The compact star in the SU(3) sigma model

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dc.creatorManka, Ryszard
dc.creatorBednarek, Ilona
dc.date2004-11-04
dc.date.accessioned2026-07-07T05:40:42Z
dc.date.available2026-07-07T05:40:42Z
dc.descriptionThe linear chiral SU(3)*SU(3) model is applied to describe properties of the compact star matter inside the quark, protoneutron and neutron star.The leads to the neutron star with the value of maximum mass close to 1.5 solar mass and radius 11 km and with the reduced value of proton fraction and very compact hyperon core.
dc.description15 pages, 6 figures, LaTeX2e,presented at at NAPP 2003 (Dubrovnik), to appear in Fizika
dc.identifierhttps://arxiv.org/abs/nucl-th/0411022
dc.identifierhttp://arxiv.org/abs/nucl-th/0411022
dc.identifierFizika B13 (2004) 355-364
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82331
dc.subjectNuclear Theory
dc.titleThe compact star in the SU(3) sigma model
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