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Enigmatic aspects of entropy inside the black hole: what do falling comoving observers see?

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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


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