Distance from fractional Brownian motion with associated Hurst index to the subspaces of Gaussian martingales involving power integrands with an arbitrary positive exponent
Abstract
We find the best approximation of the fractional Brownian motion with the Hurst index by Gaussian martingales of the form , where is a Wiener process, .
doi:
10.15559/20-VMSTA156keywords:
keywords:
[MSC2010]rm \allowdisplaybreaks\endlocaldefs
Research Article
[type=corresp,id=cor1]Corresponding author.
23 6 2020
1 Introduction
The subject of the present paper is a fractional Brownian motion (fBm) with the Hurst index . Generally speaking, a fBm with the Hurst index is a Gaussian process with zero mean and the covariance function of the form
Its properties are rather different for and . In particular, implies short-term dependence. In contrast, implies long-term dependence. Moreover, technically it is easier to deal with fBms having . Due to this and many other reasons, fBm with has been much more intensively studied in the recent years. However, the financial markets in which trading takes place quite often, demonstrate the presence of a short memory, and therefore the volatility in such markets (so called rough volatility) is well modeled by fBm with , see e.g. [Volatility]. Thus interest to fBm with small Hurst indices has substantially increased recently. Furthermore, it is well known that a fractional Brownian motion is neither a Markov process nor semimartingale, and especially it is neither martingale nor a process with independent increments unless . That is why it is naturally to search the possibility of the approximation of fBm in a certain metric by simpler processes, such as Markov processes, martingales, semimartingales or a processes of bounded variation. As for the processes of bounded variation and semimartingales, corresponding results are presented in [Andr05, Andr06] and [Thao03]. In the papers [BM08, BMishura10, MishuraB08, 5stars] approximation of a fractional Brownian motion with Gaussian martingales was studied and summarized in the monograph [MonoBMRS19], but most of problems were considered only for , for the reasons stated above.
In the present paper we continue to consider the approximation of a fractional Brownian motion by Gaussian martingales but concentrate on the case .
Let be a complete probability space with a filtration satisfying the standard assumptions. We start with the Molchan representation of fBm via the Wiener process on a finite interval. Namely, it was established in [Norros] that the fBm can be represented as
(1) |
where is a Wiener process,
is the Molchan kernel,
(2) |
and , , is the Gamma function.
Let us consider a problem of the distance between a fractional Brownian motion and the space of square integrable martingales (initially not obligatory Gaussian), adapted to the same filtration. So, we are looking for a square integrable -martingale with the bracket that is absolutely continuous w.r.t. (with respect to) the Lebesgue measure such that it minimizes the value
We observe first that and generate the same filtration, so any square integrable -martingale with the bracket that is absolutely continuous w.r.t. the Lebesgue measure, admits a representation
(3) |
where is an -adapted square integrable process such that
. Hence we can write, see
[5stars],
{align*}
E(B_t^H - M_t)^2 &= E(∫_0^t (z(t,s)-a(s))
dW_s)^2 = ∫_0^t E(z(t,s)-a(s))^2 ds
= ∫_0^t (z(t,s)- E a(s))^2 ds + ∫_0^t
Var a(s) ds.
Consequently, it is enough to minimize over continuous
Gaussian martingales. Such martingales have orthogonal and therefore
independent increments. Then the fact that they have representation \eqrefitorep with a non-random follows, e.g., from
[Skorohod].
Now let be a nonrandom measurable function of the class ; that is, is such that the stochastic integral , , is well defined w.r.t. the Wiener process (this integral is usually called the Wiener integral if the integrand is a nonrandom function). So, the problem is to find
Note that the expression to be minimized does not involve neither the fractional Brownian motion nor the Wiener process, so the problem becomes purely analytic. Moreover, since the problem posed in a general form is not observable and accessible for solution, we restrict ourselves to one particular subclass of functions. We study the class
Our main result is Theorem 1, which shows where could be reached, depending on . We also provide remarks after the theorem.
2 Distance from fBm with to the subspaces of Gaussian martingales involving power integrands
Consider a class of power functions with an arbitrary positive exponent. Thus, we now introduce the class
For the sake of simplicity, let .
Theorem 1
Let be a function of the form , , . Then:
-
(i)
For all the maximum is reached at one of the following points: or , where {align*} t_1 &= ( c_H B(γ-H+32, H+12 )(γ+1)
-c_H^2(B(γ-H+32, H+12)(γ+1))^2-2H )^ 1γ-H+12. -
(ii)
For any there exists such that for the maximum {align*} &max_t∈[0, 1] E(B^H_t - ∫_0^t s^γdW_s )^2
= t_1^2H-2 t_1^γ+12+H c_H B(γ-H+ 32,H+12) γ+1γ+12+H+ 12γ+1 t_1^2γ+1 and is reached at the point . Here , , is a beta function.
Proof.
According to Lemma 2.20 [MonoBMRS19], the distance between the fractional Brownian motion and the integral w.r.t. Wiener process equals
(4) |
where is taken from \eqrefcH.
Let us calculate the partial derivative of in :
{align*}
∂h(t,γ)∂t = t^2H-1&(2H-2t^
γ-H+12c_H
⋅B(γ-H+32,H+12)(γ+1)+t^2(
γ-H+12)).
Let us verify whether there is such that , i.e.
Changing the variable , we obtain the following quadratic equation:
(5) |
The discriminant of the quadratic equation \eqrefeqquadrat equals