Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5628
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSivaram, C-
dc.contributor.authorArun, K-
dc.date.accessioned2011-12-07T14:40:25Z-
dc.date.available2011-12-07T14:40:25Z-
dc.date.issued2012-01-
dc.identifier.citationAstrophysics and Space Science, Vol. 337, No. 1, pp. 169-172en
dc.identifier.urihttp://hdl.handle.net/2248/5628-
dc.descriptionRestricted Accessen
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractIn 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.isoenen
dc.publisherSpringeren
dc.relation.urihttp://dx.doi.org/10.1007/s10509-011-0844-1en
dc.rights© Springeren
dc.subjectBlack hole entropyen
dc.subjectMutual gravitational interactionsen
dc.subjectGravitational collapseen
dc.titleEnigmatic aspects of entropy inside the black hole: what do falling comoving observers see?en
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Enigmatic aspects of entropy inside the black hole.pdf
  Restricted Access
Restricted Access285.98 kBAdobe PDFView/Open Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.