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 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 struct...

Full description

Bibliographic Details
Main Authors: Ilona Bednarek, Ryszard Manka, Monika Pienkos
Format: Article
Language:English
Published: Public Library of Science (PLoS) 2014-01-01
Series:PLoS ONE
Online Access:http://europepmc.org/articles/PMC4154698?pdf=render