Gravitational waves from neutron stars described by modern EOS
arXiv:gr-qc/0410140 · doi:10.1063/1.1891555
Abstract
The frequencies and damping times of neutron star (and quark star) oscillations have been computed using the most recent equations of state available in the literature. We find that some of the empirical relations that connect the frequencies and damping times of the modes to the mass and radius of the star, and that were previously derived in the literature need to be modified.
3 pages, 1+1 figures, to appear in the Proceedings of "XVI SIGRAV Conference", Vietri sul Mare (Italy), 13-16 September 2004