Stability of strange stars (SS) under radial oscillation

Details Stability of strange stars (SS) under radial oscillation Stability of strange stars (SS) under radial oscillation

2005-03-17

arxiv.org/abs/astro-ph/0503378v2

Astronomy and Astrophysics

Astrophysics

5 pages, 1 figure, submitted for the proceedings of 22nd Texas Symposium on Relativistic Astrophysics held at Stanford Univers

Scientific paper

A realistic Equation of State (EOS) leads to strange stars (ReSS) which are
compact in the mass radius plot, close to the Schwarzchild limiting line (Dey
et al. 1998). We carry out a stability analysis under radial oscillations and
compare with the EOS of other SS models. We find that the ReSS is stable and an
M-R region can be identified to that effect.

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