Long time estimates for the Vlasov-Maxwell system in the non-relativistic limit
arXiv:1710.03335 · doi:10.1007/s00220-018-3208-7
Abstract
In this paper, we study the Vlasov-Maxwell system in the non-relativistic limit, that is in the regime where the speed of light is a very large parameter. We consider data lying in the vicinity of homogeneous equilibria that are stable in the sense of Penrose (for the Vlasov-Poisson system), and prove Sobolev stability estimates that are valid for times which are polynomial in terms of the speed of light and of the inverse of size of initial perturbations. We build a kind of higher-order Vlasov-Darwin approximation which allows us to reach arbitrarily large powers of the speed of light.
References in corpus (6)
- Strichartz estimates and moment bounds for the relativistic Vlasov-Maxwell system I. The -D and -D cases
- Strichartz estimates and moment bounds for the relativistic Vlasov-Maxwell system II. Continuation criteria in the 3D case
- Landau Damping in Relativistic Plasmas
- Landau damping for the linearized Vlasov Poisson equation in a weakly collisional regime
- Partially strong transparency conditions and a singular localization method in geometric optics
- Instabilities in the mean field limit