The quark strange star in the enlarged Nambu-Jona-Lasinio model

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DC pole	Wartość	Język
dc.contributor.author	Mańka, Ryszard	-
dc.contributor.author	Bednarek, Ilona	-
dc.contributor.author	Przybyła, Grzegorz	-
dc.date.accessioned	2017-12-02T14:52:30Z	-
dc.date.available	2017-12-02T14:52:30Z	-
dc.date.issued	2002-03-13	-
dc.identifier.citation	New Journal of Physics, 2002, vol. 4, p. 14.1-14.18	-
dc.identifier.issn	1367-2630	-
dc.identifier.uri	http://hdl.handle.net/20.500.12128/517	-
dc.description.abstract	The strange quark star is investigated within the enlarged SU(3) Nambu-Jona-Lasinio model. The stable quark star can exist until a maximal configuration with ρm = 3.1 × 1015 g cm -3 with Mm = 1.61 M⊙ and Rm = 8.74 km is reached. Strange quarks appear for density above ρc = 9.84 g cm-3 for the quark star with radius Rc = 8.003 km and Mc = 0.77M⊙. A comparison of quark star properties obtained in the quark mean-field approach to a neutron star model constructed within the relativistic mean-field theory is presented.	pl_PL
dc.language.iso	en	pl_PL
dc.rights	Uznanie autorstwa 3.0 Polska	*
dc.rights.uri	http://creativecommons.org/licenses/by/3.0/pl/	*
dc.subject	Nambu-Jona-Lasinio model	pl_PL
dc.subject	Mean-Field Theory	pl_PL
dc.subject	Nuclear-Matter	pl_PL
dc.subject	Neutron-Stars	pl_PL
dc.subject	Dense Matter	pl_PL
dc.subject	Hadrons	pl_PL
dc.title	The quark strange star in the enlarged Nambu-Jona-Lasinio model	pl_PL
dc.type	info:eu-repo/semantics/article	pl_PL
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