2005/08/19 by Pierre Noundjeu, P. Noundjeu, Noundjeu, P.
Economics, Econometrics and Finance · Engineering · Mathematics · Physics and Astronomy · #FOS: Physical sciences #Fluid Dynamics and Turbulent Flows #Gas Dynamics and Kinetic Theory #General Relativity and Quantum Cosmology (gr-qc) #Stochastic processes and financial applications #gr-qc
paper · pdf · doi:10.48550/arxiv.gr-qc/0508078
16 pages
arxiv created 2005/08/19 · openalex publication_date 2005/08/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The Einstein-Vlasov-Maxwell (EVM) system can be viewed as a relativistic generalization of the Vlasov-Poisson (VP) system. As it is proved below, one of nice property obeys by the first system is that the strong energy condition holds and this allows to conclude that the above system is physically viable. We show in this paper that in the context of spherical symmetry, solutions of the perturbed (EVM) system by γ:= 1/c2, c being the speed of light, exist and converge uniformly in L∞-norm, as c goes to infinity on compact time intervals to solutions of the non-relativistic (VP) system.