The neutron star in the Relativistic Mean-Field Theory

Details The neutron star in the Relativistic Mean-Field Theory The neutron star in the Relativistic Mean-Field Theory

2000-01-09

arxiv.org/abs/nucl-th/0001017v1

Phys.Rev. C62 (2000) 015802

Physics

Nuclear Physics

Nuclear Theory

21 pages, latex2e, JHEP, 12 eps figures

Scientific paper

10.1103/PhysRevC.62.015802

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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