Formation of a galaxy with a central black hole in the Lemaitre-Tolman model
| dc.creator | Krasinski, Andrzej | |
| dc.creator | Hellaby, Charles | |
| dc.date | 2003-09-25 | |
| dc.date | 2004-01-06 | |
| dc.date.accessioned | 2026-07-07T11:42:55Z | |
| dc.date.available | 2026-07-07T11:42:55Z | |
| dc.description | We construct two models of the formation a galaxy with a central black hole, starting from a small initial fluctuation at recombination. This is an application of previously developed methods to find a Lemaitre-Tolman model that evolves from a given initial density or velocity profile to a given final density profile. We show that the black hole itself could be either a collapsed object, or a non-vacuum generalisation of a full Schwarzschild-Kruskal-Szekeres wormhole. Particular attention is paid to the black hole's apparent and event horizons. | |
| dc.description | REVTeX, 22 pages including 11 figures (25 figure files). Replacement has minor changes in response to the referee, and editorial corrections. To appear in PRD | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0309119 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0309119 | |
| dc.identifier | Phys.Rev.D69:043502,2004 | |
| dc.identifier | doi:10.1103/PhysRevD.69.043502 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/201055 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Formation of a galaxy with a central black hole in the Lemaitre-Tolman model | |
| dc.type | text |