The Influence of the Enhanced Vector Meson Sector on the Properties of the Matter of Neutron Stars
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 $SU(3)_{L}\times SU(3)_{R}$ 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.
- Publication:
-
PLoS ONE
- Pub Date:
- September 2014
- DOI:
- 10.1371/journal.pone.0106368
- arXiv:
- arXiv:1312.3219
- Bibcode:
- 2014PLoSO...9j6368B
- Keywords:
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- Astrophysics - Solar and Stellar Astrophysics;
- Nuclear Theory
- E-Print:
- 13 pages, 17 figures