Scalar field collapse and cosmic censorship

dc.contributor.author	Goswami, Rituparno
dc.contributor.author	Joshi, Pankaj S.
dc.contributor.author	Malafarina, D.
dc.date.accessioned	2015-12-23T04:34:54Z
dc.date.available	2015-12-23T04:34:54Z
dc.date.issued	2012-02-28
dc.identifier.citation	Goswami Rituparno, Joshi Pankaj S., Malafarina, D.; 2012; Scalar field collapse and cosmic censorship; 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/123456789/955
dc.description.abstract	We analyze here the final fate of complete gravitational collapse of a massless scalar field within general relativity. A class of dynamical solutions with initial data close to the Friedmann-Lemaˆıtre-Robertson-Walker (FLRW) collapse model is explicitly given and the Einstein equations are integrated numerically in a neighborhood of the center. We show that the initial data space is evenly divided between the dynamical evolutions that terminate in a black hole final state and those that produce a locally naked singularity. We comment on the genericity aspects of the collapse end-states and the connection to cosmic censorship conjecture is pointed out.	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.subject	scalar fields	ru_RU
dc.title	Scalar field collapse and cosmic censorship	ru_RU
dc.type	Article	ru_RU