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The neutron star in the Relativistic Mean-Field Theory

Ryszard Manka·Ilona Bednarek·Grzegorz Przybyla
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Abstract

The nucleon effective mass, binding energy and neutron star configuration in the Relativistic Mean-Field Theory (RMF) is considered. The calculation are motivated by the construction of the equation of state for a neutron star in the RMF. The equation of state for the parameters set TM1 is calculated using the Feynman - Bogolubov variational method for temperature different from zero. The structure of the neutron star is presented. The maximal stable configuration are obtained for: M_max=1.91 M_Sun and R=12.84 km.

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Ryszard Manka, Ilona Bednarek, Grzegorz Przybyla. 2000-01-09. The neutron star in the Relativistic Mean-Field Theory. https://doi.org/10.1103/physrevc.62.015802

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