The influence of the enhanced vector meson sector on the properties of the matter of neutron stars.
basic_science · Level V
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- Record sourced from PubMed, PMID 25188304.
- Also identified by DOI 10.1371/journal.pone.0106368 and PMC identifier PMC5255077.
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Abstract
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 x SU(3)R symmetry. The emphasis is put on the physical properties of the matter of a neutron star as well as on its internal structure. 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.