Isospin asymmetry and neutron star properties

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DC pole	Wartość	Język
dc.contributor.author	Bednarek, Ilona	-
dc.contributor.author	Pieńkos, Monika	-
dc.date.accessioned	2018-11-06T15:06:00Z	-
dc.date.available	2018-11-06T15:06:00Z	-
dc.date.issued	2017	-
dc.identifier.citation	Acta Physica Polonica B, Vol. 48, no. 12 (2017), s. 2365-2374	pl_PL
dc.identifier.issn	0587-4254	-
dc.identifier.uri	http://hdl.handle.net/20.500.12128/6971	-
dc.description.abstract	Asymmetric nuclear matter is studied within the relativistic mean field approach. Models with the ω-ρ and σ-ρ cross-interactions, through their remarkable ability to modify the density dependence of the symmetry energy, have been used to analyse the saturation properties of asymmetric nuclear matter.	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	gwiazda neutronowa	pl_PL
dc.subject	izospin	pl_PL
dc.title	Isospin asymmetry and neutron star properties	pl_PL
dc.type	info:eu-repo/semantics/article	pl_PL
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