Abstract

We investigate a system of N Brownian particles with the Coulomb interaction in any dimension \(d\ge 2\), and we assume that the initial data are independent and identically distributed with a common density \(\rho _0\) satisfying \(\int _{\mathbb {R}^{d}}\rho _0\ln \rho _0\,\hbox {d}x<\infty \) and \(\rho _0\in L^{\frac{2d}{d+2}} (\mathbb {R}^{d}) \cap L^1(\mathbb {R}^{d}, (1+|x|^2)\,\hbox {d}x)\). We prove that there exists a unique global strong solution for this interacting partsicle system and there is no collision among particles almost surely. For \(d=2\), we rigorously prove the propagation of chaos for this particle system globally in time without any cutoff in the following sense. When \(N\rightarrow \infty \), the empirical measure of the particle system converges in law to a probability measure and this measure possesses a density which is the unique weak solution to the mean-field Poisson–Nernst–Planck equation of single component.

Highlights

  • Let, F, P be a probability space, endowed with the standard d-dimensional Brownian motions associated with this space

  • For d = 2, we rigorously prove the propagation of chaos for this particle system globally in time without any cutoff in the following sense

  • 1 Background Let, F, P be a probability space, endowed with the standard d-dimensional Brownian motions associated with this space

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Summary

Background

Let , F , P be a probability space, endowed with the standard d-dimensional Brownian motions associated with this space. With the uniform estimates of entropy and the second moments for the particle system (1.1), Lemma 3.2 shows that (μt (ω))t≥0 has a density (ρt (ω))t≥0 a.s. Using the fact that μ(ω) is a.s. a solution to the self-consistent martingale problem in Definition 1, Theorem 5.2 shows that ρ(ω) is the unique weak solution to the mean-field Poisson–Nernst–Planck (PNP) equations of single component:. Lemma 2.2 Let {(Xti,ε)t≥0}Ni=1 be the unique strong solution to (2.14) and (ftN,ε)t≥0 be its joint time marginal distribution with density (ρtN,ε)t≥0. Lemma 2.3 Let {(Xti,ε)t≥0}Ni=1 be the unique strong solution to (2.14) and (ρtN,ε)t≥0 be its joint time marginal density. Combining (2.90), (2.91), (2.92), (2.93) and (2.94), letting ε → 0 in (2.89), one has ρN satisfies the following equation ρ0N φ dX t 0 i=j t φρN dXds. Combining the regularity of ρN from Lemma 2.3, we obtain that ρN is exactly a weak solution to (2.1). We have concluded the proof of Theorem 2.1 so far

Tightness of the empirical measures
Propagation of chaos for 2D
Propagation of chaos result
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