Phase Transition and Hybrid Star in a Nonlinear $\sigma - \omega$ model

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3128

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DC Field	Value	Language
dc.contributor.author	Acharya, S	-
dc.contributor.author	Maharana, L	-
dc.contributor.author	Mohanty, R	-
dc.contributor.author	Panda, P. K	-
dc.date.accessioned	2008-08-14T06:21:11Z	-
dc.date.available	2008-08-14T06:21:11Z	-
dc.date.issued	1999-04	-
dc.identifier.citation	International Journal of Modern Physics E, Vol. 8, No. 2, pp. 107 - 120	en
dc.identifier.uri	http://hdl.handle.net/2248/3128	-
dc.description.abstract	The phase transition between the nuclear matter and the quark matter is examined. The relativistic mean field theory(RMF) is consider with interacting nucleons and mesons using TM1 parameter set for the nuclear matter equations of state. It is found that the trasition point depends on coupling constant $\alpha_s$ and bag pressure. From the study of the structure of a hybrid neutron star, it is observed that the star contains quark matter in the interior and neutron matter on the outer perifery.	en
dc.format.extent	161024 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	World Scientific	en
dc.relation.uri	http://arxiv.org/abs/nucl-th/9811041v1	en
dc.subject	Nuclear Theory	en
dc.subject	Phase Transition	en
dc.subject	Hybrid Star	en
dc.title	Phase Transition and Hybrid Star in a Nonlinear $\sigma - \omega$ model	en
dc.type	Article	en
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