Stochastic Euler Schemes and Dissipative Evolutions in the Space of Probability Measures
Giulia Cavagnari, Giuseppe Savaré, Giacomo Enrico Sodini
TL;DR
This work develops a measure-theoretic framework for the convergence of stochastic time-discretization schemes, notably the explicit Euler method, for evolution equations driven by random velocity fields in the space of probability measures. By recasting dynamics as multivalued probability vector fields (MPVFs) on $(oldsymbol{P}_2(oldsymbol{X}), W_2)$ and employing barycentric projections, the authors prove strong convergence of interpolated trajectory laws to the $oldsymbol{\lambda}$-evolution variational inequality (EVI) solution generated by the maximal dissipative extension of the barycenter. They establish lifting results that connect discrete Euler updates with continuous-time curve measures, derive semigroup structures under total dissipativity, and show stability under approximations. The framework is illustrated through stochastic dissipative flows and nonlocal interaction fields, covering stochastic gradient-descent-like dynamics and interacting particle systems, which highlights the approach’s broad applicability to continuous-time stochastic schemes in measure spaces.
Abstract
We study the convergence of stochastic time-discretization schemes for evolution equations driven by random velocity fields, including examples like stochastic gradient descent and interacting particle systems. Using a unified framework based on Multivalued Probability Vector Fields, we analyze these dynamics at the level of probability measures in the Wasserstein space. Under suitable dissipativity and boundedness conditions, we prove that the laws of the interpolated trajectories converge to those of a limiting evolution governed by a maximal dissipative extension of the associated barycentric field. This provides a general measure-theoretic study for the convergence of stochastic schemes in continuous time.
