Abstract
We analyze the error estimates of a fully discrete scheme for solving a semilinear stochastic subdiffusion problem driven by integrated fractional Gaussian noise with a Hurst parameter . The covariance operator Q of the stochastic fractional Wiener process satisfies for some , where denotes the Hilbert–Schmidt norm. The Caputo fractional derivative and Riemann–Liouville fractional integral are approximated using Lubich’s convolution quadrature formulas, while the noise is discretized via the Euler method. For the spatial derivative, we use the spectral Galerkin method. The approximate solution of the fully discrete scheme is represented as a convolution between a piecewise constant function and the inverse Laplace transform of a resolvent-related function. By using this convolution-based representation and applying the Burkholder–Davis–Gundy inequality for fractional Gaussian noise, we derive the optimal convergence rates for the proposed fully discrete scheme. Numerical experiments confirm that the computed results are consistent with the theoretical findings.
Keywords:
stochastic semilinear subdiffusion; fractional Gaussian noise; Caputo fractional derivative; spectral Galerkin method MSC:
65M12; 65M06; 65M70; 35S10
1. Introduction
Consider the following semilinear stochastic subdiffusion problem driven by integrated fractional Gaussian noise, with ,
where with is a linear elliptic operator and is some regular domain with smooth boundary. Here, F is a smooth real-valued function specified in Section 2 and a zero-mean, -valued Gaussian noise defined in a complete filtered probability space . Here and denote the Caputo fractional derivative and Riemann–Liouville integral, respectively [1,2,3].
Let be the eigenvalues and eigenfunctions of the elliptic operator A. We assume that takes the following Fourier series form
where is one dimensional fractional Brownian motion with Hurst parameter [2]. Let be the covariance operator of the Gaussian process such that where Q is a self-adjoint, non-negative, linear bounded operator on .
We assume that A satisfies the following resolvent estimate, with , see Lubich et al. [4], Thomée [5],
which implies that, with , see Yan et al. [6],
Many application problems can be effectively described using (1) including thermal diffusion in media with fractional geometry [7], in highly heterogeneous aquifers [8], underground environmental challenges [9], and the study of random walks [10], among others. To provide further clarity, we can consider between phenomena with short-term memory characterized by H in the range and those with long-term memory characterized by H in the range . From the viewpoint of mathematics, the Hurst index reflects the Hölder property of fractional Brownian motion’s trajectory.
Let us consider the following physical problem which can be modeled by (1), [11,12]. Let the functions , , and represent the body temperature, energy, and flux density, respectively. Then, for constants and a with , we have
The above equations lead to the classical heat equation:
However, in reality, the propagation speed is generally finite due to interruptions in heat flow caused by the material’s response. If the material has thermal memory, we often use the following model to characterize it:
with the constant and kernel . To account for external random effects, we express the energy term as
where , , and is a centered Gaussian noise that is white in time and fractional in space. Differentiating (4), we obtain
which provides a physical explanation for the fractional derivative and fractional integral with respect to t in (1).
The investigation into the existence, uniqueness, and regularity of time-fractional Stochastic Partial Differential Equations (SPDEs) has been a subject of extensive research. Chen et al. [11] successfully demonstrated both the existence and uniqueness of a stochastic time-fractional PDE in both its divergence and non-divergence forms. Anh et al. [13] explored the weak-sense solution of a time-fractional SPDE that exhibits fractional spatial and temporal characteristics. Mijena and Nane [14] investigated the existence and uniqueness of a continuous random field solution to a space-time-fractional SPDE. In a subsequent study [15], they analyzed the weak intermittency in the solution and the propagation of intermittency fronts. Liu et al. [16] studied the existence and uniqueness of solutions to time-fractional SPDEs with a more general quasi-linear elliptic operator. Chen [17] conducted a comprehensive analysis of moments, Hölder continuity, and intermittency in the solution for one-dimensional nonlinear stochastic time-fractional diffusion, see also [18,19]. Shukla et al. [20] considered the approximate controllability of Hilfer fractional stochastic evolution inclusions of order .
Recent advances have also been made in the field of numerical analysis for time-fractional SPDEs. Jin et al. [21] proposed numerical methods for stochastic linear time-fractional partial differential equations driven by integrated noise. Gunzburger, Li, and Wang [1,22] studied time discretization and finite element methods for approximating stochastic linear integrated-differential equations driven by space-time white noises. Wu et al. [23] considered the L1 scheme for approximating the linear stochastic subdiffusion problems driven by integrated space-time white noises. Cao et al. [24] considered the spatial semidiscretization of solving stochastic linear evolution equations driven by fractional noise, with the Hurst index . Deng et al. [25] investigated the existence, uniqueness, and spatial semidiscrete schemes for semilinear stochastic wave equations driven by fractional noise, with the Hurst index . For numerical methods related to stochastic parabolic partial differential equations, refer to Wang et al. [26], Dai et al. [27], Liu [28], Yan [29], Kruse [30], Jentzen and Kloeden [31], Chen et al. [32], and the references therein. For recent numerical methods in deterministic time-fractional differential equations, see [33,34] and the references therein.
Nie and Deng [2] recently proposed a unified framework for the numerical analysis of stochastic semilinear fractional diffusion equations with and ,
where they introduced a novel Burkholder–Davis–Gundy inequality for fractional Gaussian noise. They used the spectral Galerkin method and the convolution quadrature formula to discretize the Laplacian and Riemann–Liouville fractional derivatives, respectively, and provided error estimates for the proposed numerical methods.
In this paper, we adopt a similar approach to that in [2] to conduct a numerical analysis of (1). However, Equation (1) includes a more general nonlinear term compared to that used in [2]. We approximate the Caputo time-fractional derivative and the Riemann–Liouville fractional integral using the first-order Lubich convolution quadrature formula, while discretizing the fractional noise via the Euler method. For spatial discretization, we use the spectral Galerkin method. Our fully discrete scheme is formulated by expressing the approximate solution as a convolution between a piecewise constant function and the inverse Laplace transform of a function associated with the resolvent. We obtain both the temporal and spatial regularity of the solutions. Optimal error estimates in the , norm are obtained via the Laplace transform method, showing precisely how the parameters , , and influence the convergence orders. Numerical results are also provided to confirm that the computed outcomes are consistent with the theoretical findings.
The paper is organized as follows. In Section 2, we present some preliminaries and assumptions. In Section 3, we consider the spatial and temporal regularities of the solution in (1). In Section 4, we apply the spectral Galerkin method for spatial discretization. The time discretization of (1) is studied in Section 5. Finally, in Section 6, we provide some numerical simulations to validate the theoretically predicted convergence order discussed in Section 5. Throughout this paper, we use to denote positive constants independent of the functions and parameters concerned, but not necessarily the same at different occurrences.
2. Preliminaries and Main Assumptions
Let be the Sobolev space defined by
with norm .
Let be the Hilbert–Schmidt operators space from to equipped with the following inner product and norm
We will provide some main assumptions on nonlinear term , fractional noise term , which will be used throughout this paper.
Assumption 1.
For the nonlinear term F, we assume that there exist , such that
Assumption 2.
The space-time fractional Gaussian noise takes the following Fourier series form
where is one dimensional fractional Brownian motion with Hurst parameter .
Moreover, we assume
Lemma 1
([24,35]). For and , we have
where denotes the one-dimensional fractional Brownian motion with the Hurst parameter H.
Lemma 2
([36,37]). For and , there holds
where denotes the one-dimensional fractional Brownian motion with the Hurst parameter H.
Lemma 3
([2]). For with , , there exist positive such that
Here denote the fractional Sobolev space with .
Lemma 4
([2]). For and with , we have
Lemma 5.
For and , we have
Proof.
We only prove (12) here. The proof of (13) is similar.
Case 1. When , the It isometry may show
Case 2. When , let be the zero extension of on such that . By Lemma 1, the definition of the semi-norm in , and the fact coincides with , it holds
Further by Lemma 3, we get
Case 3. When , by Lemmas 2 and 4, we have
□
Lemma 6.
Let , then we have
Further we have, for ,
Proof.
See the Appendix A. □
3. Temporal and Spatial Regularities in the Solution of (1)
Denote and , then (1) can be written as
Taking the Laplace transform of (18), we have
which implies that
By the inverse Laplace transform, we have
where
and, with being the Laplace transform of ,
Here
According to the resolvent estimate (3) and interpolation theory, we have, for ,
Combining (20) and (21), we can easily get, with and ,
Remark 1.
The solution operators also satisfy the following properties:
and, with ,
Here with denote the Mittag–Leffler functions.
The existence and uniqueness of the mild solution of (1) in with can be considered by using the Banach contraction mapping theorem similar to [38]. To save space, we omit the proof here. Now we turn to the spatial and temporal regularities in the solution of (1).
Theorem 1.
Let be the solution of (1). Suppose that Assumptions 1 and 2 hold. Let and . Then we have, with ,
where .
Proof.
Simple calculations give
As for I, the estimate (22) with , Assumption condition (6) lead to
where we require .
When , by (22) with , the Assumption (7), and Remark 1, we have
where is determined by the temporal regularity in Theorem 2.
As for II, by (21), we have, noting that , that is which implies when ,
where we need to preserve the boundedness of , which leads to and .
For , we have
which implies that, by Grönwall lemma,
Theorem 2.
Let be the mild solution of (1). Suppose that Assumptions 1 and 2 are fulfilled. Let , , , . Then we have, with ,
where .
Proof.
Remark 2.
When , we get which is consistent with the well known results for the stochastic heat equation with trace class noise.
4. Spatial Discretization
In this section, we shall use the spectral Galerkin method to discretize the spatial variable of Equation (1). Let span be a finite dimensional subspace, and define the projection operator by
Define by which generates a family of resolvent operators in . Obviously, we have
and
The spectral Galerkin semeidiscrete scheme of (1) can be written as: find such that
Taking Laplace transform and inverse Laplace transform gives
where , These operators have the similar smoothing properties as . Similar to the proofs of Theorems 1 and 2, one can get the same spatial and temporal regularities of .
Now we turn to the error estimates of the spatial discretization.
Theorem 3.
Proof.
By (19) and (32), we have
The regularity of (22) with , and the Assumption (7) on F give
By the regularity of (22) with , the Assumption condition (6) on F, and (30), we have
Applying the inequality (17) and (30), and the resolvent estimate (21), with , we obtain
From (34)–(36), we derive, noting [22],
which complete the proof of Theorem 3. □
5. Time Discretization
Let be a partition of and the time step size. At , we consider the following approximations:
and
where are generated by , respectively, that is,
see Jin et al. [21].
For the noise term , we approximate it at using the Euler method as follows:
Let denote the fully approximate solution of , we define the following fully discretization scheme
Taking the discrete Laplace transform in both sides of (37), we have
Denote the discrete Laplace transform of , by
respectively. We then have
which implies
By using the inverse discrete Laplace transform, we get, with
where .
Denote where is a suitable approximation of , we then have
which implies
We will show that can be expressed as the convolution of the piecewise constant function , . To obtain this, we first introduce the following piecewise constant function , defined by, with ,
and
Similar to the proof of Lemma 2.1 in Wu et al. [23], we may show that in (38) can be written as
where
and
Denote
Then we have
Next, we introduce several lemmas that will be used in the error estimation of the fully discretized scheme.
Lemma 7
([1]). Let for , then we have
where means that , and are equivalent on .
Lemma 8.
Let for , we obtain
and, with ,
Proof.
Here, we only prove the latter. By using the resolvent estimate (2), the differential mean value theorem, and Lemma 7, we obtain:
which completes the proof of the required inequality. □
We now turn to show the error estimate of fully discretization approximation.
Proof.
For I, employing Assumption condition (6), the regularity of , resolvent estimate (20) and the first inequality in Lemma 8, we have
As for , we first divide it into three parts by using the following Taylor expansion
Thus we obtain
where
As for , noting that
and
we get
Applying the assumptions (8), (6) on F, and Hölder inequality , and the spatial regularity of , one can obtain
By simple calculation, we have
To estimate , we proceed similarly to the estimate of . By using the Hölder inequality, we obtain:
Case 1: For , we have
where we divide and choose due to , which implies .
Case 2: For , we arrive, similarly to Case 1,
As for , similar to the estimate of , note that we obtain
As for , applying assumption (9) and Theorem 2, we give
Now we estimate . Applying Assumption condition (7), we have
For , we can split it as
For , we have
Here we choose with such that and .
For , by Cauchy–Schwarz inequality and Lemma 8, there holds
On one hand, we have
where we require to preserve the boundedness of .
On the other hand, we have
Meanwhile, we need to preserve the boundedness of .
Finally, we turn to estimate . Denote . By the inequality (17) and variable substitution, we have
Due to Lemmas A1 and A2 in Appendix A, one can split into three parts.
Here we split into and to guarantee .
Note that , then one has for . Thus, by Lemmas A2 and A3 in Appendix A, we have the following cases:
If ,
If , then
As for , by Lemma 8, the Assumption condition 2, and , there holds
If , then
If , we have
For , we first have the following estimate, with ,
where we have used .
If , note that , by choosing , we have
If , by choosing , we have
If , by choosing , we have
Finally combining the above estimates, and employing Theorem 3 we have
where . By discrete Grönwall inequality, one has
where
The proof of Theorem 4 is complete. □
6. Numerical Experiments
In this section, we provide numerical results for the following time-fractional semilinear stochastic partial differential Equation (SPDE), where and .
Assume that the covariance operator Q of the -valued fractional Wiener process has eigenvalues given by for , where . Two cases are of particular interest in applications:
Case 1. When , is referred to as white noise since .
Case 2. When , is known as trace-class noise, as .
Under the assumption that , it follows that is approximately , where denotes the dimension of the space variable [2]. This result is derived from the following observation, noting ,
if . Based on this, we observe that in the trace-class case, when , we have . In contrast, in the white noise case, when , we have .
By Theorem 4, the convergence rate in time is given by:
where .
In the numerical simulations presented below, we experimentally determine the convergence rates for the following two cases:
Case 1. When , corresponds to white noise. In this case, we have in the one-dimensional case. Therefore, the theoretical convergence rate is .
Case 2. When , corresponds to trace-class noise. Here, we have , leading to a theoretical convergence rate of .
Let represent the time step size for the partition , where T is the final time. We demonstrate the numerical simulations using a one-dimensional example on the unit interval . In our computations, we set and the time step size . All expected values are computed using trajectories. We focus solely on examining the temporal convergence rates.
The final time is set to . The reference solution is computed using a much finer temporal mesh with . The numerical results for various combinations of the Hurst parameter H, the fractional orders and , as well as for both trace-class noise () and white noise (), are provided in Table 1, Table 2, Table 3 and Table 4. All numerical simulations were conducted using MATLAB R2018a (version 9.4).
Table 1.
The -error at with and .
Table 2.
The -error at with and .
Table 3.
The -error at with and .
Table 4.
The -error at with and .
In Table 1, Table 2, Table 3 and Table 4, the numbers in parentheses in the “rate” column indicate the theoretical rates predicted by Theorem 4. The experimentally determined convergence rates in time are in good agreement with the theoretical predictions, fully confirming the error analysis, despite the relatively small number of trajectories used to compute the expectations. The convergence improves consistently as the fractional orders and and H increase, reflecting enhanced temporal regularity of the solution. The running times are provided in the final columns in Table 1, Table 2, Table 3 and Table 4.
In Table 1, we set and . For (the white noise case), the theoretical convergence order is . For (the trace-class noise case), the theoretical convergence rate becomes . In both cases, we observe that the experimentally determined convergence orders exceed the theoretical expectations.
In Table 2, we set and . For (the white noise case), the theoretical convergence order is . For (the trace-class noise case), the theoretical convergence rate is . Again, the observed experimental orders are higher than the theoretical values.
In Table 3, we set and . For (the white noise case), the theoretical convergence order is . For (the trace-class noise case), the theoretical convergence rate is . The experimentally determined orders, once more, surpass the theoretical predictions.
In Table 4, we set and . For (the white noise case), the theoretical convergence order is . For (the trace-class noise case), the theoretical convergence rate is . As observed in the previous cases, the experimental convergence rates exceed the theoretical predictions.
7. Conclusions
In this work, we developed a fully discrete scheme to approximate the stochastic time-fractional diffusion problem driven by integrated fractional noise with a Hurst parameter . The Caputo time-fractional derivative and fractional integral were approximated using a first-order convolution quadrature formula, while the fractional noise was approximated using the Euler method. For spatial discretization, we used the spectral Galerkin method. By applying the convolution-based expression of the approximate solution, we obtained the error estimates for the proposed fully discrete scheme. In future work, we aim to extend these techniques to develop numerical approximations for nonlinear stochastic subdiffusion problems driven by multiplicative integrated fractional noise.
Author Contributions
Both authors contributed equally to this work. X.W. conducted the theoretical analysis, wrote the original draft, and carried out the numerical simulations. Y.Y. introduced and provided guidance in this research area. All authors have read and agreed to the published version of the manuscript.
Funding
This research was funded by the Shanxi Natural Science Foundation Project: “Analysis and Computation of the Fractional Phase Field Model of Lithium Batteries”, 2022, No. 202103021224317.
Data Availability Statement
Data are contained within the article.
Acknowledgments
The authors express their gratitude to the reviewers and the Associate Editor for their helpful comments.
Conflicts of Interest
The authors declare no conflicts of interest.
Appendix A
In this Appendix, we provide the proof of Lemma 6 and introduce several lemmas that are essential for proving the main theorems presented in this paper.
Proof of Lemma 6.
We will prove the first equality; the others can be demonstrated in a similar manner. Note that
Thus we have, using the orthogonality of basis functions,
Since the fractional Brownian motions and are independent and the cross terms for have mean zero and vanish, we arrive at
By Lemma 2.5, we get
which completes the proof of the first equality. □
Proof.
We only prove . Note that
Then by Cauchy integral formula, one obtain
The proof of the first equality is complete. □
Lemma A2.
Let
Denote . Then we get
Proof.
Extending the definition of to any (still denote ) by
which is possible since is defined for any .
By Laplace transform, we may have, with ,
and
Denote , we have, by definition of ,
Further, we have, with ,
Thus, by applying the above analysis, we obtain
Hence,
Note that , we obtain
□
Lemma A3.
Let , we have
Proof.
When , the desired estimate can be obtained by Lemma 7, resolvent estimate and Lemma A2. That is
As for , simple calculation gives
Since , one can choose a suitable , such that . Let be small enough to satisfy . Obviously
which shows exists, for . Thus
According to the fact , the desired result is reached. More precisely, if , we obtain
If , we obtain
The proof is complete. □
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