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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/7095
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dc.contributor.authorPieńkos, Monika-
dc.date.accessioned2018-11-16T11:18:25Z-
dc.date.available2018-11-16T11:18:25Z-
dc.date.issued2013-
dc.identifier.citationActa Physica Polonica B, Vol. 44, no. 11 (2013), s. 2389-2395pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/7095-
dc.description.abstractThe equation of state (EoS) of a hot proto-neutron star matter with trapped neutrinos was calculated within the effective SU(3) theory with the enhanced vector meson sector.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectgwiazdy neutronowepl_PL
dc.subjectrównania stanupl_PL
dc.subjectfizyka matematycznapl_PL
dc.titleNeutrinos in proto-neutron star modelspl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.identifier.doi10.5506/APhysPolB.44.2389-
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