Structure of a Warm Hyperon Star

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DC pole	Wartość	Język
dc.contributor.author	Bednarek, Ilona	-
dc.contributor.author	Pieńkos, Monika	-
dc.date.accessioned	2018-11-20T08:25:58Z	-
dc.date.available	2018-11-20T08:25:58Z	-
dc.date.issued	2011	-
dc.identifier.citation	Acta Physica Polonica B, Vol. 42, no. 11 (2011), s. 2221-2228	pl_PL
dc.identifier.issn	0587-4254	-
dc.identifier.uri	http://hdl.handle.net/20.500.12128/7122	-
dc.description.abstract	The analysis based on the relativistic mean field (RMF) theory with the isoscalar–isovector interactions has been performed in order to study properties of a warm, asymmetric nuclear matter in -equilibrium. The influence of this additional meson interactions on the composition and structure of a neutron star has been studied. The obtained results refer to the case with only nucleon degree of freedom and to a neutron star matter which includes hyperons.	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	gwiazdy neutronowe	pl_PL
dc.subject	hiperony	pl_PL
dc.subject	astrofizyka jądrowa	pl_PL
dc.title	Structure of a Warm Hyperon Star	pl_PL
dc.type	info:eu-repo/semantics/article	pl_PL
dc.identifier.doi	10.5506/APhysPolB.42.2221	-
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