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.
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Source |
|---|---|
| http://www.ncbi.nlm.nih.gov/pmc/articles/PMC4154698 | PMC |
| http://journals.plos.org/plosone/article?id=10.1371/journal.pone.0106368 | PLOS |
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