Abstract
The Euler-Maxwell system describes the evolution of a plasma when the collisions are important enough that each species is in a hydrodynamic equilibrium. In this paper we prove global existence of small solutions to this system set in the whole three-dimensional space, by combining the space-time resonance method and energy estimates.
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Schedule a callMore From: Annales Scientifiques de lʼ&E.cute;cole Normale Supérieure
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