Discrimination of Quark Stars from Neutron Stars in Quadrupole Oscillations

Details Discrimination of Quark Stars from Neutron Stars in Quadrupole Oscillations Discrimination of Quark Stars from Neutron Stars in Quadrupole Oscillations

2002-09-17

arxiv.org/abs/astro-ph/0209320v1

Prog.Theor.Phys. 108 (2002) 801-808

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, accepted for publication in Prog. Theor. Phys

Scientific paper

10.1143/PTP.108.801

The frequencies and damping times due to gravitational radiation are calculated for self-bound quark star models. The results are compared with those for neutron star models. They are markedly contrasted in less relativistic cases. The distinction derived here from a simple model of quark stars may be relevant to the future theoretical and observational studies, since the oscillation properties essentially depend on the mass and radius of an equilibrium star.

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