Neutron star matter equation of state and gravitational wave emission

Details Neutron star matter equation of state and gravitational wave emission Neutron star matter equation of state and gravitational wave emission

2005-07-21

arxiv.org/abs/astro-ph/0507497v1

Mod.Phys.Lett.A20:2335-2350,2005

Astronomy and Astrophysics

Astrophysics

15 pages, 8 figures. To be published as a Brief Review in Modern Physics Letters A

Scientific paper

10.1142/S0217732305018335

The EOS of strongly interacting matter at densities ten to fifteen orders of magnitude larger than the typical density of terrestrial macroscopic objects determines a number of neutron star properties, including the pattern of gravitational waves emitted following the excitation of nonradial oscillation modes. This paper reviews some of the approaches employed to model neutron star matter, as well as the prospects for obtaining new insights from the experimental study of gravitational waves emitted by neutron stars.

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