Gravitational waves from neutron stars described by modern EOS

Details Gravitational waves from neutron stars described by modern EOS Gravitational waves from neutron stars described by modern EOS

2004-10-28

arxiv.org/abs/gr-qc/0410140v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

3 pages, 1+1 figures, to appear in the Proceedings of "XVI SIGRAV Conference", Vietri sul Mare (Italy), 13-16 September 2004

Scientific paper

10.1063/1.1891555

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.

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