The general solution for relativistic spherical shells
| dc.contributor.author | Kijowski, J. | |
| dc.contributor.author | Magli, G. | |
| dc.contributor.author | Malafarina, D. | |
| dc.date.accessioned | 2015-12-23T09:19:18Z | |
| dc.date.available | 2015-12-23T09:19:18Z | |
| dc.date.issued | 2005 | |
| dc.description.abstract | The general exact solution of the Einstein-matter field equations describing spherically symmetric shells satisfying an equation of state in closed form is discussed under general assumptions of physical reasonableness. The solutions split into two classes: a class of “astrophysically interesting” solutions describing “ordinary” matter with positive density and pressure, and a class of “phantom-like” solutions with positive density but negative active gravitational mass, which can also be of interest in several “very strong fields” regimes. Known results on linear-barotropic equations of state are recovered as particular cases. | ru_RU |
| dc.identifier.citation | Kijowski J., Magli G., Malafarina D.; 2005; The general solution for relativistic spherical shells; http://arxiv.org/find/all/1/all:+malafarina/0/1/0/all/0/1 | ru_RU |
| dc.identifier.uri | http://nur.nu.edu.kz/handle/123456789/968 | |
| dc.language.iso | en | ru_RU |
| dc.subject | Research Subject Categories::NATURAL SCIENCES::Physics | ru_RU |
| dc.subject | astrophysics | ru_RU |
| dc.subject | gravitational collapse | ru_RU |
| dc.title | The general solution for relativistic spherical shells | ru_RU |
| dc.type | Article | ru_RU |