General relativistic model for mixed fluid sphere with equation of state

Ragel, F. C.; Thirukkanesh, S.

dc.contributor.author	Ragel, F. C.
dc.contributor.author	Thirukkanesh, S.
dc.date.accessioned	2019-08-08T03:31:33Z
dc.date.available	2019-08-08T03:31:33Z
dc.date.issued	2019
dc.identifier.uri	http://www.digital.lib.esn.ac.lk/handle/123456789/3935
dc.description.abstract	We generate a general frame work to solve the Einstein system with an equation of state that describe static spherically symmetric anisotropic matter distribution in terms of a generating function. It is examined for a Van der Waals type equation of state with a physically reasonable form of generating function. The model satisfies all the required major physical properties of a realistic star. It is shown to be stable in the low-density regime that may represent a liquid–gas mixed fluid sphere.	en_US
dc.language.iso	en	en_US
dc.publisher	The European Physical Journal	en_US
dc.title	General relativistic model for mixed fluid sphere with equation of state	en_US
dc.type	Article	en_US
dc.identifier.sslno	01	en_US