The Stability of an Isentropic Model for a Gaseous Relativistic Star
| dc.creator | Negi, P. S. | |
| dc.date | 2007-02-01 | |
| dc.date.accessioned | 2026-07-07T10:37:13Z | |
| dc.date.available | 2026-07-07T10:37:13Z | |
| dc.description | We show that the isentropic subclass of Buchdahl's exact solution for a gaseous relativistic star is stable and gravitationally bound for all values of the compactness ratio $u [\equiv (M/R)$, where $M$ is the total mass and $R$ is the radius of the configuration in geometrized units] in the range, $0 < u \leq 0.20$, corresponding to the {\em regular} behaviour of the solution. This result is in agreement with the expectation and opposite to the earlier claim found in the literature. | |
| dc.description | 9 pages (including 1 table); accepted for publication in GRG | |
| dc.identifier | https://arxiv.org/abs/gr-qc/0702005 | |
| dc.identifier | http://arxiv.org/abs/gr-qc/0702005 | |
| dc.identifier | Gen.Rel.Grav.39:529-534,2007 | |
| dc.identifier | doi:10.1007/s10714-007-0402-x | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180308 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The Stability of an Isentropic Model for a Gaseous Relativistic Star | |
| dc.type | text |