Quark matter imprint on Gravitational Waves from oscillating stars

Details Quark matter imprint on Gravitational Waves from oscillating stars Quark matter imprint on Gravitational Waves from oscillating stars

2006-03-17

arxiv.org/abs/astro-ph/0603464v2

Gen.Rel.Grav.39:1323,2007

Astronomy and Astrophysics

Astrophysics

Eight pages, four figures. Revised version, to appear on General Relativity and Gravitation

Scientific paper

10.1007/s10714-007-0444-0

We discuss the possibility that the detection of gravitational waves emitted by compact stars may allow to constrain the MIT bag model of quark matter equation of state. Our results show that the combined knowledge of the frequency of the emitted gravitational wave and of the mass, or the radiation radius, of the source allows one to discriminate between strange stars and neutron stars and set stringent bounds on the bag constants.

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