The surface-symmetric Einstein-Vlasov system with cosmological constant
| dc.creator | Tchapnda, Sophonie Blaise | |
| dc.creator | Noutchegueme, Norbert | |
| dc.date | 2003-04-25 | |
| dc.date | 2003-10-17 | |
| dc.date.accessioned | 2026-07-07T03:27:48Z | |
| dc.date.available | 2026-07-07T03:27:48Z | |
| dc.description | The results on local existence and continuation criteria obtained by G. Rein in [4] are extended to the case with a non-zero cosmological constant. It is also shown that for the spherically symmetric case and a positive cosmological constant there is a large class of initial data with global existence and inflationary asymptotics in the future as in the case of plane or hyperbolic symmetry treated in [7]. Furthermore we analyze the behaviour of the energy-momentum tensor at late times. | |
| dc.description | 15 pages, proofs shortened, new global results | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0304098 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0304098 | |
| dc.identifier | Math.Proc.Cambridge Phil.Soc. 138 (2005) 541-553 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/34575 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The surface-symmetric Einstein-Vlasov system with cosmological constant | |
| dc.type | text |