Exact solution for the interior of a black hole
| dc.creator | Nieuwenhuizen, Theo M. | |
| dc.date | 2008-05-27 | |
| dc.date.accessioned | 2026-07-07T09:41:08Z | |
| dc.date.available | 2026-07-07T09:41:08Z | |
| dc.description | Within the Relativistic Theory of Gravitation it is shown that the equation of state $p=ρ$ holds near the center of a black hole. For the stiff equation of state $p=ρ-ρ_c$ the interior metric is solved exactly. It is matched with the Schwarzschild metric, which is deformed in a narrow range beyond the horizon. The solution is regular everywhere, with a specific shape at the origin. The gravitational redshift at the horizon remains finite but is large, $z\sim 10^{23}$$M_\odot/M$. Time keeps its standard role also in the interior. The energy of the Schwarzschild metric, shown to be minus infinity in the General Theory of Relativity, is regularized in this setup, resulting in $E=Mc^2$. | |
| dc.description | 12 pages newFNLstyle. 4 figures | |
| dc.identifier | https://arxiv.org/abs/0805.4169 | |
| dc.identifier | http://arxiv.org/abs/0805.4169 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/161724 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Exact solution for the interior of a black hole | |
| dc.type | text |