Nuclear matter in the derivative scalar coupling model. Energy per nucleon and a finite temperature equation of state

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3902

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DC Field	Value	Language
dc.contributor.author	Datta, B	-
dc.contributor.author	Sahu, P. K	-
dc.date.accessioned	2008-09-26T16:55:31Z	-
dc.date.available	2008-09-26T16:55:31Z	-
dc.date.issued	1993-12-02	-
dc.identifier.citation	Physics Letters B, Vol. 318, No. 2, pp. 277 - 280	en
dc.identifier.issn	0370-2693	-
dc.identifier.uri	http://hdl.handle.net/2248/3902	-
dc.description	Restricted Access	-
dc.description.abstract	We calculate an equation of state of nuclear matter based on the derivative scalar coupling model proposed by Zimanyi and Moszkowski, using improved values of the saturation density and binding energy. Comparison of this model's prediction for the energy per nucleon is made with available estimates from heavy-ion collision data and with the theoretical requirement for a prompt type II supernova bounce. We also derive a finite temperature equation of state for nuclear matter based on this model	en
dc.language.iso	en	en
dc.publisher	Elsevier Science B.V.	en
dc.relation.uri	http://dx.doi.org/10.1016/0370-2693(93)90128-5	en
dc.subject	Scalar coupling model	en
dc.subject	Nucleon	en
dc.subject	Binding energy	en
dc.subject	Supernova	en
dc.title	Nuclear matter in the derivative scalar coupling model. Energy per nucleon and a finite temperature equation of state	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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