Structure and properties of neutron stars in the Relativistic Mean - Field Theory

Details Structure and properties of neutron stars in the Relativistic Mean - Field Theory Structure and properties of neutron stars in the Relativistic Mean - Field Theory

2000-12-08

arxiv.org/abs/nucl-th/0012026v1

Int.J.Mod.Phys. D10 (2001) 607-624

Physics

Nuclear Physics

Nuclear Theory

18 pages, latex2e, 10 colour eps figures, submitted to International Journal of Modern Physics

Scientific paper

10.1142/S0218271801001104

Properties of rotating neutron stars with the use of relativistic mean-field theory are considered. The performed analysis of neutron star matter is based on the nonlinear Lgrangian density. The presence of nonlinear interaction of vector mesons modifies the density dependence of the rho field and influences bulk parameters of neutron stars. The observed quasi-periodic X-ray oscillations of low mass X-ray binaries can be used in order to constrain the equation of state of neutron star matter. Having assumed that the maximum frequency of the quasi periodic oscillations originates at the circular orbit it is possible to estimate masses and radii of neutron stars.

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