1212.2369 (M. Bejger)

Parameters of rotating neutron stars with and without hyperons    [PDF]

M. Bejger

The discovery of a 2 Msun neutron star provided a robust constraint for the theory of exotic dense matter, questioning the existence of strange baryons in the interiors of neutron stars. With many theories failing to reproduce this observational result, several equations of state containing hyperons are consistent with it. We study global properties of stars using equations of state containing hyperons, and compare them to those without hyperons in order to find similarities, differences and limits that can be compared with the astrophysical observations. Rotating, axisymmetric and stationary stellar configurations in General Relativity are obtained, and their global parameters are studied. Approximate formulae describing the behavior of the maximum and minimum stellar mass, compactness, surface redshifts and moments of inertia as functions of spin frequency are provided. We also study the thin disk accretion and compare the spin-up evolution of stars with different moments of inertia.

View original: http://arxiv.org/abs/1212.2369