Hyperons in anisotropic neutron star

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Abstract

The influence of modification of one of the assumptions in standard non-rotating static neutron star calculation i.e., the anisotropic pressure of neutron star matter with hyperons in its core within the framework of extended relativistic mean field model is investigated. It is found that the maximum mass and the redshift predictions are quite compatible with the recent observational constraints if this assumption is relaxed.

Original languageEnglish
Article number012003
JournalJournal of Physics: Conference Series
Volume539
Issue number1
DOIs
Publication statusPublished - 1 Jan 2014
Event11th Conference of Theoretical Physics and Nonlinear Phenomena: From Universe to String's Scale, CTPNP 2014 - Surakarta, Indonesia
Duration: 15 Feb 201415 Feb 2014

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