Abstract
In this paper, we study the stochastic Hamiltonian flow in Wasserstein manifold, the probability density space equipped with \(L^2\)-Wasserstein metric tensor, via the Wong–Zakai approximation. We begin our investigation by showing that the stochastic Euler–Lagrange equation, regardless it is deduced from either the variational principle or particle dynamics, can be interpreted as the stochastic kinetic Hamiltonian flows in Wasserstein manifold. We further propose a novel variational formulation to derive more general stochastic Wasserstein Hamiltonian flows, and demonstrate that this new formulation is applicable to various systems including the stochastic Schrödinger equation, Schrödinger equation with random dispersion, and Schrödinger bridge problem with common noise.
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Acknowledgements
The authors would like to thank the anonymous referees and the associate editor for their comments and suggestions.
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The research is partially supported by Georgia Tech Mathematics Application Portal (GT-MAP) and by research grants NSF DMS-1830225, and ONR N00014-21-1-2891, the start-up funds P0039016 and internal grants (P0041274,P0045336) from Hong Kong Polytechnic University, the CAS AMSS-PolyU Joint Laboratory of Applied Mathematics and the grant from the Research Grants Council of the Hong Kong Special Administrative Region, China (PolyU25302822 for ECS project).
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A Appendix
A Appendix
Proof of Lemma 2.2
The local existence of (2.4) and (2.1) is ensured thanks to the local Lipschitz condition of f and \(\sigma \). To obtain a global solution, a priori bound on \(H_0(x,p)\) is needed. Denote the solutions of (2.1) and (2.4) with same initial condition \((x_0,p_0)\) by \((x_t^{\delta },p_t^{\delta }), \delta >0\) and \(x_t^{0},p_t^{0}\), respectively. Applying the chain rule to \(H_0(x_t^{\delta },p_t^{\delta })\) for (2.4) and (2.1), we get that
By applying growth condition (2.3) and taking expectation on the second equation, we derive that
The first inequality leads to \(H_0(x_t^{\delta },p_t^{\delta })<\infty \) since \(\dot{\xi }_{\delta }(s)=\frac{B_{t_{k+1}}-B_{t_k}}{\delta },\) if \(s\in [t_k,t_{k+1}].\) Furthermore, taking expectation on the first inequality, applying Fernique’s theorem (see, e.g. [27]) for Gaussian variable and independent increments of \(B_t\), we get that
where [w] is the integer part of the real number w. The second inequality yield that \(H_0(x_t,p_t)<\infty , a.s,\) and the global existence of the strong solution of (2.4). Similarly, for \(p\ge 2\), we have that
Furthermore, applying the above bounded moment estimate, we obtain that for \(s\le t\),
However, the above estimate of \(x^{\delta }\) is too rough and exponentially depending on \(\frac{1}{\delta }\). As a consequence, we can not expect any convergence result. A delicate estimate of \((x^{\delta },p^{\delta })\) is needed.
Assume that \(t\in [t_k,t_{k+1}],\) \(t_k=k\delta .\) Then by using the expansion of (2.1), we have that
Making use of the growth condition (2.3), we have that
By using the Gronwall–Bellman inequality, we obtain that
For simplicity, assume that \(T=K\delta .\) Denote \([t]_{\delta }=t_k=k\delta \) if \(t\in [t_k,t_{k+1}).\) The definition of \(\xi _{\delta }(s)\) yields that \(s\in [t_j,t_{j+1}]\)
Define a stopping time \(\tau _R=\inf \{t\in [0,T]| \int _0^{[t]_{\delta }}|\dot{\xi }_{\delta }|^2 \delta ds \ge R\}.\) The stopping time is well-defined since the quadratic variation process of Brownian motion is bounded in [0, T]. Then taking \(t\le \tau _{R}\) and using Hölder’s inequality, then it holds that
Similarly, one could obtain a analogous estimate of (A.1) with the integral over \([t_{k-1},t_{k}]\), where \(t_k\), \(k\le K\), \(t_K\le \tau _R.\) By the Cauchy inequality and taking expectation on both sides of (A.1), applying the Burkholder–Davis–Gundy inequality (see e.g, [35]) and using the independent increments of Brownian motion, we get
Applying the Fernique theorem and choosing sufficient small \(\delta \) such that \(12c_1\delta <1,\) then we have that
The above estimation gives
Then the Grownall’s inequality yield that
Combining the above estimates with (A.1) and the Burkholder–Davis–Gundy inequality, we conclude that
Similarly, by choosing sufficient small \(\delta \), we have that for \(t\in [0,\tau ^R)\),
As a consequence, by again using (A.1), we obtain that
Next we show the convergence in probability of the solution of (2.1) to that of (2.4). Introduce another stopping time \(\tau _{R_1}:=\inf \{t\in [0,T]| |x_t|+|p_t|\ge R_1, |x^{\delta }_{[t]_{\delta }}|+|p^{\delta }_{[t]_{\delta }}|\ge R_1 \}.\) Let \(t\in [0,\tau _{R}\wedge \tau _{R_1}).\) By using the polynomial growth condition of \(f,\sigma \) and the fact that \(\sigma \) is independent of p, we obtain that
where \(C_g\) and \(C_f\) are constants depending on f and g. To deal with the last term, we split it as follows,
Taking expectation on \(II^1\), using the property of the discrete martingale, the a prior estimates for \(H_0(x_t,p_t)\) and \(H_0(x_t^{\delta },p_t^{\delta })\) and Hölder’s inequality, we have that
Similar arguments lead to \({\mathbb {E}}[II^4]\le C(R_1)\delta ^{\frac{1}{2}}.\) For the term \(II^3\), applying the continuity estimate of \(x_t\) and \(x^{\delta }_t,\) as well as independent increments of the Brownian motion, we get
where \(C(R_1)>0\) is monotone with \(R_1.\) Combining the above estimates, we achieve that
Then the Gronwall’s inequality implies that
By making use of (A.2) and Chebshev’s inequality, we conclude that
Here, \({\mathbb {E}}[|x(t)|+|p(t)|+|x^\delta (t)|+|p^\delta (t)|]<C(1+C_R)\) is ensured by \({\mathbb {E}}[\sup \limits _{t\in [0,\tau ^R)} H_0^{2}(x_{t}^{\delta },p_{t}^{\delta })] \le C_{R}.\) Taking limit on \(\delta \rightarrow 0,\) \(R_1\rightarrow \infty \), and \(R \rightarrow \infty \) leads to
Similarly, one could utilize the properties of martingale and obtain the following estimate, for large enough \(q>0,\)
This implies that for large enough \(q>4\),
Combining the above estimate and applying the Chebshev’s inequality, we further obtain
\(\square \)
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Cui, J., Liu, S. & Zhou, H. Stochastic Wasserstein Hamiltonian Flows. J Dyn Diff Equat (2023). https://doi.org/10.1007/s10884-023-10264-4
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DOI: https://doi.org/10.1007/s10884-023-10264-4