Stability of strange stars (SS) under radial oscillation

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dc.creatorSinha, Monika
dc.creatorDey, Jishnu
dc.creatorDey, Mira
dc.creatorRay, Subharthi
dc.creatorBhowmick, Siddhartha
dc.date2005-03-17
dc.date2005-03-21
dc.date.accessioned2026-07-07T02:17:15Z
dc.date.available2026-07-07T02:17:15Z
dc.descriptionA 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.
dc.description5 pages, 1 figure, submitted for the proceedings of 22nd Texas Symposium on Relativistic Astrophysics held at Stanford University, 13th-17th December, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0503378
dc.identifierhttp://arxiv.org/abs/astro-ph/0503378
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9103
dc.subjectAstrophysics
dc.titleStability of strange stars (SS) under radial oscillation
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