DC pole | Wartość | Język |
dc.contributor.author | Pieńkos, Monika | - |
dc.date.accessioned | 2018-11-16T11:18:25Z | - |
dc.date.available | 2018-11-16T11:18:25Z | - |
dc.date.issued | 2013 | - |
dc.identifier.citation | Acta Physica Polonica B, Vol. 44, no. 11 (2013), s. 2389-2395 | pl_PL |
dc.identifier.issn | 0587-4254 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/7095 | - |
dc.description.abstract | The 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.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 | równania stanu | pl_PL |
dc.subject | fizyka matematyczna | pl_PL |
dc.title | Neutrinos in proto-neutron star models | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
dc.identifier.doi | 10.5506/APhysPolB.44.2389 | - |
Pojawia się w kolekcji: | Artykuły (WNŚiT)
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