The general solution for relativistic spherical shells

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dc.contributor.author	Kijowski, J.
dc.contributor.author	Magli, G.
dc.contributor.author	Malafarina, D.
dc.date.accessioned	2015-12-23T09:19:18Z
dc.date.available	2015-12-23T09:19:18Z
dc.date.issued	2005
dc.identifier.citation	Kijowski J., Magli G., Malafarina D.; 2005; The general solution for relativistic spherical shells; 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/123456789/968
dc.description.abstract	The general exact solution of the Einstein-matter field equations describing spherically symmetric shells satisfying an equation of state in closed form is discussed under general assumptions of physical reasonableness. The solutions split into two classes: a class of “astrophysically interesting” solutions describing “ordinary” matter with positive density and pressure, and a class of “phantom-like” solutions with positive density but negative active gravitational mass, which can also be of interest in several “very strong fields” regimes. Known results on linear-barotropic equations of state are recovered as particular cases.	ru_RU
dc.language.iso	en	ru_RU
dc.subject	Research Subject Categories::NATURAL SCIENCES::Physics	ru_RU
dc.subject	astrophysics	ru_RU
dc.subject	gravitational collapse	ru_RU
dc.title	The general solution for relativistic spherical shells	ru_RU
dc.type	Article	ru_RU