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The influence of the enhanced vector meson sector on the properties of the matter of neutron stars

This paper gives an overview of the model of a neutron star with non-zero strangeness constructed within the framework of the nonlinear realization of the chiral $SU(3)_{L}\times SU(3)_{R}$ symmetry. The emphasis is put on the physical properties of the matter of a neutron star. The obtained solution is particularly aimed at the problem of the construction of a theoretical model of a neutron star matter with hyperons that will give high value of the maximum mass.

preprint2013arXivOpen access
Ilona BednarekRyszard MankaMonika Pienkos
nucl-thastro-ph.SR
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Ilona BednarekRyszard MankaMonika Pienkos

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