Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3281

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DC Field	Value	Language
dc.contributor.author	Panda, P. K	-
dc.contributor.author	Sahu, R	-
dc.contributor.author	Das, C	-
dc.date.accessioned	2008-09-01T09:15:54Z	-
dc.date.available	2008-09-01T09:15:54Z	-
dc.date.issued	1999-09	-
dc.identifier.citation	Physical review C, Vol. 60, No. 3, pp. 038801 - 038804	en
dc.identifier.issn	0556-2813	-
dc.identifier.uri	http://hdl.handle.net/2248/3281	-
dc.description.abstract	A mean-field description of nonoverlaping nucleon bags bound by the self-consistent exchange of σ, ω, and ρ mesons is used to investigate the properties of neutron matter at finite temperature. We use the equation of state of zero temperature to study the rotating neutron star in the Komatsu-Eriguchi-Hachisu method. The mass, radius, and angular velocity of the neutron star are calculated and compared with the Walecka model.	en
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRC/v60/e038801	en
dc.subject	Neutron matter	en
dc.subject	Quark meson coupling model	en
dc.title	Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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