| dc.contributor.author | Sivaram, C | |
| dc.contributor.author | Arun, K | |
| dc.date.accessioned | 2011-12-07T14:40:25Z | |
| dc.date.available | 2011-12-07T14:40:25Z | |
| dc.date.issued | 2012-01 | |
| dc.identifier.citation | Astrophysics and Space Science, Vol. 337, No. 1, pp. 169-172 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/5628 | |
| dc.description | Restricted Access | en |
| dc.description | The original publication is available at springerlink.com | |
| dc.description.abstract | In a recent paper it was suggested that inclusion of mutual gravitational interactions can give a possible scenario for reversing gravitation collapse and averting a singular phase. We extend this idea to the still unsolved problem of matter collapsing beyond black hole event horizons. For a comoving observer there is no change in entropy as he goes through the horizon. Matter collapses to a minimum radius, and then can re-expand with the same entropy. It is shown that phase space inside a collapsing black hole is also invariant. | en |
| dc.language.iso | en | en |
| dc.publisher | Springer | en |
| dc.relation.uri | http://dx.doi.org/10.1007/s10509-011-0844-1 | en |
| dc.rights | © Springer | en |
| dc.subject | Black hole entropy | en |
| dc.subject | Mutual gravitational interactions | en |
| dc.subject | Gravitational collapse | en |
| dc.title | Enigmatic aspects of entropy inside the black hole: what do falling comoving observers see? | en |
| dc.type | Article | en |