beyond: the curvature penalty survives on the longest wavelengths only. The Gaussian damping is one choice among many: within the block-diagonal class of Proposition 4.11, any blockwise deviation from transport with n|δn|2/kn<\sum _n|\delta _n|^2/k_n<\infty is admissible, and only the ν3\nu ^{-3} asymptotic and the calibration above are specific to ϖn=eν2ωn2/2\varpi _n=e^{-\nu ^2\omega _n^2/2}. Keeping the model’s drift exactly on the two longest modes and transport elsewhere costs as much as ν=4\nu =4 (both give a Sharpe ratio of 0.600.60). What this corner gives up is the cylindrical noise itself: with σnσ0\sigma _n\equiv \sigma _0 the stationary variances σ02/(2kn)\sigma _0^2/(2k_n) do not sum. The short-end cost of Theorem 5.2 therefore does not arise here, and the case for one shock per maturity that motivates the model is met no better than by the completion (§7.3).

5.3The long end

One question remains before the spread is restored. In any arbitrage-free model the long zero-coupon rate, where it exists as a limit, is almost surely nondecreasing [16]; the general rigorous proof is [27]. Does complexification interact with this long-maturity rigidity of Gaussian HJM models? It does not, in either direction.

Proposition 5.5 (DIR and complexification are orthogonal) . In a model of Assumption 2.6:

  1. every stable oscillatory block satisfies |Bb(τ)|Ceδτ0|\B _b(\tau )|\le Ce^{-\delta \tau }\to 0 for some δ>0\delta >0 and has bounded Ib(τ)\Iv _b(\tau ), so 1τIb(τ)Xb,t0\frac 1\tau \Iv _b(\tau )^\top \X _{b,t}\to 0: complex modes contribute nothing to the long yield;
  2. with no level mode (kerM=0\ker M=0) the whole factor contribution to the long yield vanishes;
  3. a level mode with Cte00C_te_0\neq 0 — volatility-loaded or cross-loaded, the same condition — has I0(τ)=b0τ\Iv _0(\tau )=b_0\tau and forces qtq_t to grow linearly with slope b02e0Cte0b_0^2e_0^\top C_te_0, the standard Gaussian-HJM long-end pathology; a level mode with Cte00C_te_0\equiv 0 is frozen, and so is its contribution to the long yield.

The long-end behaviour thus depends only on the (generalised) kernel of MM and on how volatility loads it: complexification neither causes nor cures anything at the long end.

Proof.For the model class, consistency holds for every initial state, so Bx=r0φ0Hw\B ^\top x=r_0-\varphi _0\in H_w for every xx, i.e. every component of B\B lies in HwH_w. Controllability makes B(0)\B (0) cyclic for MM (Lemma 2.4), so each Jordan cell of MM contributes its top chain function to the components of B\B; HwH_w-membership (§2.1) then excludes exponents with Reλ>0\operatorname {Re}\lambda >0, undamped oscillations, and any Jordan tail over the kernel. Hence, in real Jordan coordinates, B(τ)=b0e0+Bdec(τ)\B (\tau )=b_0e_0+\B _{\mathrm {dec}}(\tau ): an at most one-dimensional constant level loading on kerM=kergenM\ker M=\ker _{\mathrm {gen}}M, and a strictly stable remainder with |Bdec(τ)|Ceδτ|\B _{\mathrm {dec}}(\tau )|\le Ce^{-\delta \tau } for some δ>0\delta >0.

(i) Oscillatory blocks. They lie in Bdec\B _{\mathrm {dec}}, and MbM_b is invertible (ω0\omega \neq 0), so Ib(τ)=Mb1(eMbτ1)Bb(0)\Iv _b(\tau )=M_b^{-1}(e^{M_b\tau }-\one )\B _b(0) is bounded; for every fixed tt, 1τIb(τ)Xb,t0\frac 1\tau \Iv _b(\tau )^\top \X _{b,t}\to 0 surely. Complex modes contribute nothing to any long-maturity average, in particular not to the long yield.

(ii) No level mode. If kerM=0\ker M=0, the bound applies to all of B\B: I\Iv is bounded and the factor contribution 1τI(τ)Xt\frac 1\tau \Iv (\tau )^\top \X _t vanishes in the limit.

(iii) Level mode. With I(τ)=τb0e0+Idec(τ)\Iv (\tau )=\tau b_0e_0+\Iv _{\mathrm {dec}}(\tau ), Idec:=0τBdec\Iv _{\mathrm {dec}}:=\int _0^\tau \B _{\mathrm {dec}} bounded, and B(τ)=b0e0+O(eδτ)\B (\tau )=b_0e_0+O(e^{-\delta \tau }),

qt(τ)=B(τ)CtI(τ)=τb02e0Cte0+o(τ).q_t(\tau )=\B (\tau )^\top C_t\Iv (\tau )=\tau \,b_0^2\,e_0^\top C_te_0+o(\tau ).
Since Ct0C_t\succeq 0, e0Cte0=|Σte0|2e_0^\top C_te_0=|\Sigma _t^\top e_0|^2 vanishes exactly when Cte0=0C_te_0=0: volatility-loaded and cross-loaded are the same condition, and there is no third case. If 0te0Cse0ds>0\int _0^te_0^\top C_se_0\,ds>0, (6) gives φt\varphi _t a term linear in τ\tau with that integral times b02b_0^2 as slope. The curve then leaves HwH_w (nonconstant affine tails have infinite norm, Theorem 4.3(b)), and the long yield limτ1τ0τft\lim _\tau \frac 1\tau \int _0^\tau f_t is ++\infty for such tt: the standard Gaussian-HJM long-end explosion, of which the Ho–Lee check (Remark 2.9) is the n=1n=1 instance. If instead Cte00C_te_0\equiv 0, then also e0Ct0e_0^\top C_t\equiv 0, every term of qtq_t containing the level direction dies, and qt(τ)=Bdec(τ)CtIdec(τ)=O(eδτ)q_t(\tau )=\B _{\mathrm {dec}}(\tau )^\top C_t\Iv _{\mathrm {dec}}(\tau )=O(e^{-\delta \tau }). Moreover the level factor is constant in time (dx0=e0MXdt+e0ΣtdW=0dx_0=e_0^\top M^\top \X \,dt+e_0^\top \Sigma _t\,d\W =0 because Me0=0Me_0=0 and Σte0=0\Sigma _t^\top e_0=0), so the long yield exists and is frozen: trivially consistent with [16], with nothing left for the pathology to act on.

Every statement above depends only on kerM\ker M and on Cte0C_te_0; no oscillatory quantity enters any of them. That is the orthogonality claim.

Remark 5.6 . The finite θmax\theta _{\max } of [13] is a deliberate choice made precisely to sidestep the θ\theta \to \infty regime, with [16] cited; on a compact maturity interval the theorem does not apply. The accurate statement is conditional: the stationary Gaussian structure does not extend to θmax=\theta _{\max }=\infty, and [13] calls the limit “not innocent.”

That completes the analysis at fixed spread intensity: the model is repaired at every NN, the cost of the repair — its HJM convexity, in the sense of Remark 5.3 — is computed exactly, and the refinement limit is characterised and shown not to be a curve. One feature has been held fixed throughout — the spread that multiplies the deformation — and the next section restores it, to see whether the cost survives.

6The cost survives the stochastic spread

The model multiplies its deformation by a stochastic spread sts_t; §§45 held that spread fixed, and the obvious objection to Theorem 5.2 is that its exact cost is an artefact of freezing it. This section restores the spread and shows that it is not. The algebra closes in two conventions. In the affine convention the squared intensity vt=st2v_t=s_t^2 is a CIR factor and the deformation is conditionally Gaussian (§§6.16.4). There the short-end coefficient σ02/2-\sigma _0^2/2 is conserved at every vol-of-vol, unrenormalised (Theorem 6.4), and what stochastic intensity costs instead is an existence boundary, exact for the infinite-span surrogate (Theorem 6.5). In the bilinear completion convention, (st,Xt)(s_t,\X _t) is jointly Gaussian, the product stXts_t\X _t is represented literally as a quadratic state, and the closure is studied under an explicit recovery normalization (§§6.56.7; Remark 6.13 records what the normalization leaves aside). There no-arbitrage locks the generator and requires spread mean reversion to be slower than the target deformation decay (Theorem 6.12), and the same short-end coefficient is recovered on the η=0\eta =0 slice (Proposition 6.15). Existence of the finite-dimensional coefficient system at each truncation is decided by a determinant (Proposition 6.16); the short-end value at positive vol-of-vol is the open problem of §7.3. The affine convention answers the objection: in its uncorrelated form the short-end coefficient belongs to the maturity-local noise. Intensity scales it and adds its own terms away from the short end, but does not renormalise it, while the rest of the loading and its existence domain do change with the intensity. The bilinear convention makes visible what no-arbitrage demands of the spread itself.

6.1The affine completion and its closure

The first convention makes the squared intensity vt=st2v_t=s_t^2 a CIR factor, so that the deformation is conditionally Gaussian and the closure of §5 can be redone with a stochastic source. Statements are at general NN because the X\X-sector closure is block-diagonal and the vv-sector is scalar with additive source: the one-block calculation extends by summation.

Assumption 6.1 (Affine completion) . Fix NN and the data of Definition 5.1. The curve family is

ft(τ)=φt(τ)+ψ(τ)vt+B(τ)Xt,f_t(\tau )=\varphi _t(\tau )+\psi (\tau )\,v_t+\B (\tau )^\top \X _t,
with φt\varphi _t deterministic, ψC1\psi \in C^1, ψ(0)=0\psi (0)=0 (a normalisation; Remark 6.9), and dynamics
dXt=KXtdt+vtΣdWt,dvt=λ(v¯vt)dt+ηvtdZt,d\X _t=K\X _t\,dt+\sqrt {v_t}\,\Sigma \,d\W _t,\qquad dv_t=\lambda (\bar v-v_t)\,dt+\eta \sqrt {v_t}\,dZ_t,
λ,v¯>0\lambda ,\bar v>0, 2λv¯η22\lambda \bar v\ge \eta ^2 (Feller), Σ\Sigma the sine-only loading of Definition 5.1, and dWsinn,Zt=ρndtd\langle W^n_{\sin },Z\rangle _t=\rho _n\,dt with nρn21\sum _n\rho _n^2\le 1. Normalise v¯=1\bar v=1, so the frozen completion is recovered as η0\eta \to 0, v0=1v_0=1. This fixes the reference initialisation; consistency in Proposition 6.2 means that the drift identity holds for every initial (x,v)(x,v) in a nonempty open subset of R2N×(0,)\R ^{2N}\times (0,\infty ).

Proposition 6.2 (Closure; conditional locking) . Write bns(τ)=2/θeτ/κsinωnτb^s_n(\tau )=\sqrt {2/\theta ^*}\,e^{-\tau /\kappa }\sin \omega _n\tau, Ins(τ)=0τbnsI^s_n(\tau )=\int _0^\tau b^s_n, and Ψ(τ):=0τψ\Psi (\tau ):=\int _0^\tau \psi. The model of Assumption 6.1 satisfies the drift condition (3), with the preceding every-initial-state consistency quantifier, if and only if

  1. K=MK=M^\top;
  2. ψ\psi solves

    (27)ψ(τ)=λψ(τ)qN(τ)η2ψ(τ)Ψ(τ)ησ0nNρn[bns(τ)Ψ(τ)+ψ(τ)Ins(τ)];\begin{equation}\label {eq:psiode} \psi '(\tau )=-\lambda \psi (\tau )-q^N(\tau )-\eta ^2\psi (\tau )\Psi (\tau ) -\eta \sigma _0\sum _{n\le N}\rho _n\bigl [b^s_n(\tau )\Psi (\tau )+\psi (\tau )I^s_n(\tau )\bigr ]; \end{equation}
  3. φ˙t(τ)=φt(τ)λv¯ψ(τ)\dot \varphi _t(\tau )=\varphi _t'(\tau )-\lambda \bar v\,\psi (\tau ).

For ρ=0\rho =0 the integrated form of (27) is the CIR-type Riccati

(28)Ψ=λΨη22Ψ2QN,QN(τ):=0τqN(s)ds.\begin{equation}\label {eq:riccati} \Psi '=-\lambda \Psi -\frac {\eta ^2}2\Psi ^2-Q^N,\qquad Q^N(\tau ):=\int _0^\tau q^N(s)\,ds. \end{equation}
Spectral locking survives conditionally: specK=specM\operatorname {spec}K=\operatorname {spec}M on the deformation sector, so Corollary 4.5’s signature holds for the conditionally Gaussian factors, with one additional real eigenvalue λ-\lambda, which does not precess (Proposition 6.8).

Proof.Volatility matching gives σt(τ)=vt(B(τ)Σ, ηψ(τ))\sigma _t(\tau )=\sqrt {v_t}\,\bigl (\B (\tau )^\top \Sigma ,\ \eta \psi (\tau )\bigr ), so the required drift (3) is vt[qN+η2ψΨ+ησ0nρn(bnsΨ+ψIns)]v_t\bigl [q^N+\eta ^2\psi \Psi +\eta \sigma _0\sum _n\rho _n(b^s_n\Psi +\psi I^s_n)\bigr ] — linear in vtv_t with no constant part, consistent with the diffusion vanishing at v=0v=0. The model’s drift is φ˙t+λ(v¯vt)ψ+BKXt\dot \varphi _t+\lambda (\bar v-v_t)\psi +\B ^\top K\X _t, while (2) demands φt+ψvt+BMXt+αt\varphi _t'+\psi 'v_t+\B ^\top M^\top \X _t+\alpha _t. Matching X\X-linear terms forces K=MK=M^\top exactly as in Proposition 2.7 (consistency in the state, then Lemma 2.4), and vv-linear terms give (27). Deterministic terms give (iii), whose solution is φt(τ)=φ0(τ+t)λv¯0tψ(τ+ts)ds\varphi _t(\tau )=\varphi _0(\tau +t)-\lambda \bar v\int _0^t\psi (\tau +t-s)\,ds; the mean intensity feeds the loading through the deterministic sector, and no global sign of ψ\psi is needed. Blocks are additive in both the X\X-matching and the source of (27), which reduces general NN to N=1N=1.

Remark 6.3 (Consistency; strictness) . (i) At η=0\eta =0, λ=0\lambda =0: vv0v\equiv v_0 and ψ=0τqN\psi =-\int _0^\tau q^N; the identity ψ(τ)ψ(τ+t)=ττ+tqN(s)ds\psi (\tau )-\psi (\tau +t)=\int _\tau ^{\tau +t}q^N(s)\,ds (immediate from ψ=0τqN\psi =-\int _0^\tau q^N) shows the static loading v0ψv_0\psi reproduces the transport (6) of the frozen completion exactly — the two constructions are the same model in different coordinates. (ii) At η=0\eta =0, λ>0\lambda >0 (deterministic time-varying intensity, still inside Proposition 2.7’s class), ψN=0τeλ(τs)qN(s)ds\psi ^N=-\int _0^\tau e^{-\lambda (\tau -s)}q^N(s)\,ds is quasi-exponential with exponent set

{λ}  {1κ±iωn}  {2κ}  {2κ±2iωn},\{-\lambda \}\ \cup \ \{-\tfrac 1\kappa \pm i\omega _n\}\ \cup \ \{-\tfrac 2\kappa \}\ \cup \ \{-\tfrac 2\kappa \pm 2i\omega _n\},
the beat lattice of Remark 2.11 plus one intensity mode: the lattice closure under beats — the “structural felicity” — is load-bearing here, keeping the strict realisation finite. (iii) For η0\eta \neq 0, equation (27) is nonlinear and the quasi-exponential closure argument in (ii) no longer applies. The curve family remains finite-dimensional and affine.

6.2The short-end cost under stochastic intensity

With the affine closure in hand, the question is whether the short-end cost of Theorem 5.2 survives the stochastic intensity or is renormalised away by it. It survives, one derivative down.

Theorem 6.4 (The cost is conserved, demoted one derivative, and unrenormalised) . Let ψN\psi ^N solve (27) with source qNq^N, and ψ\psi ^\infty the solution with source q=σ022e2τ/κq^\infty =\frac {\sigma _0^2}2e^{-2\tau /\kappa }, both with ψ(0)=0\psi (0)=0 and the same parameters, with ρ=0\rho =0 for the surrogate comparison. Then:

  1. Let τ\tau _\infty be the maximal existence time of the surrogate Riccati flow driven by qq^\infty, and let τN\tau _N denote the (generally different) maximal time for the finite-NN flow. For every T<min{θ,τ}T<\min \{\theta ^*,\tau _\infty \}, one has τN>T\tau _N>T for all sufficiently large NN and

    sup0τT|ψN(τ)ψ(τ)|0.\sup _{0\le \tau \le T}|\psi ^N(\tau )-\psi ^\infty (\tau )|\longrightarrow 0.
    Thus the θ\theta ^*-independent surrogate is the rigorous loading limit on the first span.
  2. For every finite NN and every admissible ρ\rho, ψN(0)=(ψN)(0)=0\psi ^N(0)=(\psi ^N)'(0)=0. For the ρ=0\rho =0 surrogate, (ψ)(0+)=σ022(\psi ^\infty )'(0^+)=-\frac {\sigma _0^2}2 exactly for every (λ,η,v¯)(\lambda ,\eta ,\bar v). Vol-of-vol does not renormalise this right derivative (a statement at τ=0+\tau =0^+, on the existence interval, which always contains a neighbourhood of 00).
  3. The first boundary layer survives one derivative down: uniformly for uu in compact subsets of [0,)[0,\infty ),

    (ψN)(uθNπ)σ02G(u).(\psi ^N)'\!\left (\frac {u\theta ^*}{N\pi }\right ) \longrightarrow -\sigma _0^2G(u).
    In particular the limiting first-layer profile has a strict local minimum G(π)σ02-G(\pi )\sigma _0^2 at u=πu=\pi.
  4. At η=0\eta =0, ψ(τ)=σ02κ2e2τ/κeλτκλ2\psi ^\infty (\tau )=-\frac {\sigma _0^2\kappa }2\, \frac {e^{-2\tau /\kappa }-e^{-\lambda \tau }}{\kappa \lambda -2}, degenerating to σ022τe2τ/κ-\frac {\sigma _0^2}2\,\tau e^{-2\tau /\kappa } at the resonance λ=2/κ\lambda =2/\kappa.

Proof.(b) is structural: at τ=0+\tau =0^+ every term of (27) except the source vanishes (ψ(0)=Ψ(0)=bns(0)=0\psi (0)=\Psi (0)=b^s_n(0)=0), so ψ(0+)=q(0+)\psi '(0^+)=-q(0^+); qN(0)=0q^N(0)=0 for every NN while q(0+)=σ02/2q^\infty (0^+)=\sigma _0^2/2 (Theorem 5.2). (a) Take ρ=0\rho =0 and set δ=ψNψ\delta =\psi ^N-\psi ^\infty, D=ΨNΨD=\Psi ^N-\Psi ^\infty. Subtracting the two copies of (27) gives not a scalar equation for δ\delta but the linear system

D=δ,δ=(λ+η2ΨN)δη2ψD(qNq),D'=\delta ,\qquad \delta '=-\bigl (\lambda +\eta ^2\Psi ^N\bigr )\delta -\eta ^2\psi ^\infty D-(q^N-q^\infty ),
whose coefficients are bounded on any interval where the two flows exist. The Fourier representation in the proof of Theorem 5.2 gives a uniform bound for the partial sums on [0,T][0,T] and pointwise convergence away from 00; dominated convergence therefore yields qNqq^N\to q^\infty in L1(0,T)L^1(0,T). Gronwall applied to |D|+|δ||D|+|\delta |, together with standard ODE continuation, gives existence through TT for all large NN and the stated uniform convergence. This argument uses T<θT<\theta ^* essentially. (c) In the layer ψN=O(τ)\psi ^N=O(\tau ) and ΨN=O(τ2)\Psi ^N=O(\tau ^2) uniformly on compact uu-windows, so (ψN)=qN+o(1)(\psi ^N)'=-q^N+o(1) and (25) applies with a sign flip. (d) Direct integration of the linear equation ψ=λψq\psi '=-\lambda \psi -q^\infty.

Under the limit, vtq(τ)v_t\,q^\infty (\tau ) is the maturity-white/X\X-sector contribution to the HJM drift. When η>0\eta >0, the full drift also contains the intensity and cross-covariance terms displayed in (27): the source term alone is not the whole instantaneous convexity.

6.3Existence, and what the surrogate costs

A Riccati loading can escape at finite maturity, and the affine completion is usable only where it does not. On an idealised infinite-span source the boundary is exact.

Theorem 6.5 (Existence boundary) . Take ρ=0\rho =0 and, as an idealised infinite-span surrogate, the source q(τ)=σ022e2τ/κq^\infty (\tau )=\frac {\sigma _0^2}2e^{-2\tau /\kappa } on all of [0,)[0,\infty ) — the interior limit of Theorem 5.2 extended beyond the span (Remark 6.6 records the fixed-span correction). The solution of (28) is global on [0,)[0,\infty ) if and only if

λ  ησ0κ/2,equivalentlyλ2  2η2Q,Q:=0q(s)ds=σ02κ4.\lambda \ \ge \ \eta \sigma _0\sqrt {\kappa /2}, \qquad \text {equivalently}\qquad \lambda ^2\ \ge \ 2\eta ^2Q_\infty ,\qquad Q_\infty :=\int _0^\infty q^\infty (s)\,ds=\frac {\sigma _0^2\kappa }4 .
Below the boundary, Ψ\Psi \downarrow -\infty at a finite τ(λ,η)\tau ^*(\lambda ,\eta ), and bond prices — exponential-affine with vv-exponent Ψ(τ)-\Psi (\tau ) — are infinite for maturities beyond τ\tau ^*; τ\tau ^*\uparrow \infty as λησ0κ/2\lambda \uparrow \eta \sigma _0\sqrt {\kappa /2}. The criterion is the CIR exponential-moment condition for E[exp(Q0vsds)]<\E \bigl [\exp \bigl (Q_\infty \int _0^\cdot v_s\,ds\bigr )\bigr ]<\infty; see [4] for the moment criterion.

Proof.Φ:=Ψ0\Phi :=-\Psi \ge 0 satisfies Φ=η22Φ2λΦ+Q(τ)\Phi '=\frac {\eta ^2}2\Phi ^2-\lambda \Phi +Q(\tau ) with Q(τ)=0τqQQ(\tau )=\int _0^\tau q^\infty \uparrow Q_\infty. If η=0\eta =0, this is a linear equation and is global. Assume henceforth η>0\eta >0. If λ22η2Q\lambda ^2\ge 2\eta ^2Q_\infty, the autonomous majorant with source QQ_\infty has fixed points Φ±=[λ±λ22η2Q]/η2\Phi _\pm =\bigl [\lambda \pm \sqrt {\lambda ^2-2\eta ^2Q_\infty }\bigr ]/\eta ^2, and the trajectory from Φ(0)=0<Φ\Phi (0)=0<\Phi _- is trapped below Φ\Phi _-: global existence. If λ2<2η2Q\lambda ^2<2\eta ^2Q_\infty, choose T0T_0 with Q(τ)Q~>λ2/(2η2)Q(\tau )\ge \widetilde Q>\lambda ^2/(2\eta ^2) for τT0\tau \ge T_0. The autonomous minorant with source Q~\widetilde Q has no fixed points and a vector field bounded below by a positive constant plus the quadratic, so it blows up in finite time, and comparison forces Φ\Phi to do the same. Finally, on the subcritical side the blow-up time is bounded below by that of the autonomous majorant with source QQ_\infty, whose vector field has no real roots, so

τ  0dϕη22ϕ2λϕ+Q=π+2arctan(λ/2η2Qλ2)2η2Qλ2  as λησ0κ/2,\tau ^*\ \ge \ \int _0^\infty \frac {d\phi }{\frac {\eta ^2}2\phi ^2-\lambda \phi +Q_\infty } =\frac {\pi +2\arctan \bigl (\lambda \big /\sqrt {2\eta ^2Q_\infty -\lambda ^2}\,\bigr )} {\sqrt {2\eta ^2Q_\infty -\lambda ^2}} \ \longrightarrow \ \infty \qquad \text {as }\lambda \uparrow \eta \sigma _0\sqrt {\kappa /2},
which is the stated divergence of τ\tau ^*.

Remark 6.6 (The fixed-span completion; surrogate accuracy) . Theorem 5.2 identifies qq^\infty only on (0,θ)(0,\theta ^*). The quasi-exponential continuation of the fixed-span completion differs beyond the span: on (θ,2θ)(\theta ^*,2\theta ^*),

qspan(τ)=σ022e2τ/κσ02e2θ/κq^\infty _{\mathrm {span}}(\tau )=\frac {\sigma _0^2}2e^{-2\tau /\kappa } -\sigma _0^2e^{-2\theta ^*/\kappa }
— negative on this second span. This follows by inserting τ=θ+u\tau =\theta ^*+u, 0<u<θ0<u<\theta ^*, into the periodic Fourier sums in the proof of Theorem 5.2: the first-harmonic sum changes sign, whereas the even-harmonic sum is unchanged. Thus its left and right limits at θ\theta ^* are respectively σ022e2θ/κ\frac {\sigma _0^2}{2}e^{-2\theta ^*/\kappa } and σ022e2θ/κ-\frac {\sigma _0^2}{2}e^{-2\theta ^*/\kappa }: the full two-sided jump has size σ02e2θ/κ\sigma _0^2e^{-2\theta ^*/\kappa }, although every finite sum takes the midpoint value qN(θ)=0q^N(\theta ^*)=0.

For completeness, the fixed-span continuation is well-defined on the whole half-line. In the Fourier representation used in Theorem 5.2, the partial sine sums with coefficients ωn/(κ2+ωn2)\omega _n/(\kappa ^{-2}+\omega _n^2) are uniformly bounded, while the remaining coefficient sequences are absolutely summable. Consequently, for a constant CC independent of NN,

|qN(τ)|C(eτ/κ+e2τ/κ),τ0.|q^N(\tau )|\le C\bigl (e^{-\tau /\kappa }+e^{-2\tau /\kappa }\bigr ), \qquad \tau \ge 0.
The Fourier series converges pointwise away from the lattice θN\theta ^*\mathbb N (and to its midpoint values on that null set); call the a.e. limit qspanq^\infty _{\mathrm {span}}. Dominated convergence on [0,)[0,\infty ) then gives
Qspan(τ):=0τqspan(s)ds,Qspan(τ)limN0qN(s)ds.Q^{\mathrm {span}}(\tau ):=\int _0^\tau q^\infty _{\mathrm {span}}(s)\,ds,\qquad Q^{\mathrm {span}}(\tau )\longrightarrow \lim _{N\to \infty }\int _0^\infty q^N(s)\,ds.
Termwise evaluation of the absolutely convergent terminal series yields the true terminal convexity mass
Qspan:=limNQN()=σ02κ4[cothyycsch2y],y=θκ,Q^{\mathrm {span}}_\infty :=\lim _{N\to \infty }Q^N(\infty )=\frac {\sigma _0^2\kappa }4 \Bigl [\coth y-y\,\operatorname {csch}^2y\Bigr ],\qquad y=\frac {\theta ^*}\kappa ,
strictly below the surrogate’s Q=σ02κ/4Q_\infty =\sigma _0^2\kappa /4. The preceding domination proves both Qspan(τ)QspanQ^{\mathrm {span}}(\tau )\to Q^{\mathrm {span}}_\infty and supτ0|Qspan(τ)|<\sup _{\tau \ge 0}|Q^{\mathrm {span}}(\tau )|<\infty. This terminal mass does not give an if-and-only-if existence criterion because QspanQ^{\mathrm {span}} need not be monotone and can overshoot its limit. Writing Qspan:=supτ0Qspan(τ)<\overline Q^{\mathrm {span}}:=\sup _{\tau \ge 0}Q^{\mathrm {span}}(\tau )<\infty, comparison for Φ=Ψ\Phi =-\Psi gives the rigorous bracket
λ22η2Qspanglobal existence,global existenceλ22η2Qspan.\lambda ^2\ge 2\eta ^2\overline Q^{\mathrm {span}} \quad \Longrightarrow \quad \text {global existence}, \qquad \text {global existence}\quad \Longrightarrow \quad \lambda ^2\ge 2\eta ^2Q^{\mathrm {span}}_\infty .
The first implication uses the autonomous majorant with source Qspan\overline Q^{\mathrm {span}}; the second follows because if the terminal discriminant is negative, the source is eventually bounded below by a supercritical constant. Finally,
QspanQ=1+(24y)e2y+O(ye4y),\frac {Q^{\mathrm {span}}_\infty }{Q_\infty } =1+(2-4y)e^{-2y}+O(ye^{-4y}),
so the relative correction is O(ye2y)O(ye^{-2y}), about 10510^{-5} at the reference y=7.5y=7.5.

Remark 6.7 (DIR companion) . Conditionally Gaussian rates are unbounded below, so bond prices are exponential moments of integrated intensity; Theorem 6.5 says the total convexity mass σ02κ/4\sigma _0^2\kappa /4 must be an admissible such moment. This is the not-innocent-limit phenomenon of §5.3 resurfacing in the vol-of-vol direction: the affine extension prices maturity-white risk globally only while mean reversion dominates ησ0κ/2\eta \sigma _0\sqrt {\kappa /2}. The “not innocent” caution of [13] acquires a second exact instance.

6.4Where complex spectrum may not live

The deformation sector carries rotation freely. The intensity sector cannot, and the reason is positivity rather than anything spectral.

Proposition 6.8 (Precession constraints in the intensity sector) . Suppose more generally that mm intensity factors vR+mv\in \R ^m_+ drive the deformation covariance, with affine dynamics dv=(a+Kv)dt+diag(ηivi)dZdv=(a+\mathcal Kv)\,dt+\operatorname {diag}(\eta _i\sqrt {v_i})\,dZ. Invariance of the cone R+m\R ^m_+ (admissibility, [1418]) requires the drift to point inward on each face: a0a\ge 0 and K\mathcal K Metzler (nonnegative off-diagonal). For m2m\le 2 the spectrum of a Metzler matrix is real. For m3m\ge 3 complex pairs occur (cyclic feedback) but are confined to a Perron sector: rotation is bounded by decay relative to the Perron root (Dmitriev–Dynkin–Karpelevich-type sector theorems; [5]). In particular the model’s scalar spread (m=1m=1) cannot precess, and no two-factor intensity can. Higher-dimensional positive cones may carry complex pairs, but only under the Perron-sector restrictions just described; in particular they do not admit an unconstrained isolated two-dimensional rotation block.

Proof.Admissibility. At a face point v0v\ge 0 with vi=0v_i=0, the ii-th diffusion entry ηivi\eta _i\sqrt {v_i} vanishes, so invariance of the cone requires the drift to satisfy ai+jiKijvj0a_i+\sum _{j\ne i}\mathcal K_{ij}v_j\ge 0 there; v=0v=0 gives ai0a_i\ge 0, and v=Tejv=Te_j with TT\to \infty gives Kij0\mathcal K_{ij}\ge 0 for jij\ne i. (With the Feller strengthening on each face these conditions are also sufficient; [1814].)

m2m\le 2. m=1m=1 is trivial. For m=2m=2 the characteristic polynomial of K\mathcal K has discriminant (K11K22)2+4K12K210(\mathcal K_{11}-\mathcal K_{22})^2+4\mathcal K_{12}\mathcal K_{21}\ge 0 because the off-diagonal entries are nonnegative: the spectrum is real. (Equivalently, read on a rotation cell: the boundary drift v˙2|v2=0=ωv1\dot v_2|_{v_2=0}=-\omega v_1 must be nonnegative, forcing ω=0\omega =0.)

Isolated blocks. Every principal submatrix of a Metzler matrix is Metzler; a decoupled 2×22\times 2 intensity block would be 2×22\times 2 Metzler, hence has real spectrum. No admissible intensity sector, in any dimension, contains an isolated rotation cell.

Perron sector for m3m\ge 3. Set c0:=maxi(Kii)+c_0:=\max _i(-\mathcal K_{ii})^+, so P:=K+c010P:=\mathcal K+c_0\one \ge 0 entrywise. By Perron–Frobenius [5], ρ(P)specP\rho (P)\in \operatorname {spec}P, so the spectral abscissa α:=maxRespecK\alpha :=\max \operatorname {Re}\operatorname {spec}\mathcal K is attained by a real eigenvalue and ρ(P)=α+c0\rho (P)=\alpha +c_0. Any eigenvalue μ=ξ+iζ\mu =\xi +i\zeta of K\mathcal K has |μ+c0|ρ(P)|\mu +c_0|\le \rho (P), i.e.

ζ2(αξ)(α+ξ+2c0):\zeta ^2\le (\alpha -\xi )\,(\alpha +\xi +2c_0):
rotation is bounded by the decay gap to the Perron root, at the scale set by the diagonal. Complex pairs do occur — the cyclic 3×33\times 3 permutation matrix has spectrum {1,e±2πi/3}\{1,e^{\pm 2\pi i/3}\} and saturates the bound — but an unconstrained rotation pair, ξ=α\xi =\alpha with ζ0\zeta \neq 0, is excluded, since there ζ20\zeta ^2\le 0. Sharper sector theorems (Dmitriev–Dynkin–Karpelevich) are in [5]. In the conditionally Gaussian construction the rotation cells sit in the X\X-fibre, unconstrained by positivity; only the intensity carries the cone restriction, and for the model that intensity is scalar.

Remark 6.9 (Gauge freedom; what remains open) . ψ(0)=0\psi (0)=0 is a normalization, not a necessity: changing it changes the short rate’s direct intensity loading and hence the Riccati source. Likewise, adding a vector gNvtg_Nv_t to the X\X-drift redistributes terms between the scalar and factor sectors. Any assertion uniform in NN must impose a structured-gauge condition such as supN|BN(0)gN|<\sup _N|\B _N(0)^\top g_N|<\infty; a uniform 2\ell ^2 bound on gNg_N alone does not imply this, because BN(0)\B _N(0) has NN nonzero cosine coordinates. The completion freedom of Remark 5.3(iii) therefore persists. The gauge condition stated here is what is needed for conclusions that are uniform over finite truncations.

That closes the affine convention. The completion’s closure exists with a stochastic source (Proposition 6.2). The short-end coefficient is conserved and unrenormalised at every vol-of-vol (Theorem 6.4). Its price is an existence boundary, exact for the infinite-span surrogate and bracketed for the fixed span (Theorem 6.5, Remark 6.6). And rotation stays confined to the deformation sector (Proposition 6.8).

The affine convention is, however, a surrogate: it carries the spread through its square. The model’s own algebra multiplies the deformation by sts_t itself, so stB(τ)Xts_t\B (\tau )^\top \X _t is bilinear when (st,Xt)(s_t,\X _t) is jointly Gaussian, and the literal reading lies in the quadratic–Gaussian class [234]. Within polynomial term-structure families, degree two is the last nontrivial case under the hypotheses of the maximal-degree theorem [20], so the bilinear family is the natural terminal member of that class. The construction below fixes a recovery normalization and studies the finite-dimensional HJM closure it induces; what no-arbitrage asks of the spread itself becomes visible only here.

6.5The bilinear channel: quadratic–Gaussian family and normalization

Here is the family, together with the normalization under which its closure is studied.

Assumption 6.10 (Quadratic–Gaussian family and recovery normalization) . State Zt=(st,Xt)R1+2NZ_t=(s_t,\X _t)\in \R ^{1+2N} with

dZt=(AZt+a)dt+ΛdWt,A=(β00K),a=(βs¯0),dZ_t=(\mathcal AZ_t+a)\,dt+\Lambda \,d\W _t,\qquad \mathcal A=\begin {pmatrix}-\beta& 0\\0&K\end {pmatrix},\qquad a=\begin {pmatrix}\beta \bar s\\ \mathbf 0\end {pmatrix},
β,s¯>0\beta ,\bar s>0, V:=ΛΛV:=\Lambda \Lambda ^\top with spread variance η2\eta ^2, the sine-only deformation loading CC of Definition 5.1, and spread–deformation correlation ρ\rho (set to 00 in the displayed specialization). Curve family
ft(τ)=φt(τ)+b(τ)Zt+ZtG(τ)Zt,b=(YbX),G=(g12γ12γH),f_t(\tau )=\varphi _t(\tau )+\mathbf b(\tau )^\top Z_t+Z_t^\top \mathbf G(\tau )Z_t,\qquad \mathbf b=\begin {pmatrix}Y\\ \mathbf b_X\end {pmatrix},\qquad \mathbf G=\begin {pmatrix}g&\tfrac 12\boldsymbol \gamma ^\top \\ \tfrac 12\boldsymbol \gamma&H \end {pmatrix},
where G(τ)S1+2N\mathbf G(\tau )\in \mathbb S^{1+2N} and H(τ)S2NH(\tau )\in \mathbb S^{2N} are symmetric. The symmetry is part of the parametrisation, not a restriction on the model: adding a skew Ha(τ)H_a(\tau ) leaves the curve ftf_t unchanged while altering the coefficient system, so only the symmetric part is identified. The family is indexed by η\eta with β\beta, s¯\bar s, KK and the deformation loading CC held fixed, which is what allows a normalization imposed at η=0\eta =0 to constrain the family. The recovery normalization is a model choice: for every η\eta in the family set γη(0)=B(0)\boldsymbol \gamma _\eta (0)=\B (0), together with gη(0)=0g_\eta (0)=0, Hη(0)=0H_\eta (0)=\mathbf 0, and bX,η(0)=0\mathbf b_{X,\eta }(0)=\mathbf 0; at η=0\eta =0 require in addition that the bilinear loading reproduce the completed deformation loading, γ0(τ)B(τ)\boldsymbol \gamma _0(\tau )\equiv \B (\tau ). The normalization is not a consequence of no-arbitrage. Without it, the η=0\eta =0 bilinear equation admits, for every KK, the loading γ(τ)=e(Kβ1)τB(0)\boldsymbol \gamma (\tau )=e^{(K^\top -\beta \one )\tau }\B (0), and nothing locks.

On every maturity interval considered below, b\mathbf b and G\mathbf G are C1C^1 in maturity, φ\varphi is jointly C1C^1 on the corresponding maturity–time triangles, and the integrability hypotheses of Lemma 2.1 hold. The matching equations below are identities between coefficients, maturity by maturity.

Proposition 6.11 (QG–HJM matching) . Require (3) for every initial state in a nonempty open subset of R1+2N\R ^{1+2N}, equivalently as a polynomial identity in the current state. The model of Assumption 6.10 is then consistent if and only if, with GI(τ):=0τG\mathbf G_I(\tau ):=\int _0^\tau \mathbf G and bI:=0τb\mathbf b_I:=\int _0^\tau \mathbf b,

G=AG+GA2(GVGI+GIVG),b=Ab+2Ga2(GIVb+GVbI),\mathbf G'=\mathcal A^\top \mathbf G+\mathbf G\mathcal A -2\bigl (\mathbf GV\mathbf G_I+\mathbf G_IV\mathbf G\bigr ),\qquad \mathbf b'=\mathcal A^\top \mathbf b+2\mathbf Ga -2\bigl (\mathbf G_IV\mathbf b+\mathbf GV\mathbf b_I\bigr ),
and φ˙t=φt+bVbIabtr(GV)\dot \varphi _t=\varphi _t'+\mathbf b^\top V\mathbf b_I-a^\top \mathbf b -\operatorname {tr}(\mathbf GV).

Proof.For fixed τ\tau, Itô’s formula gives the family’s drift, by polynomial degree in zz, as

φ˙t+ba+tr(GV)+(Ab+2Ga)z+z(AG+GA)z,\dot \varphi _t+\mathbf b^\top a+\operatorname {tr}(\mathbf GV) +\bigl (\mathcal A^\top \mathbf b+2\mathbf Ga\bigr )^\top z +z^\top \bigl (\mathcal A^\top \mathbf G+\mathbf G\mathcal A\bigr )z,
and its Brownian loading is (b+2Gz)Λ(\mathbf b+2\mathbf Gz)^\top \Lambda. The HJM covariance term is
(b+2Gz)V(bI+2GIz).(\mathbf b+2\mathbf Gz)^\top V(\mathbf b_I+2\mathbf G_Iz).
Its constant, linear, and symmetric quadratic coefficients are respectively
bVbI,2(GIVb+GVbI),2(GVGI+GIVG).\mathbf b^\top V\mathbf b_I,\qquad 2\bigl (\mathbf G_IV\mathbf b+\mathbf GV\mathbf b_I\bigr ),\qquad 2\bigl (\mathbf GV\mathbf G_I+\mathbf G_IV\mathbf G\bigr ).
Equating these coefficients with those of τft\partial _\tau f_t proves the displayed system and the scalar transport equation. Conversely, substitution makes the polynomial drift identity hold, proving sufficiency.

That is the matching system; the next subsection reads off what the recovery normalization locks in it.

6.6What the normalization forces

Matching is now a matter of reading the block system, and three things fall out of it: the generator is locked, the spread must be slowly varying, and the family is not closed under no-arbitrage.

Theorem 6.12 (Structure forced by the recovery normalization) . Impose the recovery normalization. Then:

  1. (Conditional gauge locking.) Given the recovery normalization, the bilinear block forces K=M+β1K=M^\top +\beta \one, uniquely; no-arbitrage alone does not lock (Assumption 6.10). Only the products are observable: the homogeneous bilinear stXts_t\X _t block has drift coefficient MM^\top. When s¯0\bar s\ne 0, the full product drift also contains the affine source βs¯Xt\beta \bar s\,\X _t; correspondingly the augmented observable system retains the spectrum of KK. The split of homogeneous decay between ss and X\X is invisible in the product: (s,X)(cs,X/c)(s,\X )\mapsto (c\,s,\X /c) fixes stXts_t\X _t for every c0c\neq 0, and it extends to a gauge of the whole curve family only when the linear and quadratic loadings and the parameters are transformed to match. Spectral locking (Corollary 4.5) holds on the homogeneous bilinear block.
  2. (The spread must be slowly varying.) specK=β1κ±iωn\operatorname {spec}K =\beta -\frac 1\kappa \pm i\omega _n: the state is stationary iff β<1/κ\beta <1/\kappa — the spread must mean-revert more slowly than the deformation decays.
  3. (Generated blocks.) The bilinear family is not closed: the drift condition generates exactly three completion blocks — an s2s^2-loading gg sourced by the convexity, a matrix XX\X \X ^\top-loading HH sourced by the spread’s vol-of-vol, and a linear X\X-loading bX\mathbf b_X sourced by the mean spread. At ρ=0\rho =0 the closed system is

    (29)g=2βgγCγI4η2ggI,γ=Mγ2η2(gγI+gIγ)2(HCγI+HICγ),H=KH+HK2(HCHI+HICH)η22(γγI+γIγ),Y=βY+2βs¯g2η2(YgI+YIg)(γICbX+γCbX,I),bX=KbX+βs¯γη2(YγI+YIγ)2(HCbX,I+HICbX),\begin{equation}\label {eq:qgsys} \begin {aligned} g'&=-2\beta g-\boldsymbol \gamma ^\top C\boldsymbol \gamma _I-4\eta ^2gg_I,\\ \boldsymbol \gamma '&=M\boldsymbol \gamma -2\eta ^2(g\boldsymbol \gamma _I+g_I\boldsymbol \gamma ) -2(HC\boldsymbol \gamma _I+H_IC\boldsymbol \gamma ),\\ H'&=K^\top H+HK-2(HCH_I+H_ICH) -\tfrac {\eta ^2}2\bigl (\boldsymbol \gamma \boldsymbol \gamma _I^\top +\boldsymbol \gamma _I\boldsymbol \gamma ^\top \bigr ),\\ Y'&=-\beta Y+2\beta \bar s\,g-2\eta ^2(Yg_I+Y_Ig) -\bigl (\boldsymbol \gamma _I^\top C\,\mathbf b_X+\boldsymbol \gamma ^\top C\,\mathbf b_{X,I}\bigr ),\\ \mathbf b_X'&=K^\top \mathbf b_X+\beta \bar s\,\boldsymbol \gamma -\eta ^2(Y\boldsymbol \gamma _I+Y_I\boldsymbol \gamma ) -2(HC\,\mathbf b_{X,I}+H_IC\,\mathbf b_X), \end {aligned} \end{equation}
    Here subscript II denotes 0τ\int _0^\tau. At η=0\eta =0, H0H\equiv 0 and γ=B\boldsymbol \gamma =\B exactly, while
    g(τ)=0τe2β(τu)qN(u)du.g(\tau )=-\int _0^\tau e^{-2\beta (\tau -u)}q^N(u)\,du.
    This is quasi-exponential, with {2β}\{-2\beta \} adjoined to the beat lattice of Remark 6.3.

Proof.(a) The sXs\X-block of the G\mathbf G-equation with the recovery normalization γ=B\boldsymbol \gamma =\B at η=0\eta =0 reads B=(Kβ1)B\B '=(K^\top -\beta \one )\B, i.e. (Kβ1M)B(τ)=0(K^\top -\beta \one -M)\B (\tau )=0 for all τ\tau: the constant matrix annihilates span{B(τ):τ0}\operatorname {span}\{\B (\tau ):\tau \ge 0\}, which is all of R2N\R ^{2N} by controllability (Lemma 2.4), so K=M+β1K=M^\top +\beta \one, uniquely. The homogeneous bilinear coefficient in d(sX)d(s\X ) is β1+K=M-\beta \one +K=M^\top; when s¯0\bar s\ne 0 the same Itô calculation also gives the affine term βs¯Xdt\beta \bar s\,\X \,dt. (b) Immediate from (a). (c) Substitute the block forms of G\mathbf G, A\mathcal A, aa, VV into the matrix system of Proposition 6.11 and read off the (s,s)(s,s)-, (s,X)(s,\X )- and (X,X)(\X ,\X )-components: this yields (29), and the three sources are the ssss-, XX\X \X-, and ss-linear components of 2(GVGI+GIVG)-2(\mathbf GV\mathbf G_I+\mathbf G_IV\mathbf G) and 2Ga2\mathbf Ga. At η=0\eta =0 the HH-source vanishes and H(0)=0H(0)=0 gives H0H\equiv 0, whence γ=B\boldsymbol \gamma =\B exactly and the gg-line integrates in closed form.

Remark 6.13 (Endpoint scope) . The model of [13] imposes Y(0)=0Y(0)=0, Y(θ)=1Y(\theta ^*)=1, and Dirichlet conditions on the deformation. Those conditions are not imposed by the recovery system. In particular, γ(0)=B(0)\boldsymbol \gamma (0)=\B (0) contains cosine coordinates, whereas the model’s deformation vanishes at the short endpoint. This is therefore a completion of the selected bilinear algebra under a recovery normalization, not a literal recovery of the model’s endpoint conditions.

Remark 6.14 (Linear–quadratic relation) . By Itô, d(s2)=[η2+2βs¯s2βs2]dt+2ηsdZd(s^2)=[\eta ^2+2\beta \bar s\,s-2\beta s^2]\,dt+2\eta s\,dZ; setting dZ~:=sgn(st)dZd\widetilde Z:=\operatorname {sgn}(s_t)\,dZ, a Brownian motion by Lévy’s characterisation, turns the diffusion into 2ηvdZ~2\eta \sqrt {v}\,d\widetilde Z. In the central case s¯=0\bar s=0 — outside Assumption 6.10’s s¯>0\bar s>0, and taken here only as the comparison point — the squared spread is then CIR with (λ,v¯,ηv)=(2β, η22β, 2η)(\lambda ,\bar v,\eta _v)=\bigl (2\beta ,\ \tfrac {\eta ^2}{2\beta },\ 2\eta \bigr ), at the Feller-violating corner, as it must be (an OU process crosses zero). The loading comparison below is unaffected by v¯\bar v, which enters only the deterministic transport. Under this map the gg-line of (29) with γ\boldsymbol \gamma frozen to B\B is identical to the ψ\psi-equation (27). So §6.1 is the central, level-blind case (cf. the linear-quadratic equivalence of [10]). The additional QG content is exactly two channels absent from §6.1: the γ\boldsymbol \gamma-flow, i.e. curve volatility from XdsX\,ds — the deformation level times the spread’s vol-of-vol — and the matrix sector HH.

Proposition 6.15 (Finite-truncation short-end identities) . For every finite NN and every parameter set on the local existence interval, gN(0)=(gN)(0)=0g^N(0)=(g^N)'(0)=0. In the exactly solvable case η=0\eta =0 one has H0H\equiv 0, γ=B\boldsymbol \gamma =\B, and, on the first span after passing to the interior completion limit,

g(τ)=σ02κ2e2τ/κe2βτ2βκ2,g^\infty (\tau )=-\frac {\sigma _0^2\kappa }2\, \frac {e^{-2\tau /\kappa }-e^{-2\beta \tau }}{2\beta \kappa -2},
with the resonant value g(τ)=σ022τe2τ/κg^\infty (\tau )=-\frac {\sigma _0^2}2\tau e^{-2\tau /\kappa } at β=1/κ\beta =1/\kappa. Consequently (g)(0+)=σ02/2(g^\infty )'(0^+)=-\sigma _0^2/2, and on fixed first-layer windows
(gN)(uθNπ)σ02G(u).(g^N)'\!\left (\frac {u\theta ^*}{N\pi }\right ) \longrightarrow -\sigma _0^2G(u).

Proof.At τ=0\tau =0 all integrated loadings in the gg-equation vanish, giving the finite-NN identities. When η=0\eta =0, the system reduces to g+2βg+qN=0g'+2\beta g+q^N=0 with g(0)=0g(0)=0. The displayed formula follows from Theorem 6.4(d) under (λ,ηv)=(2β,0)(\lambda ,\eta _v)=(2\beta ,0); the first-layer limit follows exactly as in Theorem 6.4(c).

Both identities hold at every finite NN. Whether the loading that carries them exists at every maturity is the remaining question.

6.7Finite-truncation existence

What remains is whether the bilinear loading exists at every maturity. At fixed NN that question has an exact answer, through the linearisation of the loading Riccati.

Proposition 6.16 (Finite-dimensional QG existence domain) . For every fixed finite NN, the integrated loading solves the autonomous matrix Riccati equation

GI=G(0)+AGI+GIA2GIVGI,GI(0)=0.\mathbf G_I'=\mathbf G(0)+\mathcal A^\top \mathbf G_I+ \mathbf G_I\mathcal A-2\mathbf G_IV\mathbf G_I, \qquad \mathbf G_I(0)=0.
If
(UW)=(A2VG(0)A)(UW),U(0)=1,W(0)=0,\begin {pmatrix}U\\W\end {pmatrix}' =\begin {pmatrix}-\mathcal A&2V\\ \mathbf G(0)&\mathcal A^\top \end {pmatrix} \begin {pmatrix}U\\W\end {pmatrix}, \qquad U(0)=\one ,\quad W(0)=0,
then GI=WU1\mathbf G_I=WU^{-1} until the first positive zero of detU\det U. Thus the finite-NN flow is global if and only if detU(τ)0\det U(\tau )\ne 0 for every τ>0\tau >0. On this maximal interval, G=GI\mathbf G=\mathbf G_I' is finite. For each prescribed value of the otherwise unconstrained scalar coefficient Y(0)Y(0) (with bX(0)=0\mathbf b_X(0)=\mathbf 0 as in Assumption 6.10) and each admissible initial deterministic curve φ0\varphi _0, the remaining loading equations for b\mathbf b and φ\varphi have unique solutions. Thus the same determinant gives the maximal maturity interval of the full finite-dimensional HJM coefficient system, subject to those initial data.

Proof.Integrating the first equation of Proposition 6.11 and using GI(0)=0\mathbf G_I(0)=0 gives the displayed autonomous Riccati equation. Wherever UU is invertible, differentiation of WU1WU^{-1} and substitution of the two linear equations give

(WU1)=G(0)+A(WU1)+(WU1)A2(WU1)V(WU1).(WU^{-1})'=\mathbf G(0)+\mathcal A^\top (WU^{-1}) +(WU^{-1})\mathcal A-2(WU^{-1})V(WU^{-1}).
Uniqueness for the Riccati initial-value problem therefore yields GI=WU1\mathbf G_I=WU^{-1}. Conversely, if GI\mathbf G_I exists on [0,T][0,T], define UU there by the linear equation U=(A+2VGI)UU'=(-\mathcal A+2V\mathbf G_I)U, U(0)=1U(0)=\one, and put W:=GIUW:=\mathbf G_IU; the pair solves the displayed Hamiltonian system, and Liouville’s formula
detU(τ)=exp0τtr(A+2VGI(u))du\det U(\tau )=\exp \int _0^\tau \operatorname {tr}\bigl (-\mathcal A+2V\mathbf G_I(u)\bigr )\,du
shows detU\det U never vanishes on [0,T][0,T]. Hence the maximal interval ends precisely when the graph chart loses invertibility, i.e. at the first positive zero of detU\det U.

Once GI\mathbf G_I is finite, the Riccati equation makes G=GI\mathbf G=\mathbf G_I' continuous. Adjoining bI=b\mathbf b_I'=\mathbf b rewrites the second matching equation as the inhomogeneous linear system

ddτ(bIb)=(012GVA2GIV)(bIb)+(02Ga).\frac {d}{d\tau }\binom {\mathbf b_I}{\mathbf b} = \begin {pmatrix} 0&\one \\ -2\mathbf GV&\mathcal A^\top -2\mathbf G_IV \end {pmatrix} \binom {\mathbf b_I}{\mathbf b} +\binom {0}{2\mathbf Ga}.
Its coefficients are continuous on every compact subinterval of the Riccati existence interval, so, for bI(0)=0\mathbf b_I(0)=0 and the prescribed b(0)\mathbf b(0), the loadings bI\mathbf b_I and b\mathbf b extend uniquely throughout that interval. With
r(τ):=bVbIabtr(GV),r(\tau ):=\mathbf b^\top V\mathbf b_I-a^\top \mathbf b -\operatorname {tr}(\mathbf GV),
the scalar equation is φ˙t=φt+r\dot \varphi _t=\varphi _t'+r. For prescribed φ0\varphi _0 its characteristic solution is
φt(τ)=φ0(τ+t)+0tr(τ+ts)ds,\varphi _t(\tau )=\varphi _0(\tau +t)+\int _0^t r(\tau +t-s)\,ds,
wherever τ+t\tau +t remains in the same interval. Hence no other coefficient can shorten the maximal maturity interval on the corresponding maturity–time triangle.

A zero of detU\det U is the maturity at which the exponential–quadratic loading system ceases to exist, and with it the family’s bond of that maturity: an existence boundary of the model, not an arbitrage strategy or an empirical estimate. For the ρ=0\rho =0 minimal recovery-gauge system, [42] proves that on each compact [β,β+](0,κ1)[\beta _-,\beta _+]\subset (0,\kappa ^{-1}) there is an explicit η0>0\eta _0>0, independent of NN, for which every finite truncation is global whenever 0ηη00\le \eta \le \eta _0.

The bilinear calculation is the finite-dimensional HJM closure of the selected spread–deformation algebra under the recovery normalization: it identifies the observable product drift and the polynomial blocks no-arbitrage forces, and Remark 6.13 records what the normalization leaves aside. Proposition 6.16 decides existence exactly at every fixed truncation; certifying the absence of conjugate points on the whole half-line at positive vol-of-vol is the global problem taken up in [42].

Within that scope the affine calculation answers the objection with which the section opened. In the uncorrelated affine convention, the maturity-white/X\X-sector short-end coefficient σ02/2-\sigma _0^2/2 is conserved at every vol-of-vol. Stochastic intensity nevertheless changes the remaining loading and can impose the existence boundary of Theorem 6.5. In the bilinear completion convention, no-arbitrage locks the homogeneous product generator, requires the stated stationarity inequality, and generates the additional completion blocks; the same coefficient is proved only on the exactly solvable η=0\eta =0 slice. Thus the invariant is the short-end coefficient of the X\X-sector source, not the full stochastic-intensity drift: the intensity scales that coefficient and adds its own terms away from the short end, but does not renormalise it. What the construction establishes, and where it stops, is collected in the conclusion.

7Conclusion

The introduction separated two questions: whether a finite truncation of the cylindrical deformation, at fixed spread intensity, is consistent with pricing, and what that truncation preserves and what depends on its maturity resolution. It posed them for a source specification whose link to the pricing measure had been left open. This section answers them in the order the mathematics settles them, gives the financial reading of the answers, and states what remains open.

7.1What has been shown

One observation carries the paper. The deformation’s sine modes are the imaginary parts of complex exponentials, so the smallest shift-invariant family containing them is not their span but the doubled sine–cosine envelope (Proposition 4.1), and the coordinates the envelope adjoins carry no noise. Read on the envelope, the model’s open link to Q\Q becomes a decidable question with a located answer. Whether its factor drift is arbitrage-free is the polynomial divisibility mMpzm_M\mid p-z (Theorem 4.3), with the convexity HJM adds carried by the deterministic sector as in Proposition 2.7. Here the model’s symbol p(z)=z+κz2/2p(z)=z+\kappa z^2/2 fixes only z=0z=0, and its failure sits in the silent coordinates, beyond the reach of any change of measure.

Everything the paper says about pricing consistency follows from that location. Deterministic roll-down — the rotation ωn\omega _n acting on the cosine partners — lies outside the volatility span, so no finite sine truncation admits an equivalent local martingale measure with the model’s own volatility. The discrepancy is realised by an explicit arbitrage in N+1N+1 bonds on an open dense set of maturity panels (Theorem 4.6), and its stationary size grows like N\sqrt N rather than fading under refinement (Proposition 4.8). In the infinite model the shift that would remove it has infinite Cameron–Martin energy (Proposition 4.10). Giving the silent coordinates noise of their own (§4.7) changes the finite verdict from an impossibility to a price: each truncation then admits an equivalent measure, at a Sharpe cost growing like N3/2N^{3/2}. The infinite verdict stands, since the infinite laws are singular (Proposition 4.11). That all of this is proved on finite-dimensional invariant subspaces is not a convenience: under cylindrical noise forward rates are not semimartingales (Proposition 3.3), so those subspaces are where this paper makes the question rigorous.

The same coordinates are where the repair goes. Adjoin the roll-down states, keep the sine-driven noise, correct only the drift, and every truncation becomes an ordinary 2N2N-factor Gaussian HJM model (§5). What the repair adds is the roll-down the model’s span could not carry and the convexity HJM then requires. The convexity is where the cost lies, and the cost is exact: its refinement limit is q(τ)=σ022e2τ/κq^\infty (\tau )=\frac {\sigma _0^2}2e^{-2\tau /\kappa }, a short-end jump of σ02/2\sigma _0^2/2 reached through a boundary layer of width θ/N\theta ^*/N with the universal profile GG (Theorem 5.2). Restoring the stochastic spread leaves this coefficient in place in the uncorrelated affine convention: σ02/2-\sigma _0^2/2 is conserved at every vol-of-vol, while the rest of the loading changes and an existence boundary appears, exact for the infinite-span surrogate (Theorems 6.4 and 6.5). The short-end cost is therefore a property of the maturity-local noise, not of the frozen intensity. In the bilinear completion convention, no-arbitrage locks the homogeneous product generator and recovers the coefficient on the exactly solvable η=0\eta =0 slice (Theorem 6.12, Proposition 6.15).

Refinement answers the finite-implementation question first at the level of the coefficients entering bond returns. The convexity density converges locally uniformly on compact subsets of (0,θ)(0,\theta ^*), and, after natural zero-padding, the bond-return volatility vectors converge in 2\ell ^2; every finite truncation prices its own bonds consistently. The short-end nonuniformity is resolved on the scale θ/N\theta ^*/N by the profile of Theorem 5.2, while Remark 6.6 records the separate far-end discontinuity. These are coefficient limits; the infinite traded-bond market itself is the first open problem of §7.3.

At the level of the forward curve the completions do not converge. Within the affine realisation class of Assumption 2.6, spectral locking replaces the model’s λnn2\lambda _n\asymp n^2 by the uniform decay 1/κ1/\kappa (Corollary 4.5). That n2n^2 decay came from the maturity diffusion κ2θ2\frac \kappa 2\partial _\theta ^2 and made the cylindrical field function-valued (Propositions 3.2 and 5.4). The pricing counterpart established here is therefore a family of finite-factor bond models indexed by resolution, with exact limits for specified bond-level coefficients but no curve-valued refinement limit. Resolution is therefore where the economics enters, as §5.2 says: factor count is a modelling choice with an exact convexity attached, not a numerical grid parameter. Within this refinement and its minimal completion, a curve-valued limit can be obtained only by giving up maturity-local noise or no-arbitrage at every resolution; §5.2 shows what the first of these buys. The long end stands apart from all of this: the Dybvig–Ingersoll–Ross constraint is neither caused nor cured by complexification (Proposition 5.5). What the limit means for short-maturity volatility, and the witness for pricing, is the subject of the next subsection.

7.2Economic interpretation

The completion prices its own finite-dimensional volatility specification; it does not assign a preference-free premium to the maturity-white component of the historical model of [13]. Once the sine-only volatility and the minimal sine–cosine envelope have been fixed, however, the HJM drift is no longer optional. Its first-span interior limit satisfies

q(τ)=12ddτΣ(τ)2=σ022e2τ/κ,q^\infty (\tau )=\frac 12\frac {d}{d\tau }\|\Sigma (\tau )\|^2 =\frac {\sigma _0^2}{2}e^{-2\tau /\kappa },

and hence Σ(τ)2σ02τ\|\Sigma (\tau )\|^2\sim \sigma _0^2\tau as τ0\tau \downarrow 0. This is the model-internal economic meaning of the kink: short-maturity bond volatility scales as σ0τ\sigma _0\sqrt \tau rather than linearly in τ\tau, as it would for a smooth finite-factor volatility loading. The order of limits is limτ0limN\lim _{\tau \downarrow 0}\lim _{N\to \infty } and the two do not commute: at fixed NN, Ins(τ)=2/θωnτ2/2+O(τ3)I^s_n(\tau )=\sqrt {2/\theta ^*}\,\omega _n\tau ^2/2+O(\tau ^3), so Σ(τ)=O(τ2)\|\Sigma (\tau )\|=O(\tau ^2). The τ\sqrt \tau law is a property of the refinement limit, not of any single truncation.

The boundary layer also records nonuniformity of implementation. At every finite NN the drift density vanishes at the endpoint, while at each fixed interior maturity it approaches the nonzero limit above. The theorem therefore quantifies the local convexity cost of this chosen completion and the maturity scale on which successive truncations disagree.

The finite-bond witness gives the pricing-consistency problem a separate, security-level meaning. The original NN-sine truncation does not merely fail a factor-coordinate identity: for generic maturities, N+1N+1 risky bonds contain a locally riskless self-financing direction whose discounted drift has a known sign after observing the current state. Likewise, dN2\mathfrak d_N^2 is a normalized factor-quotient diagnostic: its linear growth shows that the unreachable drift does not become negligible per retained mode, and Remark 4.9 says what it does and does not measure. Under the isotropic loading of §4.7, by contrast, the invariant is a market-price-of-risk energy. There EN\sqrt {\mathcal E_N} is the stationary root-mean-square of the maximal instantaneous Sharpe ratio of the NNth truncated market, and its limit E\sqrt {\mathcal E} is finite exactly when the block defect energy n|δn|2/kn\sum _n|\delta _n|^2/k_n is (Proposition 4.11).

7.3Limitations and open problems

The claims above stop at the following boundaries, each stated so that what would remove it is visible; see also Remarks 2.10, 4.4, 4.9, 5.3(iii), 6.9 and 6.13.

  1. Boundary conditions and domain. The comparison extends the eigenmodes from [0,θ][0,\theta ^*] to R+\R _+ by their quasi-exponential expressions; the Dirichlet conditions are respected only in the sense of Proposition 4.1, which shows precisely that they are incompatible with shift-invariance. The completion abandons them (its cosine coordinates are nonzero at τ=0\tau =0).
  2. Finite dimensionality is a real loss. That finitely many factors need not span the risks driving fixed-income markets is itself an established empirical theme [12]. The central argument of [13] — that hedging practice reflects maturity-specific risk which kk-factor models misrepresent — is not answered by the completion. Whether the exchange of maturity-specific risk for a finite arbitrage-free completion is acceptable depends on whether one is pricing or forecasting, which is the dichotomy drawn in [13].
  3. The bond witness is structural. Theorem 4.6 assumes frictionless continuous trading, strictly positive bond prices, and a generic finite panel, and it rebalances predictable cofactor exposures over a short interval. Transaction costs, position constraints, discrete observations, and market microstructure are not modeled.

Two questions stand open at these boundaries, and each is now posed exactly. The first is whether traded-bond processes are semimartingales under the fully infinite cylindrical dynamics. The repairing shift has infinite Cameron–Martin energy (Proposition 4.10), so the finite-dimensional repair does not extend to the infinite model as a change of measure. A bond-level or distribution-valued limit model — traded-bond semimartingales, a martingale measure, cross-maturity consistency — is where the infinite case would be decided. At the level of the factor laws the answer is known once the silent coordinates carry noise, the infinite laws being mutually singular (Proposition 4.11); it is the bond level that stays open, under both loadings. The second is whether the bilinear channel carries the short-end coefficient at positive vol-of-vol: a global conjugate-point problem, of which the uniform small-vol-of-vol region of [42] is the first piece.

What is settled is where the model’s finite sine truncations stand relative to the arbitrage-free class. They lie outside it at every resolution, by a margin that grows with resolution. The minimal repair is the doubled completion, whose cost is exact; and that cost is the HJM drift maturity-local volatility requires under Q\Q, its short-end value independent of the frozen intensity used to measure it.

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How to cite

Zeyu Cao and Shaosai Huang (2026). Cylindrical Yield-Curve Dynamics and the Arbitrage-Free Class. Working paper, version of September 2026. Kspectra Research. SSRN 7444240 (doi:10.2139/ssrn.7444240). https://kspectra.ai/papers/cylindrical-yield-curve-dynamics/

@misc{cao2026cylindrical,
  author = {Cao, Zeyu and Huang, Shaosai},
  title  = {{Cylindrical Yield-Curve Dynamics and the Arbitrage-Free Class}},
  year   = {2026},
  month  = sep,
  note   = {Working paper, version of September 2026},
  doi    = {10.2139/ssrn.7444240},
  url    = {https://kspectra.ai/papers/cylindrical-yield-curve-dynamics/}
}

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