Phase volume occupied by a test particle around an incipient blackhole
| dc.contributor.author | Padmanabhan, T. | |
| dc.date.accessioned | 2012-03-01T11:48:18Z | |
| dc.date.available | 2012-03-01T11:48:18Z | |
| dc.date.issued | 1989-04-03 | |
| dc.description.abstract | The volume of phase space g( E) available for a system with a definite energy E plays an important role in statistical mechanics. We compute g(E) for a test particle in Schwarzschild geometry and show that it diverges as the source evolves to form a black hole. The implications of the result are discussed. | en_US |
| dc.identifier.uri | http://hdl.handle.net/11007/48 | |
| dc.language.iso | en | en_US |
| dc.publisher | Elsevier Science Publishers | en_US |
| dc.relation.ispartofseries | Physics Letters A;Vol. 136, No. 4, 5, 1989 | |
| dc.subject | Incipient blackhole | en_US |
| dc.subject | Phase volume - non-relativistic potentials | en_US |
| dc.subject | Phase volume - general relativity | en_US |
| dc.title | Phase volume occupied by a test particle around an incipient blackhole | en_US |
| dc.type | Article | en_US |