Gravitational collapse without a remnant
| dc.creator | Chang, Zhe | |
| dc.creator | Guan, Cheng-Bo | |
| dc.creator | Huang, Chao-Guang | |
| dc.creator | Li, Xin | |
| dc.date | 2008-04-24 | |
| dc.date.accessioned | 2026-07-07T11:50:11Z | |
| dc.date.available | 2026-07-07T11:50:11Z | |
| dc.description | We investigate the gravitational collapse of a spherically symmetric, inhomogeneous star, which is described by a perfect fluid with heat flow and satisfies the equation of state $p=ρ/3$ or $p=Cρ^\ga$ at its center. Different from the ordinary process of gravitational collapsing, the energy of the whole star is emitted into space. And the remaining spacetime is a Minkowski one at the end of the process. | |
| dc.description | 9 pages, 9 figures, to appear in Int. J. Theor. Phys | |
| dc.identifier | https://arxiv.org/abs/0804.3892 | |
| dc.identifier | http://arxiv.org/abs/0804.3892 | |
| dc.identifier | Int.J.Theor.Phys.47:2479-2491,2008 | |
| dc.identifier | doi:10.1007/s10773-008-9681-6 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/203481 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gravitational collapse without a remnant | |
| dc.type | text |