DC pole | Wartość | Język |
dc.contributor.author | Bednarek, Ilona | - |
dc.date.accessioned | 2018-11-24T09:45:19Z | - |
dc.date.available | 2018-11-24T09:45:19Z | - |
dc.date.issued | 2009 | - |
dc.identifier.citation | Acta Physica Polonica B, Vol. 40, no. 11 (2009), s. 3071-3077 | pl_PL |
dc.identifier.issn | 0587-4254 | - |
dc.identifier.uri | http://hdl.handle.net/20.500.12128/7208 | - |
dc.description.abstract | The extended nonlinear model has been applied to construct neutron star matter equation of state. In the case of neutron star matter with nonzero strangeness the extension of the vector meson sector by the inclusion
of nonlinear mixed terms results in the stiffening of the equation of state and accordingly in the higher value of the maximum neutron star mass. | 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 | materia jądrowa | pl_PL |
dc.title | Hyperon Star | pl_PL |
dc.type | info:eu-repo/semantics/article | pl_PL |
Pojawia się w kolekcji: | Artykuły (WNŚiT)
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