Equation of State in the σ - ω - ρ Model Supported by the Observational Data of 4U 1608-52 Neutron Star

Details Equation of State in the σ - ω - ρ Model Supported by the Observational Data of 4U 1608-52 Neutron Star Equation of State in the σ - ω - ρ Model Supported by the Observational Data of 4U 1608-52 Neutron Star

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010chphl..27a0401w&link_type=abstract

Chinese Physics Letters, Volume 27, Issue 1, pp. 010401 (2010).

Physics

3

Scientific paper

The properties of the neutron star rotating at 619Hz (which is the spin frequency of 4U 1608-52 neutron star) are investigated by using an equation of state (EOS) of the nuclear matter in the relativistic σ-ω-ρ model. It is shown that the EOS in the relativistic σ-ω-ρ model is supported by the observational mass and radius of the 4U 1608-52 neutron star. Moreover, a strict constraint on the polar redshift of 4U 1608-52 neutron star is obtained.

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