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Cylindrical stochastic integration and applications to financial term structure modeling

Johannes Assefa Department of Mathematics
TU Dresden
[email protected]
 and  Philipp Harms Division of Mathematical Sciences
Nanyang Technological University, Singapore
[email protected]
Abstract.

We develop a novel—cylindrical—solution concept for stochastic evolution equations. Our motivation is to establish a Heath–Jarrow–Morton framework capable of analysing financial term structures with discontinuities, overcoming deep stochastic-analytic limitations posed by mild or weak solution concepts. Our cylindrical approach, which we investigate in full generality, bypasses these difficulties and nicely mirrors the structure of a large financial market.

2020 Mathematics Subject Classification:
60H05 (Primary), 60H15, 91G30 (Secondary)
The authors thank Christa Cuchiero, Claudio Fontana, Johannes Müller, Thorsten Schmidt, Guillaume Szulda, and Josef Teichmann for helpful discussions. Philipp Harms gratefully acknowledges financial support by the National Research Foundation Singapore under the award NRF-NRFF13-2021-0012 and by Nanyang Technological University Singapore under the award NAP-SUG

1. Introduction

We develop a new mathematical framework, using cylindrical measure-valued processes, for stochastic modelling of financial term structures with discontinuities, as observed in energy and interest rate markets.

Cylindrical random variables came up in the 1960s and 1970s in the development of probability theory on Banach spaces and locally convex vector spaces [34]. Their raison d’être is that they are easy to construct, for instance by specifying their Fourier transform or by writing down a stochastic integral equation in weak form. However, it can be notoriously difficult to verify that a cylindrical random variable is non-cylindrical, i.e., a random variable in the usual sense. This is one of the main challenges in the construction of infinite-dimensional stochastic integrals, and the answer is negative beyond e.g. nuclear spaces [36] or UMD Banach spaces [31, 37].

We circumvent these difficulties by fully embracing the cylindrical approach. Thus, we give up on the hard problem of constructing non-cylindrical integrals and instead work with much simpler cylindrical integrals. Specifically, given any existing integral, stochastic or not, we define a new cylindrical integral by a canonical and simple construction; see Theorem 2.7. In important special cases, this yields the cylindrical Brownian or Lévy integrals of [8, 30, 32, 3]. Importantly, bounds for the non-cylindrical integral translate into bounds for the induced cylindrical integral. This allows us to develop a theory of cylindrical stochastic evolution equations with suitable a-priori estimates; see Theorem 3.4.

From a financial perspective, cylindrical processes can be seen as models of large financial markets. Indeed, a large financial market is simply a collection of tradeable assets, all of which are semimartingales, with no further structure imposed [17]. If one assumes without loss of generality that linear combinations of tradeable assets are tradeable, then a large financial market is precisely a cylindrical semimartingale, i.e., a collection of semimartingales indexed by the elements of some linear space.

We exploit this connection to define cylindrical models for financial term structures with discontinuities. The discontinuities are caused by jumps in the underlying at predictable times and are empirically well documented in real-world markets. For example, interest rates are influenced by policy updates of the central bank, stock prices are influenced by earnings announcements of the company, energy prices are influenced by maintenance works in the power grid, and all of these events tend to happen at pre-scheduled times; cf. Figs. 1 and 2. The immediate modeling implication is that the forward rates cannot be continuous functions of the time to maturity but must be measure-valued [27, 15].

More precisely, we develop a Heath–Jarrow–Morton (HJM) framework for measure-valued forward rates as in [27]. Actually, the forward rates are merely cylindrically measure-valued because measure-valued stochastic convolutions are ill-defined, as explained in Remark 4.1. Nevertheless, bond prices and a roll-over bank account are well-defined, as shown in Theorem 4.5, and the corresponding large financial market satisfies no asymptotic free lunch with vanishing risk [17] if a HJM drift condition is satisfied under an equivalent probability measure. Extensions to more general driving noise would be possible within the same framework, thanks to the general construction of the cylindrical stochastic integral. Our modeling framework is versatile and can be applied to other financial markets, as well, including energy markets. In principle, it also lends itself to numerical discretization by similar methods as for non-cylindrical models [1, 12], but we have not explored this any further.

Markovian methods constitute an interesting complementary approach for constructing measure-valued processes. They can be used to treat non-Lipschitz coefficients as for instance in super Brownian motion [25] and more general affine or polynomial measure-valued processes [14, 19, 16]. Notably, these processes are non-cylindrical and take values in the cone of non-negative measures. There are wide-ranging financial applications in stochastic portfolio theory [18], rough volatility modeling [20], and recently also term structure modeling [15]. The connection to cylindrical stochastic analysis is via martingale problems with cylindrical test functionals, as explained in Remark 4.8.

The structure of the paper is as follows. Section 2 develops the cylindrical integral in full generality. Section 3 considers the special case of stochastic integration and establishes well-posedness of cylindrical stochastic evolution equations. Section 4 develops applications to cylindrically measure-valued forward rate models. Appendix A explains relations to cylindrical vector measures, which are of independent interest but not needed elsewhere in the paper. Appendix B contains some auxiliary results on measurable versions of stochastic processes.

Refer to caption
Figure 1. EONIA rates jump at predictable times due to pre-scheduled monetary policy meetings of the ECB and due to regulatory constraints coming into effect at pre-scheduled dates. Figure taken from [27].
Refer to caption
Figure 2. Half hourly electricity prices in the UK jumped at predictable times in October 2016 due to pre-scheduled maintenance work on French nuclear power plants. Figure taken from [38].

2. Cylindrical vector integration

This section describes both abstractly and by examples how any given integral can be turned into a cylindrical integral. The construction is canonical and simple. Throughout this section, EE, FF, GG, and HH are Banach spaces, and there is a continuous bilinear function F×GHF\times G\to H, which is denoted by juxtaposition. Moreover, SS is a set, 𝒜\mathcal{A} is an algebra of subsets of SS, and Σ\Sigma is the sigma algebra generated by 𝒜\mathcal{A}. A finitely additive map μ:𝒜G\mu:\mathcal{A}\to G is called vector measure. A function f:SFf:S\to F is called elementary if it is measurable and has finite range. The set of elementary functions f:SFf:S\to F is denoted by (S,F)\mathcal{E}(S,F). Limits of pointwise converging sequences of elementary functions are called strongly measurable.

Definition 2.1 (Elementary integrals).

The elementary integral of μ\mu with respect to the bilinear form F×GHF\times G\to H is the linear operator

(1) (S,F)fSfμ:=i=1nfiμ(Ai)H,\mathcal{E}(S,F)\ni f\mapsto\int_{S}f\mu:=\sum_{i=1}^{n}f_{i}\,\mu(A_{i})\in H,

where nn\in\mathbb{N}, fiFf_{i}\in F, and Ai𝒜A_{i}\in\mathcal{A} are such that f=i=1nfi𝟙Aif=\sum_{i=1}^{n}f_{i}\mathds{1}_{A_{i}}. The operator norm of this elementary integral, with (S,F)\mathcal{E}(S,F) carrying the supremum norm, is called semivariation of μ\mu and is denoted by μF,G,H\|\mu\|_{F,G,H}. Moreover, for any f(S,F)f\in\mathcal{E}(S,F), the function

(2) fμ:𝒜AS𝟙AfμHf\mu:\mathcal{A}\ni A\mapsto\int_{S}\mathds{1}_{A}f\mu\in H

is finitely additive, and its semivariation with respect to the canonical bilinear form ×HH\mathbb{R}\times H\to H is denoted by fμ:=fμ,H,H\|f\|_{\mu}:=\|f\mu\|_{\mathbb{R},H,H}.

Remark 2.2 (Notation).

The above notation is quite concise and has been chosen carefully. For greater clarity, we add some remarks.

  1. (a)

    Integration is denoted by fμ\int f\mu instead of f𝑑μ\int fd\mu. The advantage is that this results in the common notation f𝑑X\int fdX in the special case where μ=dX\mu=dX is the differential of a semimartingale XX. This is described in Section 3.

  2. (b)

    The expression fμf\mu implicitly uses the bilinear form F×GHF\times G\to H, which by convention is denoted merely by juxtaposition. Accordingly, fμf\mu is a finitely additive function 𝒜H\mathcal{A}\to H.

  3. (c)

    The semivariation μF,G,H\|\mu\|_{F,G,H} is defined by integrating FF-valued integrands over the GG-valued integrator μ\mu and measuring the outcome in the norm of HH.

  4. (d)

    In the special case F=F=\mathbb{R} and G=HG=H, the semivariation fμ,H,H\|f\mu\|_{\mathbb{R},H,H} is defined by integrating \mathbb{R}-valued integrands over the HH-valued integrator μ\mu and measuring the outcome in the norm of HH. This integral uses the canonical bilinear form ×HH\mathbb{R}\times H\to H.

A major challenge in building a good integration theory is to extend the elementary integral to a large set of integrands. We next list a selection of well-known examples. All of these are non-cylindrical integrals, which can subsequently be cylindrified with the help of Theorem 2.7.

Example 2.3 (Integral on bounded measurable functions).

[22] Assume that FF is finite dimensional. Then, (S,F)\mathcal{E}(S,F) is dense in the set (S,F)\mathcal{L}^{\infty}(S,F) of bounded (strongly) measurable functions with the supremum norm. Indeed, bounded subsets of FF can be covered by finitely many ϵ\epsilon-balls, for any ϵ>0\epsilon>0, and projection to the nearest center of a ball defines an ϵ\epsilon-approximation in (S,F)\mathcal{L}^{\infty}(S,F). If μF,G,H<\|\mu\|_{F,G,H}<\infty, then the elementary integral extends uniquely to a continuous linear operator

(3) (S,F)fSfμH.\mathcal{L}^{\infty}(S,F)\ni f\mapsto\int_{S}f\mu\in H.

A set ASA\subset S is called a μ\mu-null set if

(4) inf{i𝟙AiμF,G,H:Ai𝒜,AiAi}=0.\inf\left\{\sum_{i\in\mathbb{N}}\|\mathds{1}_{A_{i}}\mu\|_{F,G,H}:A_{i}\in\mathcal{A},A\subseteq\bigcup_{i\in\mathbb{N}}A_{i}\right\}=0.

The space L(S,F)L^{\infty}(S,F) is defined as the quotient of (S,F)\mathcal{L}^{\infty}(S,F) modulo equality up to null sets, and the elementary integral factors through a continuous linear operator

(5) L(S,F)fSfμH.L^{\infty}(S,F)\ni f\mapsto\int_{S}f\mu\in H.

The disadvantage of this integral is that the uniform topology on the space of integrands is quite strong. A more elaborate version, which comes with a dominated convergence theorem, is presented next.

Example 2.4 (Bartle integral).

[5] Let μ:ΣG\mu:\Sigma\to G be countably additive on 𝒜=Σ\mathcal{A}=\Sigma with μF,G,H<\|\mu\|_{F,G,H}<\infty and suppose that there exists a control measure ν\nu, i.e., a countably additive function ν:Σ0\nu:\Sigma\to\mathbb{R}_{\geq 0} such that ν(A)0\nu(A)\to 0 is equivalent to 𝟙AμF,G,H0\|\mathds{1}_{A}\mu\|_{F,G,H}\to 0. Then, the elementary integral extends uniquely to a continuous linear map

(6) (S,F)fSfμH,\mathcal{L}^{\infty}(S,F)\ni f\mapsto\int_{S}f\mu\in H,

where (S,F)\mathcal{L}^{\infty}(S,F) carries the structure111Boundedly pointwise convergence is a non-topological notion of convergence; see e.g. [24]. of boundedly pointwise convergence. As before, one may pass to the quotient space L(S,F)L^{\infty}(S,F).

The take-away is that existence of a control measure already implies dominated convergence, even in the general context of vector integration. This is extremely useful in many applications, including stochastic integration, but is limited to bounded integrands. The most general class of integrands can be obtained by an isometric extension of the elementary integral, as shown in the subsequent two examples.

Example 2.5 (Lebesgue integral).

Let F=G=H=F=G=H=\mathbb{R} with bilinear form ×\mathbb{R}\times\mathbb{R}\to\mathbb{R} given by multiplication. Assume that μ:Σ0\mu:\Sigma\to\mathbb{R}_{\geq 0} is countably additive on 𝒜=Σ\mathcal{A}=\Sigma, i.e., μ\mu is a measure. Let L1(S,)L^{1}(S,\mathbb{R}) be the completion of (S,)\mathcal{E}(S,\mathbb{R}) with respect to the seminorm μ\|\cdot\|_{\mu}. Then, L1(S,)L^{1}(S,\mathbb{R}) can be identified with the Lebesgue space of integrable real-valued functions modulo equality up to null sets. Moreover, the elementary integral extends to a linear operator

(7) L1(S,)fSfμL^{1}(S,\mathbb{R})\ni f\mapsto\int_{S}f\mu\in\mathbb{R}

with operator norm less than or equal to 11.

Example 2.6 (Bochner integral).

[10] Let F=HF=H and G=G=\mathbb{R} with bilinear form F×FF\times\mathbb{R}\to F given by vector-times-scalar multiplication, let μ:Σ0\mu:\Sigma\to\mathbb{R}_{\geq 0} be non-negative and countably additive on 𝒜=Σ\mathcal{A}=\Sigma, and let L1(S,F)L^{1}(S,F) be the completion of (S,F)\mathcal{E}(S,F) with respect to the seminorm μ\|\cdot\|_{\mu}. Then, L1(S,F)L^{1}(S,F) can be identified with the Bochner space of strongly measurable functions f:SFf:S\to F such that fL1(S,)\|f\|\in L^{1}(S,\mathbb{R}), modulo equality up to null sets. Moreover, the elementary integral extends to a linear operator

(8) L1(S,H)fSfμHL^{1}(S,H)\ni f\mapsto\int_{S}f\mu\in H

with operator norm less than or equal to 11.

Some further examples of integrals are presented in Section 3. The common point is that the elementary integral has a continuous extension to some Banach space of integrands, which contains the elementary integrands as a dense subspace. We next show that any such integral can be turned into a new cylindrical integral in a canonical and general way.

Theorem 2.7 (Cylindrical integration).

Assume that the elementary integral in Definition 2.1 has a continuous extension to some normed space II of integrands:

(9) IfSfμH.I\ni f\mapsto\int_{S}f\mu\in H.

If EE is non-trivial, then the linear operator

(10) L(E,I)f(EeSf(e)μH)L(E,H)L(E,I)\ni f\mapsto\Big{(}E\ni e\mapsto\int_{S}f(e)\mu\in H\Big{)}\in L(E,H)

has the same operator norm as the original integral and is called cylindrified integral.

Proof.

As EE is non-trivial, the functor L(E,)L(E,\cdot) is norm-preserving. To spell this out in further detail, let T:IHT:I\to H be the given integral, and let

T^:L(E,I)L(E,H),f(eT(fe))\hat{T}:L(E,I)\to L(E,H),\qquad f\mapsto\left(e\mapsto T(fe)\right)

be the cylindrified integral, obtained by applying the functor L(E,)L(E,\cdot) to TT. Writing \bigcirc for the unit balls in the respective spaces, we have

T^L(L(E,I),L(E,H))\displaystyle\|\hat{T}\|_{L(L(E,I),L(E,H))} =supfL(E,I)T^fL(E,H)=supfL(E,I)supeE(T^f)eH\displaystyle=\sup_{f\in\bigcirc L(E,I)}\|\hat{T}f\|_{L(E,H)}=\sup_{f\in\bigcirc L(E,I)}\sup_{e\in\bigcirc E}\|(\hat{T}f)e\|_{H}
=supfL(E,I)supeET(fe)HsupfITfH=TL(I,H),\displaystyle=\sup_{f\in\bigcirc L(E,I)}\sup_{e\in\bigcirc E}\|T(fe)\|_{H}\leq\sup_{f\in\bigcirc I}\|Tf\|_{H}=\|T\|_{L(I,H)},

where the inequality is actually an equality because EE is non-trivial. ∎

The take-away is that any integral can be turned into a cylindrical integral, which is an element-wise application of the original integral. As an aside, the name cylindrical integral stems from stochastic integration: There, HH is a space of random variables, and elements of L(E,H)L(E,H) are called cylindrical random variables; see Section 3. Cylindrification can be expressed also in the language of vector measures, as explained in Appendix A.

3. Cylindrical stochastic analysis

This section describes some stochastic integrals together with their cylindrified counterparts and establishes well-posedness of cylindrical stochastic evolution equations under Lipschitz conditions on the coefficients. Throughout this section, (Ω,,𝔽=(t)t[0,T],)(\Omega,\mathcal{F},\mathbb{F}=(\mathcal{F}_{t})_{t\in[0,T]},\mathbb{P}) is a filtered probability space satisfying the usual conditions, ΩT=[0,T]×Ω\Omega_{T}=[0,T]\times\Omega, \mathcal{R} is the semi-ring of predictable rectangles in ΩT\Omega_{T}, i.e.,

(11) ={{0}×A:A0}{(s,t]×A:As,0stT},\mathcal{R}=\big{\{}\{0\}\times A:A\in\mathcal{F}_{0}\big{\}}\cup\big{\{}(s,t]\times A:A\in\mathcal{F}_{s},0\leq s\leq t\leq T\big{\}},

𝒜\mathcal{A} is the algebra generated by \mathcal{R}, and 𝒫\mathcal{P} is the sigma algebra generated by 𝒜\mathcal{A}. As any set in 𝒜\mathcal{A} is a finite union of sets in \mathcal{R}, the elementary functions over \mathcal{R} and 𝒜\mathcal{A} coincide and are denoted simply by (ΩT,)\mathcal{E}(\Omega_{T},\mathbb{R}). Unless specified otherwise, ΩT\Omega_{T} carries the predictable sigma algebra 𝒫\mathcal{P}. Subscripts 𝔽\mathbb{F} in names of functions spaces denote adaptedness to the filtration 𝔽\mathbb{F}, examples being C𝔽([0,T],L2(Ω,H))C_{\mathbb{F}}([0,T],L^{2}(\Omega,H)) or L𝔽2(Ω,L2([0,T],H))L^{2}_{\mathbb{F}}(\Omega,L^{2}([0,T],H)). The space of Hilbert-Schmidt operators between Hilbert spaces UU and HH is denoted by L2(U,H)L_{2}(U,H).

Example 3.1 (Semimartingale integral).

[29, 9, 23, 30] Let p[1,)p\in[1,\infty), let X:[0,T]Lp(Ω,)X:[0,T]\to L^{p}(\Omega,\mathbb{R}) be a stochastic process which is adapted and right-continuous in probability, and let dX:Lp(Ω,)dX:\mathcal{R}\to L^{p}(\Omega,\mathbb{R}) be given by

(12) dX({0}×A)\displaystyle dX(\{0\}\times A) =X0𝟙A,\displaystyle=X_{0}\mathds{1}_{A}, A0,\displaystyle A\in\mathcal{F}_{0},
(13) dX((s,t]×A)\displaystyle dX((s,t]\times A) =(XtXs)𝟙A,\displaystyle=(X_{t}-X_{s})\mathds{1}_{A}, As,0stT.\displaystyle A\in\mathcal{F}_{s},0\leq s\leq t\leq T.

Then, dXdX extends uniquely to an additive function dX:𝒜Lp(Ω,)dX:\mathcal{A}\to L^{p}(\Omega,\mathbb{R}) because any set 𝒜\mathcal{A} is a finite union of sets in \mathcal{R}. Moreover, the following are equivalent:

  1. (a)

    dXdX extends (uniquely) to a countably additive function dX:𝒫Lp(Ω,)dX:\mathcal{P}\to L^{p}(\Omega,\mathbb{R}).

  2. (b)

    The elementary integral

    (14) (ΩT,)fΩTf𝑑XLp(Ω,)\mathcal{E}(\Omega_{T},\mathbb{R})\ni f\mapsto\int_{\Omega_{T}}fdX\in L^{p}(\Omega,\mathbb{R})

    is continuous with respect to the supremum norm on (ΩT,)\mathcal{E}(\Omega_{T},\mathbb{R}) and therefore has a unique continuous extension222The set (ΩT,)\mathcal{E}(\Omega_{T},\mathbb{R}) is dense in (ΩT,)\mathcal{L}^{\infty}(\Omega_{T},\mathbb{R}), as shown in Example 2.3.

    (15) (ΩT,)fΩTf𝑑XLp(Ω,),\mathcal{L}^{\infty}(\Omega_{T},\mathbb{R})\ni f\mapsto\int_{\Omega_{T}}fdX\in L^{p}(\Omega,\mathbb{R}),

    whose operator norm dX,Lp(Ω),Lp(Ω)\|dX\|_{\mathbb{R},L^{p}(\Omega),L^{p}(\Omega)} is the semivariation of the vector measure dXdX and is called LpL^{p}-Emery metric.

  3. (c)

    Up to a modification, X=M+AX=M+A for a pp-integrable martingale MM and a process AA of pp-integrable variation.

As usual, one may pass from (ΩT,)\mathcal{L}^{\infty}(\Omega_{T},\mathbb{R}) to its quotient L(ΩT,)L^{\infty}(\Omega_{T},\mathbb{R}). Moreover, for any Banach space EE, the resulting cylindrified integral is of the form

(16) L(E,L(ΩT,))fΩTf𝑑XL(E,Lp(Ω,)).L(E,L^{\infty}(\Omega_{T},\mathbb{R}))\ni f\mapsto\int_{\Omega_{T}}fdX\in L(E,L^{p}(\Omega,\mathbb{R})).
Example 3.2 (Itô integral).

[31, 13] Let HH and UU be separable Hilbert spaces, and let WW be UU-cylindrical Brownian motion, i.e., W:L2([0,T],U)L2(Ω,)W:L^{2}([0,T],U)\to L^{2}(\Omega,\mathbb{R}) is a linear isometry with values in centered Gaussian random variables. Then, the elementary integral

(17) (ΩT,L2(U,H))fΩTf𝑑WL2(Ω,H)\mathcal{E}(\Omega_{T},L_{2}(U,H))\ni f\mapsto\int_{\Omega_{T}}fdW\in L^{2}(\Omega,H)

is well defined and extends to the Itô isometry

(18) L2(ΩT,L2(U,H))=L𝔽2(Ω,L2([0,T],L2(U,H)))fΩTf𝑑WL2(Ω,H).L^{2}(\Omega_{T},L_{2}(U,H))=L^{2}_{\mathbb{F}}(\Omega,L^{2}([0,T],L_{2}(U,H)))\ni f\mapsto\int_{\Omega_{T}}fdW\in L^{2}(\Omega,H).

The equality above is due to the fact that [0,T][0,T] carries an absolutely continuous measure [33]. More generally, if HH is merely UMD Banach and p(1,)p\in(1,\infty), the elementary integral extends to an isomorphism

(19) L𝔽p(Ω,γ(L2([0,T],U)),H)fΩTf𝑑WLp(Ω,H),L^{p}_{\mathbb{F}}(\Omega,\gamma(L^{2}([0,T],U)),H)\ni f\mapsto\int_{\Omega_{T}}fdW\in L^{p}(\Omega,H),

where γ\gamma stands for γ\gamma-radonifying linear operators. Even more generally, if HH is merely an abstract L1L^{1} space, one retains a continuous (but not necessarily isomorphic) integral of the above form. However, beyond these settings, there are Banach spaces HH such that the above extension of the elementary integral does not exist. Nevertheless, by Theorem 2.7 it always exists in a cylindrical form, namely, as a linear isomorphism

(20) L(E,L𝔽p(Ω,L2([0,T],U))fΩTfdWL(E,Lp(Ω,)).L(E,L^{p}_{\mathbb{F}}(\Omega,L^{2}([0,T],U))\ni f\mapsto\int_{\Omega_{T}}fdW\in L(E,L^{p}(\Omega,\mathbb{R})).

This generalizes the above integrals if EE is a dual or pre-dual of HH because Lp(Ω,H)L^{p}(\Omega,H) is then continuously included in L(E,Lp(Ω,))L(E,L^{p}(\Omega,\mathbb{R})).

Example 3.3 (Stochastic convolutions).

Let HH and UU be separable Hilbert spaces, let WW be UU-cylindrical Brownian motion, let EE be a Banach space, and let S:0L(E)S:\mathbb{R}_{\geq 0}\to L(E) be a strongly continuous semigroup. For any fL(E,L2(ΩT,L2(U,H)))f\in L(E,L^{2}(\Omega_{T},L_{2}(U,H))), the function

(21) E×[0,T](e,t)((s,ω)𝟙[0,t](s)f(Stse)(s,ω))L2(ΩT,L2(U,H))E\times[0,T]\ni(e,t)\mapsto\big{(}(s,\omega)\mapsto\mathds{1}_{[0,t]}(s)f(S_{t-s}e)(s,\omega)\big{)}\in L^{2}(\Omega_{T},L_{2}(U,H))

is continuous. Applying the Itô integral of Example 3.2 yields a continuous function

(22) E×[0,T](e,t)0tf(Stse)(s)𝑑WsL2(Ω,H).E\times[0,T]\ni(e,t)\mapsto\int_{0}^{t}f(S_{t-s}e)(s)dW_{s}\in L^{2}(\Omega,H).

The integral is continuous and adapted in t[0,T]t\in[0,T] and continuous and linear in eEe\in E. Thus, writing f(Stse)f(S_{t-s}e) as (Stsf)e(S_{t-s}^{*}f)e, which is a pull-back of ff along StsS_{t-s} followed by evaluation at ee, one obtains a continuous linear operator

(23) L(E,L2(ΩT,L2(U,H)))f0Ssfs𝑑WsL(E,C𝔽([0,T],L2(Ω,H))),L(E,L^{2}(\Omega_{T},L_{2}(U,H)))\ni f\mapsto\int_{0}^{\cdot}S_{\cdot-s}^{*}f_{s}dW_{s}\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))),

which shall be called cylindrical stochastic convolution. Similarly, using pathwise Bochner integrals instead of Itô integrals, one obtains a cylindrical deterministic convolution

(24) L(E,L2(ΩT,H))f0Ssfs𝑑sL(E,C𝔽([0,T],L2(Ω,H))).L(E,L^{2}(\Omega_{T},H))\ni f\mapsto\int_{0}^{\cdot}S_{\cdot-s}^{*}f_{s}ds\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))).

The cylindrical convolutions in Example 3.3 can be used to develop a theory of cylindrical stochastic evolution equations, as shown next.

Theorem 3.4 (Cylindrical stochastic evolution equations).

Let UU and HH be separable Hilbert spaces, let WW be UU-cylindrical Brownian motion, let EE be a Banach space, let S:0L(E)S:\mathbb{R}_{\geq 0}\to L(E) be a strongly continuous semigroup, let X0L(E,L2((Ω,0,),H))X_{0}\in L(E,L^{2}((\Omega,\mathcal{F}_{0},\mathbb{P}),H)), and let FF and GG be Lipschitz functions

(25) F:L(E,C𝔽([0,T],L2(Ω,H)))\displaystyle F:L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))) L(E,C𝔽([0,T],L2(Ω,H))),\displaystyle\to L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))),
(26) G:L(E,C𝔽([0,T],L2(Ω,H)))\displaystyle G:L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))) L(E,C𝔽([0,T],L2(Ω,L2(U,H)))).\displaystyle\to L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,L_{2}(U,H)))).

Then, there exists a unique XL(E,C𝔽([0,T],L2(Ω,H)))X\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))) which satisfies

(27) Xt=StX0+0tStsF(X)s𝑑s+0tStsG(X)s𝑑Ws,X_{t}=S_{t}^{*}X_{0}+\int_{0}^{t}S_{t-s}^{*}F(X)_{s}ds+\int_{0}^{t}S_{t-s}^{*}G(X)_{s}dW_{s},

for all t[0,T]t\in[0,T], where the integrals are EE-cylindrical, StsFS_{t-s}^{*}F denotes the pull-back of FF along StsS_{t-s}, and similarly for StsGS_{t-s}^{*}G.

Proof.

We first verify that the right-hand side of the integral equation is well-defined. For any XL(E,C𝔽([0,T],L2(Ω,H)))X\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))), the integrands are given by

(28) F(X)\displaystyle F(X) L(E,C𝔽([0,T],L2(Ω,H))),\displaystyle\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))), G(X)\displaystyle G(X) L(E,C𝔽([0,T],L2(Ω,L2(U,H)))).\displaystyle\in L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,L_{2}(U,H)))).

Any continuous adapted function with values in L2(Ω,H)L^{2}(\Omega,H) or L2(Ω,L2(U,H))L^{2}(\Omega,L_{2}(U,H)) has a predictable version by Lemma B.2, giving rise to continuous inclusions

(29) C𝔽([0,T],L2(Ω,H))\displaystyle C_{\mathbb{F}}([0,T],L^{2}(\Omega,H)) L2(ΩT,H),\displaystyle\to L^{2}(\Omega_{T},H),
(30) C𝔽([0,T],L2(Ω,L2(U,H)))\displaystyle C_{\mathbb{F}}([0,T],L^{2}(\Omega,L_{2}(U,H))) L2(ΩT,L2(U,H)).\displaystyle\to L^{2}(\Omega_{T},L_{2}(U,H)).

For later use, we note that the operator norm of these inclusions is T\sqrt{T}. Via these inclusions, the integrands are given by

(31) F(X)\displaystyle F(X) L(E,L2(ΩT,H)),\displaystyle\in L(E,L^{2}(\Omega_{T},H)), G(X)\displaystyle G(X) L(E,L2(ΩT,L2(U,H))).\displaystyle\in L(E,L^{2}(\Omega_{T},L_{2}(U,H))).

By an application of the cylindrical stochastic convolutions in Example 3.3, one obtains that the right-hand side of the integral equation,

(32) K(X):=SX0+0SsF(X)s𝑑s+0SsG(X)s𝑑Ws\displaystyle K(X):=S_{\cdot}^{*}X_{0}+\int_{0}^{\cdot}S_{\cdot-s}^{*}F(X)_{s}ds+\int_{0}^{\cdot}S_{\cdot-s}^{*}G(X)_{s}dW_{s}

belongs to L(E,C𝔽([0,T],L2(Ω,H)))L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H))). The function

(33) K:L(E,C𝔽([0,T],L2(Ω,H)))L(E,C𝔽([0,T],L2(Ω,H)))K:L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H)))\to L(E,C_{\mathbb{F}}([0,T],L^{2}(\Omega,H)))

is Lipschitz continuous as a composition of Lipschitz functions. The Lipschitz constant of KK is bounded by a constant times T\sqrt{T}. Thus, for sufficiently small TT, the operator KK is a contraction and has a unique fixed point by the Banach fixed point theorem. For arbitrary TT, one obtains a unique fixed point by concatenation of solutions on small sub-intervals of [0,T][0,T]. ∎

4. Cylindrically measure-valued term structure models

This section is devoted to cylindrical random measures and applications to financial term structure models. Throughout this section, T>0T^{*}\in\mathbb{R}_{>0}, (Ω,,𝔽=(t)t[0,T],)(\Omega,\mathcal{F},\mathbb{F}=(\mathcal{F}_{t})_{t\in[0,T^{*}]},\mathbb{P}) is a filtered probability space satisfying the usual conditions, ΩT=[0,T]×Ω\Omega_{T^{*}}=[0,T^{*}]\times\Omega with the predictable sigma algebra 𝒫\mathcal{P}, WW is UU-cylindrical Brownian motion on a separable Hilbert space UU, (>0)\mathcal{B}(\mathbb{R}_{>0}) is the Borel sigma algebra on the positive half-line >0=(0,)\mathbb{R}_{>0}=(0,\infty), and C0(>0)C_{0}(\mathbb{R}_{>0}) is the Banach space of continuous functions f:>0f:\mathbb{R}_{>0}\to\mathbb{R} with limx0f(x)=limxf(x)=0\lim_{x\to 0}f(x)=\lim_{x\to\infty}f(x)=0. By the Riesz–Markov–Kakutani representation theorem, C0(>0)C_{0}(\mathbb{R}_{>0})^{*} is the space (>0)\mathcal{M}(\mathbb{R}_{>0}) of signed measures μ:(>0)\mu:\mathcal{B}(\mathbb{R}_{>0})\to\mathbb{R} with finite total variation μC0(>0)=μ,,\|\mu\|_{C_{0}(\mathbb{R}_{>0})^{*}}=\|\mu\|_{\mathbb{R},\mathbb{R},\mathbb{R}}. Similarly, for any Banach space EE, (>0,E)\mathcal{M}(\mathbb{R}_{>0},E) denotes the set of countably additive vector measures μ:(>0)E\mu:\mathcal{B}(\mathbb{R}_{>0})\to E with finite semivariation μ,E,E\|\mu\|_{\mathbb{R},E,E}.

The origin of this paper lies in the difficulty of constructing measure-valued stochastic integrals, as needed for Heath–Jarrow–Morton models of discontinuous term structures. This difficulty is explained next, and a solution via cylindrical random measures is developed subsequently.

Remark 4.1 (Measure-valued stochastic integration).

The development of measure-valued stochastic integrals meets several difficulties. As the space (>0)\mathcal{M}(\mathbb{R}_{>0}) is not UMD, there is no Itô isometry in the sense of Example 3.2. However, (>0)\mathcal{M}(\mathbb{R}_{>0}) is an abstract L1L^{1} space, i.e., a Banach lattice such that x+y=x+y\|x+y\|=\|x\|+\|y\| for any non-negative elements xx and yy whose infimum xyx\wedge y vanishes. Thus, it is lattice isometric to some L1L^{1} space [2, Theorem 4.27]. Therefore, a decoupling inequality holds [11, Corollary 3.21], which implies that the elementary Itô integral extends to a continuous linear map [11, Theorem 3.29]

(34) L𝔽2(Ω,γ(L2([0,T],U),(>0))f0TfdWL2(Ω,(>0)),L^{2}_{\mathbb{F}}(\Omega,\gamma(L^{2}([0,T],U),\mathcal{M}(\mathbb{R}_{>0}))\ni f\mapsto\int_{0}^{T}fdW\in L^{2}(\Omega,\mathcal{M}(\mathbb{R}_{>0})),

where γ\gamma denotes the space of gamma-radonifying operators. This integral can be used to build measure-valued term structure models which are parameterized by time-of-maturity. However, it is ill-suited for parameterization by time-to-maturity, as in Heath–Jarrow–Morton models, because measure-valued stochastic convolutions involving the shift semigroup are ill-defined. For example, if WW is scalar Brownian motion, δ0(>0)\delta_{0}\in\mathcal{M}(\mathbb{R}_{>0}) is the Dirac measure, and SS is the semigroup of left-shifts of measures, then the integral 0tStsδ0𝑑Ws\int_{0}^{t}S_{t-s}\delta_{0}dW_{s} is almost never a measure because it is the distributional derivative of a Brownian path: indeed, for any fCc((0,t))f\in C^{\infty}_{c}((0,t)),

(35) 0tStsδ0(f)𝑑Ws=0tf(ts)𝑑Ws=0tf(ts)Ws𝑑s.\int_{0}^{t}S_{t-s}\delta_{0}(f)dW_{s}=\int_{0}^{t}f(t-s)dW_{s}=\int_{0}^{t}f^{\prime}(t-s)W_{s}ds.

Abstractly, the problem is that the shift semigroup on (>0)\mathcal{M}(\mathbb{R}_{>0}) is not strongly measurable and not Rademacher-bounded. Replacing the norm topology on (>0)\mathcal{M}(\mathbb{R}_{>0}) by the weak-* topology does not help because the stochastic integral in the above example is not a measure-valued random variable despite the integrand sStsδ0s\mapsto S_{t-s}\delta_{0} being bounded predictable. The integral is, however, a cylindrical measure-valued random variable, i.e., an element of L(C0(>0),L2(Ω))L(C_{0}(\mathbb{R}_{>0}),L^{2}(\Omega)). This is detailed in the sequel.

The following lemma (a) describes cylindrical random measures as a generalization of random measures and (b) explains their relation to Lp(Ω)L^{p}(\Omega)-valued vector measures. An important consequence of (b) is that cylindrical vector measures can be integrated not only against C0C_{0} functions, as suggested by their definition, but also against bounded Borel-measurable functions.

Lemma 4.2 (Cylindrical random measures).
  1. (a)

    For any p[1,]p\in[1,\infty], there is a continuous inclusion

    (36) Lp(Ω,(>0))μ(ffμ)L(C0(>0),Lp(Ω)).L^{p}(\Omega,\mathcal{M}(\mathbb{R}_{>0}))\ni\mu\mapsto\Big{(}f\mapsto\int f\mu\Big{)}\in L(C_{0}(\mathbb{R}_{>0}),L^{p}(\Omega)).
  2. (b)

    For any p(1,)p\in(1,\infty), there is an isometric isomorphism

    (37) (>0,Lp(Ω))μ(ffμ)L(C0(>0),Lp(Ω)).\mathcal{M}(\mathbb{R}_{>0},L^{p}(\Omega))\ni\mu\mapsto\Big{(}f\mapsto\int f\mu\Big{)}\in L(C_{0}(\mathbb{R}_{>0}),L^{p}(\Omega)).
Proof.
  1. (a)

    Let ii denote the function in (a). To show that ii is injective, let μLp(Ω,(>0))\mu\in L^{p}(\Omega,\mathcal{M}(\mathbb{R}_{>0})) with i(μ)=0i(\mu)=0. Then, the support of μ\mu is {0}\{0\} because for any non-zero ν(>0)\nu\in\mathcal{M}(\mathbb{R}_{>0}), there is fC0(>0)f\in C_{0}(\mathbb{R}_{>0}) with fν0\int f\nu\neq 0, and then Uf={ν~(>0):fν~0}U_{f}=\{\tilde{\nu}\in\mathcal{M}(\mathbb{R}_{>0}):\int f\tilde{\nu}\neq 0\} is an open neighborhood of ν\nu which satisfies [μUf]=[fμ0]=0\mathbb{P}[\mu\in U_{f}]=\mathbb{P}[\int f\mu\neq 0]=0. Therefore, μ\mu vanishes, and ii is injective. Furthermore, ii is continuous thanks to the following inequality, which holds for all μLp(Ω,(>0))\mu\in L^{p}(\Omega,\mathcal{M}(\mathbb{R}_{>0})) and fC0(>0)f\in C_{0}(\mathbb{R}_{>0}):

    (38) fμLp(Ω)fC0(>0)μ(>0)Lp(Ω)=fC0(>0)μLp(Ω,(>0)).\Big{\|}\int f\mu\Big{\|}_{L^{p}(\Omega)}\leq\big{\|}\|f\|_{C_{0}(\mathbb{R}_{>0})}\|\mu\|_{\mathcal{M}(\mathbb{R}_{>0})}\big{\|}_{L^{p}(\Omega)}=\|f\|_{C_{0}(\mathbb{R}_{>0})}\|\mu\|_{L^{p}(\Omega,\mathcal{M}(\mathbb{R}_{>0}))}.
  2. (b)

    Let ii denote the function in (b). Then, ii is well defined because the elementary integral of any μ(>0,Lp(Ω))\mu\in\mathcal{M}(\mathbb{R}_{>0},L^{p}(\Omega)) extends isometrically to a continuous linear operator (>0)Lp(Ω)\mathcal{L}^{\infty}(\mathbb{R}_{>0})\to L^{p}(\Omega), as explained in Example 2.3, and then restricts to a continuous linear operator i(μ):C0(>0)Lp(Ω)i(\mu):C_{0}(\mathbb{R}_{>0})\to L^{p}(\Omega). The semivariation of μ\mu is the operator norm of the elementary integral of μ\mu and coincides with the operator norms of the above extension and restriction. Thus, ii is an isometry. The surjectivity of ii follows from a version of the Riesz representation theorem; cf. [22, Section VI.2]. Thanks to the reflexivity of Lp(Ω)L^{p}(\Omega), the bi-dual of any TL(C0(>0),Lp(Ω))T\in L(C_{0}(\mathbb{R}_{>0}),L^{p}(\Omega)) is an extension T:C0(>0)Lp(Ω)T^{**}:C_{0}(\mathbb{R}_{>0})^{**}\to L^{p}(\Omega) of TT. Let B(>0)B(\mathbb{R}_{>0}) be the closure of (>0)\mathcal{E}(\mathbb{R}_{>0}) in the uniform norm. As B(>0)B(\mathbb{R}_{>0}) is isometrically included in C0(>0)C_{0}(\mathbb{R}_{>0})^{**} and contains all indicators of Borel sets, one can define μ:(>0)AT𝟙ALp(Ω)\mu:\mathcal{B}(\mathbb{R}_{>0})\ni A\mapsto T^{**}\mathds{1}_{A}\in L^{p}(\Omega). As TT^{**} is weak-* to weak-* continuous, μ\mu is weakly countably additive and, by the Orlicz–Pettis theorem [22, Corollary I.4.4], countably additive. Moreover, i(μ)=Ti(\mu)=T because the two operators coincide on the dense set of elementary integrands. Thus, ii is surjective.

Remark 4.3 (Countable additivity).

Let p(1,)p\in(1,\infty). Then, any cylindrical random measure μL(C0(>0),Lp(Ω))\mu\in L(C_{0}(\mathbb{R}_{>0}),L^{p}(\Omega)) is ‘almost’ countably additive in the following sense: for any sequence of disjoint sets Ai(>0)A_{i}\in\mathcal{B}(\mathbb{R}_{>0}),

(39) μ(iAi)=iμ(Ai)\mu\Big{(}\bigcup_{i}A_{i}\Big{)}=\sum_{i}\mu(A_{i})

up to a null set, which may depend on the sequence AiA_{i}. If μ\mu is non-cylindrical, i.e., μLp(Ω,(>0))\mu\in L^{p}(\Omega,\mathcal{M}(\mathbb{R}_{>0})), the null set can be chosen independently of the sequence AiA_{i}. This difference is minor in financial applications.

Cylindrically measure-valued processes can be constructed by solving cylindrical stochastic evolution equations, as shown next. The corresponding theory has been developed in Theorem 3.4. For financial applications, the two most important cases are where the semigroup acts via right-shifts on C0(>0)C_{0}(\mathbb{R}_{>0}) and where the semigroup acts trivially as the identity on C0(>0)C_{0}(\mathbb{R}_{>0}). Note that right-shifts on C0(>0)C_{0}(\mathbb{R}_{>0}) correspond to left-shifts on the dual space (>0)\mathcal{M}(\mathbb{R}_{>0}), in line with the Heath–Jarrow–Morton framework.

Corollary 4.4 (Cylindrically measure-valued evolution equations).

Let S:0L(C0(>0))S:\mathbb{R}_{\geq 0}\to L(C_{0}(\mathbb{R}_{>0})) be a strongly continuous semigroup, let X0L(C0(>0),L2(Ω,0,))X_{0}\in L(C_{0}(\mathbb{R}_{>0}),L^{2}(\Omega,\mathcal{F}_{0},\mathbb{P})), and let FF and BB be Lipschitz functions

(40) F:L(C0(>0),C𝔽([0,T],L2(Ω)))\displaystyle F:L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))) L(C0(>0),C𝔽([0,T],L2(Ω))),\displaystyle\to L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))),
(41) G:L(C0(>0),C𝔽([0,T],L2(Ω)))\displaystyle G:L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))) L(C0(>0),C𝔽([0,T],L2(Ω,U))).\displaystyle\to L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega,U))).

Then, there exists a unique XL(C0(>0),C𝔽([0,T],L2(Ω)))X\in L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))) which satisfies for all t[0,T]t\in[0,T] that

(42) Xt=StX0+0tStsF(X)s𝑑s+0tStsG(X)s𝑑Ws.X_{t}=S_{t}^{*}X_{0}+\int_{0}^{t}S_{t-s}^{*}F(X)_{s}ds+\int_{0}^{t}S_{t-s}^{*}G(X)_{s}dW_{s}.
Proof.

This is a special case of Theorem 3.4. ∎

We next describe financial term structure models where the collection of forward rates is given by a cylindrically measure-valued process, as given by Corollary 4.4 above. Then, the prices of bonds or futures are obtained as usual by integration of maturities and exponentiation, i.e., by the application of cylindrical functionals. This yields a large financial market, whose tradeable assets are cylindrical functionals of a cylindrical process. Besides the minimal assumption that linear combinations of tradeable assets are tradeable, there is little extra structure imposed. In particular, it is not assumed that the tradeable assets constitute a non-cylindrical process, and this assumption would also be lacking an economic foundation.

As a proof of concept, we present in Theorem 4.5 below a term structure model with two components: one for interest rates, parameterized by time-to-maturity, and another one for energy prices, parameterized by time-of-maturity. The motivation is that both interest rate and energy markets exhibit jumps at predictable times, which force the forward rates to be measure-valued. Moreover, the parameterization by time-to-maturity is well suited for dynamics depending foremost on market structure, as in the case of interest rates, whereas the parameterization by time-of-maturity is well suited for dynamics depending strongly on seasonalities, as in the case of energy markets. The additive structure of energy forwards corresponds to advance settlement of future contracts and is broken for continuous or terminal settlement unless the interest rate is constant [6, Section 4.1]. We do not know how to model continuously or terminally settled contracts with stochastic interest rates in the present generality; cf. [7].

Theorem 4.5 (Cylindrical term structure models).

Let S:0L(C0(>0))S:\mathbb{R}_{\geq 0}\to L(C_{0}(\mathbb{R}_{>0})) be the semigroup of right shifts, let F,F~L(C0(>0),C𝔽([0,T],L2(Ω)))F,\tilde{F}\in L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega))), let G,G~L(C0(>0),C𝔽([0,T],L2(Ω,U)))G,\tilde{G}\in L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega,U))), and let X,X~L(C0(>0),C𝔽([0,T],L2(Ω)))X,\tilde{X}\in L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega))) satisfy for all t[0,T]t\in[0,T^{*}] that

(43) Xt\displaystyle X_{t} =StX0+0tStsFs𝑑s+0tStsGs𝑑Ws,\displaystyle=S_{t}^{*}X_{0}+\int_{0}^{t}S_{t-s}^{*}F_{s}ds+\int_{0}^{t}S_{t-s}^{*}G_{s}dW_{s},
(44) X~t\displaystyle\tilde{X}_{t} =X~0+0tF~s𝑑s+0tG~s𝑑Ws.\displaystyle=\tilde{X}_{0}+\int_{0}^{t}\tilde{F}_{s}ds+\int_{0}^{t}\tilde{G}_{s}dW_{s}.

Then, the following statements hold, with operators on C0(>0)C_{0}(\mathbb{R}_{>0}) viewed as vector measures using the Riesz representation in Lemma 4.2 (b):

  1. (a)

    For every T,T1,T2[0,T]T,T_{1},T_{2}\in[0,T^{*}], the bond price and energy futures processes

    (45) P(t,T)=exp(Xt(0,Tt]),P~(t,T1,T2)=X~t(T1,T2),t[0,T],P(t,T)=\exp\big{(}-X_{t}(0,T-t]\big{)},\qquad\tilde{P}(t,T_{1},T_{2})=\tilde{X}_{t}(T_{1},T_{2}),\qquad t\in[0,T^{*}],

    have a predictable version, which is unique up to dtdt\otimes\mathbb{P}-null sets.

  2. (b)

    The roll-over bank account process

    (46) Bt=limni=1nP(t(i1)/n,ti/n)1,t[0,T],B_{t}=\lim_{n\to\infty}\prod_{i=1}^{n}P(t(i-1)/n,ti/n)^{-1},\qquad t\in[0,T^{*}],

    exists, has a predictable version, and is given by

    (47) Bt\displaystyle B_{t} =exp(X0(0,t]+0tFs(0,ts]𝑑s+0tGs(0,ts]𝑑Ws),\displaystyle=\exp\Big{(}X_{0}(0,t]+\int_{0}^{t}F_{s}(0,t-s]ds+\int_{0}^{t}G_{s}(0,t-s]dW_{s}\Big{)}, t[0,T].\displaystyle t\in[0,T^{*}].
  3. (c)

    For every T,T1,T2[0,T]T,T_{1},T_{2}\in[0,T^{*}], the discounted bond price P(t,T)/BtP(t,T)/B_{t} and the discounted energy future P~(t,T1,T2)/Bt\tilde{P}(t,T_{1},T_{2})/B_{t} are local martingales if and only if the following drift conditions hold:

    (48) Ft(0,Tt]=12Gt(0,Tt]U2,F~t(T1,T2)=0,dt-almost surely.F_{t}(0,T-t]=\frac{1}{2}\|G_{t}(0,T-t]\|_{U}^{2},\qquad\tilde{F}_{t}(T_{1},T_{2})=0,\qquad dt\otimes\mathbb{P}\text{-almost surely.}
  4. (d)

    If the drift condition (c) is valid for all T,T1,T2[0,T]T,T_{1},T_{2}\in[0,T^{*}], then there is no asymptotic free lunch with vanishing risk under any probability measure equivalent to \mathbb{P} in the large financial market whose primary traded asssets are the discounted bond prices P(t,T)/BtP(t,T)/B_{t} together with the discounted energy futures P~(t,T1,T2)/Bt\tilde{P}(t,T_{1},T_{2})/B_{t}, for T,T2,T2[0,T]T,T_{2},T_{2}\in[0,T^{*}].

Proof.
  1. (a)

    Thanks to the continuous linear inclusion [35]

    (49) C𝔽([0,T],L2(Ω))L2(ΩT),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega))\to L^{2}(\Omega_{T^{*}}),

    which amounts to the choice of a predictable version, the process XX is a continuous linear operator

    (50) X:C0(>0)L2(ΩT).X:C_{0}(\mathbb{R}_{>0})\to L^{2}(\Omega_{T^{*}}).

    Then, by the same argument as in Lemma 4.2 (b), XX has a Riesz representation as a countably additive vector measure

    (51) X:(>0)L2(ΩT).X:\mathcal{B}(\mathbb{R}_{>0})\to L^{2}(\Omega_{T^{*}}).

    Thanks to the countable additivity, the function

    (52) xX(0,x]L2(ΩT)\mathbb{R}\ni x\mapsto X(0,x]\in L^{2}(\Omega_{T^{*}})

    is right-continuous with left limits. By Lemma B.1, it has a measurable version

    (53) ×ΩT(x,t,ω)X(0,x](t,ω).\mathbb{R}\times\Omega_{T^{*}}\ni(x,t,\omega)\mapsto X(0,x](t,\omega)\in\mathbb{R}.

    As for any T[0,T]T\in[0,T^{*}], the function

    (54) ΩT(t,ω)(Tt,t,ω)×ΩT\Omega_{T^{*}}\ni(t,\omega)\mapsto(T-t,t,\omega)\in\mathbb{R}\times\Omega_{T^{*}}

    is measurable, one obtains the measurability of the function

    (55) ΩT(t,ω)X(0,Tt](t,ω).\Omega_{T^{*}}\ni(t,\omega)\mapsto X(0,T-t](t,\omega)\in\mathbb{R}.

    This function is uniquely determined up to dtdt\otimes\mathbb{P}-null sets because, for any X~\tilde{X} which originates from another choice of measurable version above,

    (56) 0T𝔼[(X(0,Tt](t,ω)X~(0,Tt](t,ω))2]𝑑t=0.\int_{0}^{T^{*}}\mathbb{E}\Big{[}\big{(}X(0,T-t](t,\omega)-\tilde{X}(0,T-t](t,\omega)\big{)}^{2}\Big{]}dt=0.

    Thus, by exponentiation, one obtains that the bond price process P(,T)P(\cdot,T) has a predictable version, which is determined uniquely up to a dtdt\otimes\mathbb{P}-null set. A similar reasoning applies to the energy futures process P~(,T1,T2)\tilde{P}(\cdot,T_{1},T_{2}).

  2. (b)

    For the purpose of the proof, let BtB_{t} be defined for any t[0,T]t\in[0,T^{*}] as

    (57) Bt=exp(X0(0,t]+0tFs(0,ts]𝑑s+0tGs(0,ts]𝑑Ws).B_{t}=\exp\Big{(}X_{0}(0,t]+\int_{0}^{t}F_{s}(0,t-s]ds+\int_{0}^{t}G_{s}(0,t-s]dW_{s}\Big{)}.

    These integrals are well-defined because for any t[0,T]t\in[0,T^{*}], the integrands have predictable versions

    (58) ΩT(s,ω)\displaystyle\Omega_{T^{*}}\ni(s,\omega) F(0,ts](s,ω),\displaystyle\mapsto F(0,t-s](s,\omega)\in\mathbb{R},
    (59) ΩT(s,ω)\displaystyle\Omega_{T^{*}}\ni(s,\omega) G(0,ts](s,ω)U,\displaystyle\mapsto G(0,t-s](s,\omega)\in U,

    which are uniquely determined up to dsds\otimes\mathbb{P}-null sets and square-integrable, as can be seen similarly to (a). To define the roll-over bank account process, let t[0,T]t\in[0,T^{*}], nn\in\mathbb{N}, ti=ti/nt_{i}=ti/n, and

    (60) Btn=i=1nP(ti1,ti)1=exp(i=1nXti1(0,titi1]).B^{n}_{t}=\prod_{i=1}^{n}P(t_{i-1},t_{i})^{-1}=\exp\Big{(}\sum_{i=1}^{n}X_{t_{i-1}}(0,t_{i}-t_{i-1}]\Big{)}.

    Then, by the evolution equation for XX,

    (61) logBtn\displaystyle\log B^{n}_{t} =i=1nSti1X0(0,titi1]+i=1n0ti1Sti1sFs(0,titi1]𝑑s\displaystyle=\sum_{i=1}^{n}S_{t_{i-1}}^{*}X_{0}(0,t_{i}-t_{i-1}]+\sum_{i=1}^{n}\int_{0}^{t_{i-1}}S_{t_{i-1}-s}^{*}F_{s}(0,t_{i}-t_{i-1}]ds
    (62) +i=1n0ti1Sti1sGs(0,titi1]𝑑Ws\displaystyle\qquad+\sum_{i=1}^{n}\int_{0}^{t_{i-1}}S_{t_{i-1}-s}^{*}G_{s}(0,t_{i}-t_{i-1}]dWs
    (63) =X0(0,tn]+i=1n0ti1Fs(ti1s,tis]𝑑s\displaystyle=X_{0}(0,t_{n}]+\sum_{i=1}^{n}\int_{0}^{t_{i-1}}F_{s}(t_{i-1}-s,t_{i}-s]ds
    (64) +i=1n0ti1Gs(ti1s,tis]𝑑Ws.\displaystyle\qquad+\sum_{i=1}^{n}\int_{0}^{t_{i-1}}G_{s}(t_{i-1}-s,t_{i}-s]dW_{s}.

    In terms of the round-up-to-the-grid operator

    (65) sn=min{ti:i,tis},s[0,t],\lceil s\rceil_{n}=\min\{t_{i}:i\in\mathbb{N},t_{i}\geq s\},\qquad s\in[0,t],

    this can be rewritten by purely algebraic manipulations as

    (66) logBtn\displaystyle\log B^{n}_{t} =X0(0,t]+0tFs(sns,ts]𝑑s+0tGs(sns,ts]𝑑Ws.\displaystyle=X_{0}(0,t]+\int_{0}^{t}F_{s}(\lceil s\rceil_{n}-s,t-s]ds+\int_{0}^{t}G_{s}(\lceil s\rceil_{n}-s,t-s]dW_{s}.

    For large nn, sns\lceil s\rceil_{n}-s tends to 0 from above. As FF and GG are countably additive vector measures on (>0)\mathcal{B}(\mathbb{R}_{>0}), it follows that

    (67) limnFs(sns,ts]Fs(0,ts]L2(Ω)\displaystyle\lim_{n\to\infty}\|F_{s}(\lceil s\rceil_{n}-s,t-s]-F_{s}(0,t-s]\|_{L^{2}(\Omega)} =0,\displaystyle=0,
    (68) limnGs(sns,ts]Gs(0,ts]L2(Ω,U)\displaystyle\lim_{n\to\infty}\|G_{s}(\lceil s\rceil_{n}-s,t-s]-G_{s}(0,t-s]\|_{L^{2}(\Omega,U)} =0.\displaystyle=0.

    Moreover, one has the uniform bounds

    (69) Fs(sns,ts]L2(Ω)\displaystyle\|F_{s}(\lceil s\rceil_{n}-s,t-s]\|_{L^{2}(\Omega)} FL(C0(>0),C𝔽([0,T],L2(Ω))),\displaystyle\leq\|F\|_{L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega)))},
    (70) Gs(sns,ts]L2(Ω,U)\displaystyle\|G_{s}(\lceil s\rceil_{n}-s,t-s]\|_{L^{2}(\Omega,U)} GL(C0(>0),C𝔽([0,T],L2(Ω,U))).\displaystyle\leq\|G\|_{L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T^{*}],L^{2}(\Omega,U)))}.

    Thus, by the dominated convergence theorem,

    (71) limn0tFs(sns,ts]Fs(0,ts]L2(Ω)2𝑑s=0,\displaystyle\lim_{n\to\infty}\int_{0}^{t}\|F_{s}(\lceil s\rceil_{n}-s,t-s]-F_{s}(0,t-s]\|_{L^{2}(\Omega)}^{2}ds=0,
    (72) limn0tGs(sns,ts]Gs(0,ts]L2(Ω,U)2𝑑s=0.\displaystyle\lim_{n\to\infty}\int_{0}^{t}\|G_{s}(\lceil s\rceil_{n}-s,t-s]-G_{s}(0,t-s]\|_{L^{2}(\Omega,U)}^{2}ds=0.

    This ensures convergence of the integrals in the above formula for logBtn\log B^{n}_{t}. Thus, we have shown that BtnB^{n}_{t} converges to BtB_{t} as nn tends to infinity.

  3. (c)

    This follows along the lines of [26, p. 61ff]. Fix 0tTT0\leq t\leq T\leq T^{*}. By the evolution equation for XX, one has

    (73) logP(t,T)\displaystyle-\log P(t,T) =Xt(0,Tt]\displaystyle=X_{t}(0,T-t]
    (74) =StX0(0,Tt]+0tStsFs(0,Tt]𝑑s+0tStsGs(0,Tt]𝑑Ws\displaystyle=S_{t}X_{0}(0,T-t]+\int_{0}^{t}S_{t-s}F_{s}(0,T-t]ds+\int_{0}^{t}S_{t-s}G_{s}(0,T-t]dW_{s}
    (75) =X0(t,T]+0tFs(ts,Ts]𝑑s+0tGs(ts,Ts]𝑑Ws.\displaystyle=X_{0}(t,T]+\int_{0}^{t}F_{s}(t-s,T-s]ds+\int_{0}^{t}G_{s}(t-s,T-s]dW_{s}.

    By the integral formula for BtB_{t}, the discounted bond price Z(t,T)=P(t,T)/BtZ(t,T)=P(t,T)/B_{t} satisfies

    (76) logZ(t,T)\displaystyle-\log Z(t,T) =X0(0,T]+0tFs(0,Ts]𝑑s+0tGs(0,Ts]𝑑Ws.\displaystyle=X_{0}(0,T]+\int_{0}^{t}F_{s}(0,T-s]ds+\int_{0}^{t}G_{s}(0,T-s]dW_{s}.

    This is a semimartingale, and Itô’s formula gives

    (77) Z(t,T)=Z(0,T)0tZ(s,T)(Fs(0,Ts]12Gs(0,Ts]U2)𝑑s0tZ(s,T)Gs(0,Ts]𝑑Ws.Z(t,T)=Z(0,T)-\int_{0}^{t}Z(s,T)\Big{(}F_{s}(0,T-s]-\frac{1}{2}\|G_{s}(0,T-s]\|_{U}^{2}\Big{)}ds\\ -\int_{0}^{t}Z(s,T)G_{s}(0,T-s]dW_{s}.

    Thus, Z(,T)Z(\cdot,T) is a local martingale if and only if the first drift condition in statement (c) is satisfied. A similar but simpler argument establishes the second drift condition.

  4. (d)

    Under the probability measure \mathbb{P}, the value process of any admissible trading strategy in finitely many discounted bonds and discounted energy futures is a supermartingale, thanks to the Ansel–Stricker lemma. Therefore, \mathbb{P} is a separating measure for the large financial market with discounted bonds and discounted energy futures as primary traded assets. Consequently, no asymptotic free lunch with vanishing risk holds under \mathbb{P}, and also under any measure equivalent to it [17].

Remark 4.6 (Bank account process).

The bank account process in Theorem 4.5 (b) coincides with the usual one for ‘regular’ Heath–Jarrow–Morton models. Here, regularity refers to requirement that the forward rate measures XtX_{t} are non-cylindrical and have continuous Lebesgue densities ftf_{t}, which are subject to some additional regularity and integrability conditions [26, Conditions H1–H3 and C1–C4]. Under these conditions, the bank account process may equivalently be defined by the well-known formula Bt=exp(0trs𝑑s)B_{t}=\exp(\int_{0}^{t}r_{s}ds), where rs=fs(0)r_{s}=f_{s}(0) is the short rate. In particular, the bank account process is a semimartingale. Moreover, by no-arbitrage considerations, the discounted bond prices, and consequently also the undiscounted ones, are semimartingales. In contrast, beyond the regular case, the bank account process and the undiscounted bond price processes may not be semimartingales. For instance, this happens if Xt=StX0X_{t}=S_{t}^{*}X_{0} is deterministic and X0X_{0} has infinite variation.

Example 4.7 (Cylindrical term structure models).

It is easy to specify coefficients F,F~F,\tilde{F} and G,G~G,\tilde{G} which satisfy the assumptions and drift conditions of Theorems 3.4 and 4.5, as demonstrated in the following simple example. Let eL(>0)ne\in L^{\infty}(\mathbb{R}_{>0})^{n}, and let g,g~:n𝒩2(U,(>0))g,\tilde{g}:\mathbb{R}^{n}\to\mathcal{N}_{2}(U,\mathcal{M}(\mathbb{R}_{>0})) be bounded Lipschitz functions, where 𝒩2\mathcal{N}_{2} denotes 2-nuclear operators. Then, for any XL(C0(>0),C𝔽([0,T],L2(Ω)))X\in L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))), one has Xt(e)L2(Ω,n)X_{t}(e)\in L^{2}(\Omega,\mathbb{R}^{n}) via the Riesz isomorphism in Lemma 4.2 (b), and g(Xt(e))L(Ω,𝒩2(U,(>0)))g(X_{t}(e))\in L^{\infty}(\Omega,\mathcal{N}_{2}(U,\mathcal{M}(\mathbb{R}_{>0}))) thanks to the boundedness of gg. Thus, one obtains Lipschitz functions

(78) G,G~:L(C0(>0),C𝔽([0,T],L2(Ω)))L(C0(>0),C𝔽([0,T],L2(Ω,U)))G,\tilde{G}:L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega)))\to L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega,U)))

by identifying UU with UU^{*} and setting

(79) G(X)(f)(t)=g(Xt(e))(f),G~(X)(f)(t)=g~(Xt(e))(f).G(X)(f)(t)=g(X_{t}(e))(f),\qquad\tilde{G}(X)(f)(t)=\tilde{g}(X_{t}(e))(f).

Moreover, one obtains Lipschitz functions

(80) F,F~:L(C0(>0),C𝔽([0,T],L2(Ω)))L(C0(>0),C𝔽([0,T],L2(Ω))),F,\tilde{F}:L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega)))\to L(C_{0}(\mathbb{R}_{>0}),C_{\mathbb{F}}([0,T],L^{2}(\Omega))),

which satisfy the drift conditions of Theorem 4.5, by the following definition, where the product of a measure μ(>0)\mu\in\mathcal{M}(\mathbb{R}_{>0}) with its distribution function μ(>0)\int\mu\in\mathcal{L}^{\infty}(\mathbb{R}_{>0}) is denoted by μμ(>0)\mu\int\mu\in\mathcal{M}(\mathbb{R}_{>0}), and where Tr\mathrm{Tr} denotes the trace on UU:

(81) F(X)(f)(t)=12Tr(g(Xt(e))g(Xt(e)))(f),F~(X)=0.F(X)(f)(t)=\frac{1}{2}\mathrm{Tr}\big{(}g(X_{t}(e)){\textstyle\int}g(X_{t}(e))\big{)}(f),\qquad\tilde{F}(X)=0.

Alternative specifications are possible. For instance, the coefficients could be time-dependent and could depend simultaneously on XX and X~\tilde{X}. Note that GG, as specified here, is non-cylindrically measure-valued. We have not been able to construct FF subject to the drift condition when GG is merely cylindrically measure-valued. Nevertheless, even for non-cylindrical GG, a cylindrical setting is needed because the solution XX will be merely cylindrical, as noted in Remark 4.1.

Remark 4.8 (Measure-valued processes via martingale problems).

A well-trodden path for constructing measure-valued processes is via martingale problems. Recently, this approach has been used to define models for discontinuous term structures [15], similarly to the ones defined here via cylindrical stochastic analysis. The two approaches are closely related, as described next. Let XX be a mild solution of the stochastic evolution equation in Corollary 4.4 with Markovian coefficients F(X)s=F(Xs)F(X)_{s}=F(X_{s}) and G(X)s=G(Xs)G(X)_{s}=G(X_{s}), i.e.,

(82) Xt=StX0+0tStsF(Xs)𝑑s+0tStsG(Xs)𝑑Ws.X_{t}=S_{t}^{*}X_{0}+\int_{0}^{t}S_{t-s}^{*}F(X_{s})ds+\int_{0}^{t}S_{t-s}^{*}G(X_{s})dW_{s}.

Then, thanks to the (square) integrability of the coefficients, XX is also a weak solution of the stochastic evolution equation [21, Theorem 6.5], i.e., letting AA denote the generator of the shift semigroup SS, one has for all eD(A)e\in D(A) that

(83) Xt(e)=X0(e)+0tXs(Ae)𝑑s+0tF(Xs)(e)𝑑s+0tG(Xs)(e)𝑑Ws.X_{t}(e)=X_{0}(e)+\int_{0}^{t}X_{s}(Ae)ds+\int_{0}^{t}F(X_{s})(e)ds+\int_{0}^{t}G(X_{s})(e)dW_{s}.

Thus, for any cylindrical functional f(x)=φ(x(e1),,x(en))f(x)=\varphi(x(e_{1}),\dots,x(e_{n})), where φCb(n,)\varphi\in C_{b}^{\infty}(\mathbb{R}^{n},\mathbb{R}), nn\in\mathbb{N}, and e1,,enD(A)e_{1},\dots,e_{n}\in D(A), the process

(84) f(Xt)f(X0)0tAf(Xs)Xs𝑑s0tf(Xs)F(Xs)𝑑s120tf′′(Xs)(G(Xs),G(Xs))𝑑sf(X_{t})-f(X_{0})-\int_{0}^{t}Af^{\prime}(X_{s})X_{s}ds-\int_{0}^{t}f^{\prime}(X_{s})F(X_{s})ds\\ -\frac{1}{2}\int_{0}^{t}f^{\prime\prime}(X_{s})(G(X_{s}),G(X_{s}))ds

is a local martingale, where AfAf^{\prime} is interpreted in the following sense:

(85) Af(x)y=g(x(e1),,x(en))(y(Ae1),,y(Aen)).Af^{\prime}(x)y=g^{\prime}(x(e_{1}),\dots,x(e_{n}))(y(Ae_{1}),\dots,y(Ae_{n})).

Assuming that FF and GG map non-cylindrical random measures to non-cylindrical random measures, as for instance in Example 4.7, it follows that XX solves the martingale problem with extended generator

(86) Lf(x)=Af(x)x+f(x)F(x)+12f′′(x)(G(x),G(x)),x(>0).\displaystyle Lf(x)=Af^{\prime}(x)x+f^{\prime}(x)F(x)+\frac{1}{2}f^{\prime\prime}(x)(G(x),G(x)),\qquad x\in\mathcal{M}(\mathbb{R}_{>0}).

Under suitable conditions, existence and uniqueness of solutions to such martingale problems can be shown directly by Markovian methods. Notably, this allows one to construct non-cylindrical processes with values in the cone of non-negative measures. Of course, coefficients which lead to genuinely cylindrical processes, as for example in Remark 4.1, are excluded. Solutions of the martingale problem are, in great generality, again weak and mild solutions as above, for some Brownian motion reconstructed from the solution on an extended probability space [21, Theorem 8.2].

Appendix A Cylindrical vector measures

This section explains cylindrification from the perspective of vector measures. Specifically, we show that (a) cylindrical integrals in the sense of Theorem 2.7 are integrals with respect to cylindrical vector measures and conversely that (b) cylindrical vector measures give rise to a cylindrical integral similar to Theorem 2.7. Moreover, (c) cylindrical vector measures can be identified with operator-valued vector measures. These relations are clearest in the case I=(S,F)I=\mathcal{L}^{\infty}(S,F), which shall be assumed here.

  1. (a)

    The space (S,L(E,F))\mathcal{L}^{\infty}(S,L(E,F)) of non-cylindrical integrands is continuously included in the space L(E,(S,F))L(E,\mathcal{L}^{\infty}(S,F)) of cylindrical integrands. Therefore, the cylindrical integral restricts to a continuous linear operator (S,L(E,F))L(E,H)\mathcal{L}^{\infty}(S,L(E,F))\to L(E,H) or, equivalently, a continuous linear operator EL((S,L(E,F)),H)E\to L(\mathcal{L}^{\infty}(S,L(E,F)),H). In other words, for any eEe\in E, the function eμ:𝒜E^Ge\otimes\mu:\mathcal{A}\to E\hat{\otimes}G belongs to the space baba of finitely additive functions 𝒜E^G\mathcal{A}\to E\hat{\otimes}G with finite semivariation L(E,F),E^G,H\|\cdot\|_{L(E,F),E\hat{\otimes}G,H}, where ^\hat{\otimes} is the projective tensor product. Consequently, μ\mu (or rather the linear map eeμe\mapsto e\otimes\mu) belongs to L(E,ba)L(E,ba). In this sense, μ\mu is a cylindrical vector measure, and the cylindrical integral is a continuous extension of its elementary integral.

  2. (b)

    Of course, not all elements of L(E,ba)L(E,ba) are of the simple form eeμe\mapsto e\otimes\mu. To treat the general case, let μL(E,ba)\mu\in L(E,ba), where baba now denotes the set of finitely additive functions 𝒜G\mathcal{A}\to G with finite semivariation F,G,H\|\cdot\|_{F,G,H}. Under the mild assumption that for all eEe\in E, the elementary integral with respect to μ(e)\mu(e) extends continuously to (S,F)\mathcal{L}^{\infty}(S,F), one obtains a continuous integral (S,F)L(E,H)\mathcal{L}^{\infty}(S,F)\to L(E,H). Thus, starting from an EE-cylindrical vector measure, one obtains an integral with values in the space L(E,H)L(E,H), similarly to Theorem 2.7.

  3. (c)

    Cylindrical vector measures μ:E(𝒜G)\mu:E\to(\mathcal{A}\to G) in the sense of (b) can be identified with operator-valued vector measures ν:𝒜(EG)\nu:\mathcal{A}\to(E\to G) by a flip of coordinates: ν(A)(e)=μ(e)(A)\nu(A)(e)=\mu(e)(A). This identification is a Banach isometry. To see this, recall that the semivariation norm of a vector measure is the operator norm of its elementary integral and use the fact that L(E,L(F,G))L(F,L(E,G))L(E,L(F,G))\cong L(F,L(E,G)) for any Banach spaces EE, FF, and GG. Similar results for countably additive vector measures have been obtained in [4, Theorem 4.2] building on [28].

Appendix B Measurable and predictable versions

Lemma B.1 (Measurable version).

Let T+T\in\mathbb{R}_{+}, let (S,Σ,μ)(S,\Sigma,\mu) be a measure space, let EE be a Banach space, and let D([0,T],L2(S,E))D([0,T],L^{2}(S,E)) be the Banach space of càdlàg functions [0,T]L2(S,E)[0,T]\to L^{2}(S,E) with the supremum norm. Then, any process XD([0,T],L2(S,E))X\in D([0,T],L^{2}(S,E)) has a strongly measurable version Y:[0,T]×SEY:[0,T]\times S\to E, which is uniquely defined up to dtμdt\otimes\mu-null sets, thereby giving rise to a linear embedding with operator norm bounded by T\sqrt{T}:

(87) D([0,T],L2(S,E))XYL2([0,T]×S,E).D([0,T],L^{2}(S,E))\ni X\mapsto Y\in L^{2}([0,T]\times S,E).
Proof.

We follow the lines of [21, Proposition 3.2] with continuity replaced by right-continuity with left limits. Let XD([0,T],L2(S,E))X\in D([0,T],L^{2}(S,E)). For any nn\in\mathbb{N}, there exists a finite set An[0,T]A_{n}\subset[0,T], which contains zero and satisfies

(88) supt[0,T]XtXtnL2(Ω,E)2n,\sup_{t\in[0,T]}\|X_{t}-X_{\lfloor t\rfloor_{n}}\|_{L^{2}(\Omega,E)}\leq 2^{-n},

where tn=max(An[0,t])\lfloor t\rfloor_{n}=\max(A_{n}\cap[0,t]) denotes rounding down to the grid AnA_{n}. For any t[0,T]t\in[0,T], let NtN_{t} be the set of all sSs\in S such that Xtn(s)X_{\lfloor t\rfloor_{n}}(s) does not converge to Xt(s)X_{t}(s). By Borell–Cantelli, NtN_{t} is a null set. The set N=t[0,T]{t}×NtN=\bigcup_{t\in[0,T]}\{t\}\times N_{t} is measurable and a dtμdt\otimes\mu-null set. Define Y:[0,T]×ΩEY:[0,T]\times\Omega\to E as limnXt(sn)\lim_{n\to\infty}X_{t}(\lfloor s\rfloor_{n}) for (t,s)N(t,s)\notin N and as zero otherwise. Then, YY is a version of XX and is strongly measurable as a pointwise limit of strongly measurable functions. The L2L^{2}-norm of YY is bounded by T\sqrt{T} times the supremum norm of XX. In particular, for any other strongly measurable version Y~\tilde{Y}, the L2L^{2} norm of YY~Y-\tilde{Y} vanishes, which implies that YY is determined uniquely up to dtdt\otimes\mathbb{P}-null sets. ∎

Lemma B.2 (Predictable version).

Let T+T\in\mathbb{R}_{+}, let (Ω,,𝔽=(t)t[0,T],)(\Omega,\mathcal{F},\mathbb{F}=(\mathcal{F}_{t})_{t\in[0,T]},\mathbb{P}) be a filtered probability space satisfying the usual conditions, let EE be a Banach space, let C𝔽([0,T],L2(Ω,E))C_{\mathbb{F}}([0,T],L^{2}(\Omega,E)) be the Banach space of adapted processes in C([0,T],L2(Ω,E))C([0,T],L^{2}(\Omega,E)), and let ΩT=[0,T]×Ω\Omega_{T}=[0,T]\times\Omega be endowed with the measure dtdt\otimes\mathbb{P} restricted to the predictable sigma algebra. Then, any process XC𝔽([0,T],L2(Ω,E))X\in C_{\mathbb{F}}([0,T],L^{2}(\Omega,E)) has a predictable version Y:ΩTEY:\Omega_{T}\to E, which is uniquely defined up to dtdt\otimes\mathbb{P}-null sets, thereby giving rise to a continuous linear embedding of operator norm bounded by T\sqrt{T}:

(89) C𝔽([0,T],L2(Ω))XYL2(ΩT).C_{\mathbb{F}}([0,T],L^{2}(\Omega))\ni X\mapsto Y\in L^{2}(\Omega_{T}).
Proof.

See [21, Proposition 3.7] or [35, Lemma 2.4] for the existence of a predictable version and [35, Lemma 2.4 and Proposition 2.5] for the continuous linear embedding. ∎

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