On the non-relativistic limit of the spherically symmetric Einstein-Vlasov-Maxwell system
| dc.creator | Noundjeu, P. | |
| dc.date | 2005-08-19 | |
| dc.date.accessioned | 2026-07-07T03:29:54Z | |
| dc.date.available | 2026-07-07T03:29:54Z | |
| dc.description | 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 $γ:= 1/c^{2}$, $c$ being the speed of light, exist and converge uniformly in $L^{\infty}$-norm, as $c$ goes to infinity on compact time intervals to solutions of the non-relativistic (VP) system. | |
| dc.description | 16 pages | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0508078 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0508078 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/35367 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | On the non-relativistic limit of the spherically symmetric Einstein-Vlasov-Maxwell system | |
| dc.type | text |