Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3313

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DC Field	Value	Language
dc.contributor.author	Bombaci, I	-
dc.contributor.author	Thampan, A. V	-
dc.contributor.author	Datta, B	-
dc.date.accessioned	2008-09-01T10:35:52Z	-
dc.date.available	2008-09-01T10:35:52Z	-
dc.date.issued	2000-10	-
dc.identifier.citation	Astrophysical Journal, Vol. 541, No. 2, Part 2, pp. L71 - L74	en
dc.identifier.issn	0004-637X	-
dc.identifier.uri	http://hdl.handle.net/2248/3313	-
dc.description.abstract	For a new equation of state of strange quark matter, we construct equilibrium sequences of rapidly rotating strange stars in general relativity. The sequences are the normal and supramassive evolutionary sequences of constant rest mass. We also calculate equilibrium sequences for a constant value of Ω corresponding to the most rapidly rotating pulsar PSR 1937+21. In addition, we calculate the radius of the marginally stable orbit and its dependence on Ω, relevant for modeling of kilohertz quasi-periodic oscillations in X-ray binaries.	en
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://www.journals.uchicago.edu/doi/abs/10.1086/312897	en
dc.subject	Equation of State	en
dc.subject	Relativity	en
dc.subject	Stars: Neutron	en
dc.title	Rapidly Rotating Strange Stars for a New Equation of State of Strange Quark Matter	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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