Abstract
In this article, we study a class of stochastic partial differential equations with fractional differential operators subject to some time-independent multiplicative Gaussian noise. We derive sharp conditions, under which a unique global \(L^p(\Omega )\)-solution exists for all \(p\ge 2\). In this case, we derive exact moment asymptotics following the same strategy as that in a recent work by Balan et al. (Inst Henri Poincaré Probab Stat. To appear, 2021). In the case when there exists only a local solution, we determine the precise deterministic time, \(T_2\), before which a unique \(L^2(\Omega )\)-solution exists, but after which the series corresponding to the \(L^2(\Omega )\) moment of the solution blows up. By properly choosing the parameters, results in this paper interpolate the known results for both stochastic heat and wave equations.
Similar content being viewed by others
Notes
G(t, x) corresponds to \(Y_{a,b,r,\nu ,d}(t,x)\) from [6].
Note that when \(d\ge 1\), \(b=1\) and \(a\in (0,2]\), part (1) of [6, Theorem 4.6] says that the fundamental solution Y, which is the fundamental solution G in this paper, is nonnegative provided \(r=0\) or \(r>1\). Indeed, because in this case Z is always nonnegative, for \(r>0\), Y as a fractional integral of Z (see (4.5), ibid.), Y, or our G, should also be nonnegative. We thank Guannan Hu who pointed out to us this observation.
Note that the Fourier transform is defined differently in [12].
Wiener chaos expansion has been widely to solve the linear stochastic partial differential equations. We direct interested readers to [3, Section 5] for a presentation of this procedure.
In Theorem 1.5 or eq. (1.20) of Bass et al. [2], the factor \((2\pi )^{-d}\) should not be present.
References
Balan, R.M., Chen, L., Chen, X.: Exact asymptotics of the stochastic wave equation with time-independent noise. Inst. Henri Poincaré Probab. Stat., to appear. Ann (2021)
Bass, R., Chen, X., Rosen, M.: Large deviations for Riesz potentials of additive processes. Ann. Inst. Henri Poincaré Probab. Stat. 45, 626–666 (2009)
Balan, R., Song, J.: Hyperbolic Anderson Model with space-time homogeneous Gaussian noise. ALEA Lain. Am. J. Probab. Math. Stat. 14, 799–849 (2017)
Chen, L.: Nonlinear stochastic time-fractional diffusion equations on \({\mathbb{R}}\): moments, Hölder regularity and intermittency. Trans. Am. Math. Soc. 369(12), 8497–8535 (2017)
Chen, L., Hu, Y., Hu, G., Huang, J.: Stochastic time-fractional diffusion equations on \({\mathbb{R}}^d\). Stochastics 89(1), 171–206 (2017)
Chen, L., Hu, Y., Nualart, D.: Nonlinear stochastic time-fractional slow and fast diffusion equations on \({\mathbb{R}}^d\). Stoch. Process. Appl. 129, 5073–5112 (2019)
Chen, X.: Quenched asymptotics for Brownian motion of renormalized Poisson potential and for the related parabolic Anderson models. Ann. Probab. 40(4), 1436–1482 (2012)
Chen, X.: Moment asymptotics for parabolic Anderson equation with fractional time-space noise: in Skorohod regime. Ann. Inst. Henri Poincaré: Prob. Stat. 53, 819–841 (2017)
Chen, X.: Parabolic Anderson model with rough or critical Gaussian noise. Ann. Inst. Henri Poincaré Probab. Stat. 55, 941–976 (2019)
Chen, X., Hu, Y., Song, J., Xing, F.: Exponential asymptotics for time-space Hamiltonians Ann. Inst. Henri Poincaré Probab. Stat. 51, 1529–1561 (2015)
Chen, X., Deya, A., Ouyang, C., Tindel, S.: Moment estimates for some renormalized parabolic Anderson models. Ann. Probab., To appear 2021 (2020)
Chen, X., Hu, Y.Z., Song, J., Song, X.: Temporal asymptotics for fractional parabolic Anderson model. Electron. J. Probab., 14, 39 pp (2018)
Chen, X., Li, W.: Large and moderate deviations for intersection local times. Probab. Theory Relat. Fields 128, 213–254 (2004)
Dalang, R., Khoshnevisan, D., Mueller, C., Nualart, D., Xiao, Y.: A minicourse on stochastic partial differential equations. Springer-Verlag, Berlin, 2009. xii+216 pp (2009)
Hairer, M., Labbé, C.: A simple construction of the continuum parabolic Anderson model on \({\mathbb{R}}^2\). Electron. Commun. Probab. 20(43), 11 (2015)
Hairer, M., Labbé, C.: Multiplicative stochastic heat equations on the whole space. J. Eur. Math. Soc. 20(4), 1005–1054 (2018)
Hu, Y.: Heat equations with fractional white noise potentials. Appl. Math. Optim. 43, 221–243 (2001)
Hu, Y.: Chaos expansion of heat equations with white noise potentials. Potential Anal. 16(1), 45–66 (2002)
Lê, K.: A remark on a result of Xia Chen. Stat. Probab. Lett. 118, 124–126 (2016)
Lieb, E., Loss, M.: Analysis. Second edition. Graduate Studies in Mathematics, 14. American Mathematical Society, Providence, RI (2001)
Mijena, J.B., Nane, E.: Space-time fractional stochastic partial differential equations. Stoch. Process. Appl. 125(9), 3301–3326 (2015)
Nualart, D., Nualart, E.: Introduction to Malliavin Calculus. Cambridge University Press, Cambridge (2018)
Acknowledgements
We would like to thank Raluca Balan for some useful comments on our paper and two anonymous referees for their careful reading of the paper with many good suggestions.
Author information
Authors and Affiliations
Corresponding author
Additional information
Publisher's Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Appendix
Appendix
Proof of Lemma 3.4
In this proof, \(\mu (\mathrm {d} x) = \varphi (x)\mathrm {d} x = C_{\alpha ,d}|x|^{-(d-\alpha )}\mathrm {d} x\). By the change of variables \(x' = \left( \nu /2\right) ^{1/a} x\) and \(y' = \left( \nu /2\right) ^{1/a} y\), we see that
By setting \(f^*(x) =\left( \nu /2\right) ^{-d/(2a)} f\left( \left( \nu /2\right) ^{-1/a} x \right) \), we see that
where the second equality is due to the fact that \(\int _{\mathbb {R}^d} f(x)^2 \mathrm {d} x = \int _{\mathbb {R}^d} f^*(x)^2 \mathrm {d} x\). Then an application of (3.16) proves (3.18).
Similarly, for (3.21), by change of variables \(\xi _{\sigma (j)}' = \left( \nu /2\right) ^{1/a} \xi _{\sigma (j)}\), we see that
where we have applied (3.15) and (3.18). This completes the proof of Lemma 3.4. \(\square \)
Proof of (4.9)
Starting from (3.5), by the change of variables \(t_i' = t_i/c\) and the scaling property in (3.7), we have that
where in the last line we applied (3.6). Now,
from which we see that
where in the last line we have applied (3.7). Now,
where the last line follows from a change of variables and recalling that \(\mu (\mathrm {d} \vec {\xi }\,)\) in (3.17). Lastly,
which proves (4.9). \(\square \)
Rights and permissions
About this article
Cite this article
Chen, L., Eisenberg, N. Interpolating the stochastic heat and wave equations with time-independent noise: solvability and exact asymptotics. Stoch PDE: Anal Comp 11, 1203–1253 (2023). https://doi.org/10.1007/s40072-022-00258-6
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s40072-022-00258-6
Keywords
- Stochastic partial differential equations
- Caputo derivatives
- Riemann-Liouville fractional integral
- Fractional Laplacian
- Malliavin calculus
- Skorohod integral
- Exact moment asymptotics
- Time-independent Gaussian noise
- White noise
- Global and local solutions