Non-spherical gravitational collapse of strange quark matter

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dc.contributor.authorPatil, K. D.
dc.contributor.authorZade, S. S.
dc.contributor.authorMohod, A. N.
dc.date.accessioned2012-03-06T07:31:10Z
dc.date.available2012-03-06T07:31:10Z
dc.date.issued2007-03-10
dc.description.abstractWe study the non-spherical gravitational collapse of the strange quark null fluid. The interesting feature which emerges is that the non-spherical collapse of charged strange quark matter leads to a naked singularity whereas the gravitational collapse of neutral quark matter proceeds to form a black hole. In the present brief report we extend the earlier work of T.Harko and K.S.Cheng to the non-spherical case.en_US
dc.identifier.urihttp://hdl.handle.net/11007/667
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;13/07
dc.subjectGravitational collapseen_US
dc.subjectNaked singularityen_US
dc.subjectBlack holeen_US
dc.subjectTrange quark matteren_US
dc.titleNon-spherical gravitational collapse of strange quark matteren_US
dc.typeArticleen_US

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