A family of well behaved charge analogues of Durgapal’s perfect fluid exact solution in general relativity II

Murad, Mohammad Hassan; Fatema, Saba

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dc.contributor.author	Murad, Mohammad Hassan
dc.contributor.author	Fatema, Saba
dc.date.accessioned	2018-10-15T06:06:36Z
dc.date.accessioned	2019-05-27T09:57:11Z
dc.date.available	2018-10-15T06:06:36Z
dc.date.available	2019-05-27T09:57:11Z
dc.date.issued	2012-12-18
dc.identifier.uri	http://hdl.handle.net/20.500.11948/3393
dc.description.abstract	This paper presents a family of two-parametric interior solutions of Einstein–Maxwell field equations in general relativity for a static spherically symmetric distribution of a charged perfect fluid with particular form of charge distribution. This class of solutions gives us wide range of parameters, n and K, for which the solutions are well behaved hence, suitable for modeling of compact star (e. g. bare strange quark star). The mass of star is maximized with all degree of suitability by assuming the stellar “surface” density equal to strange (quark) matter density at zero pressure. It is hoped that our investigation may be of some help in connection of some study of stellar structure. Full Text Link: https://doi.org/10.1007/s10509-012-1320-2	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.subject	General relativity	en_US
dc.subject	Exact solution	en_US
dc.subject	Static spherically symmetric metric	en_US
dc.subject	Charged fluid sphere	en_US
dc.subject	Compact object	en_US
dc.subject	Curvature coordinates	en_US
dc.subject	Reissener–Nordström	en_US
dc.title	A family of well behaved charge analogues of Durgapal’s perfect fluid exact solution in general relativity II	en_US
dc.type	Article	en_US