Monge-Amp\`ere gravitation as a $\Gamma$-limit of good rate functions
Abstract
Monge-Amp\`ere gravitation is a modification of the classical Newtonian gravitation where the linear Poisson equation is replaced by the nonlinear Monge-Amp\`ere equation. This paper is concerned with the rigorous derivation of Monge-Amp\`ere gravitation for a finite number of particles from the stochastic model of a Brownian point cloud, in the spirit of a previous work by the third author [A double large deviation principle for Monge-Amp\`ere gravitation, 2016]. The main step in this derivation is the convergence of the good rate functions corresponding to a one-parameter family of large deviation principles. Surprisingly, the derived model includes dissipative phenomena. As an illustration, we show that it leads to sticky collisions in one space dimension.
Keywords
Cite
@article{arxiv.2002.11966,
title = {Monge-Amp\`ere gravitation as a $\Gamma$-limit of good rate functions},
author = {Luigi Ambrosio and Aymeric Baradat and Yann Brenier},
journal= {arXiv preprint arXiv:2002.11966},
year = {2023}
}