Gravitational Collapse of Inhomogenous Perfect Fluid

dc.contributor.author	Satin, Seema
dc.contributor.author	Malafarina, D.
dc.contributor.author	Joshi, Pankaj S.
dc.date.accessioned	2015-12-23T08:50:52Z
dc.date.available	2015-12-23T08:50:52Z
dc.date.issued	2014
dc.identifier.citation	Satin Seema, Malafarina D., Joshi Pankaj S.; 2014; Gravitational Collapse of Inhomogenous Perfect Fluid; http://arxiv.org/find/all/1/all:+malafarina/0/1/0/all/0/1	ru_RU
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/966
dc.description.abstract	We study the complete gravitational collapse of a class of inhomogeneous perfect fluid models obtained by introducing small radial perturbations in an otherwise homogeneous matter cloud. The key feature that we assume for the perturbation profile is that of a mass profile that is separable in radial and temporal coordinates. The known models of dust and homogeneous perfect fluid collapse can be obtained from this choice of the mass profile as special cases. This choice is very general and physically well motivated and we show that this class of collapse models can lead to the formation of a naked singularity as the final state.	ru_RU
dc.language.iso	en	ru_RU
dc.subject	Research Subject Categories::NATURAL SCIENCES::Physics	ru_RU
dc.subject	gravitational collapse	ru_RU
dc.subject	black holes	ru_RU
dc.subject	naked singularities	ru_RU
dc.title	Gravitational Collapse of Inhomogenous Perfect Fluid	ru_RU
dc.type	Article	ru_RU