Stability of strange stars (SS) under radial oscillation
Astrophysics
2007-05-23 v2
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0503378,
title = {Stability of strange stars (SS) under radial oscillation},
author = {Monika Sinha and Jishnu Dey and Mira Dey and Subharthi Ray and Siddhartha Bhowmick},
journal= {arXiv preprint arXiv:astro-ph/0503378},
year = {2007}
}
Comments
5 pages, 1 figure, submitted for the proceedings of 22nd Texas Symposium on Relativistic Astrophysics held at Stanford University, 13th-17th December, 2004