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 |