Study of Proto Strange Stars (PSS) in Temperature and Density Dependent Quark Mass Model

Details Study of Proto Strange Stars (PSS) in Temperature and Density Dependent Quark Mass Model Study of Proto Strange Stars (PSS) in Temperature and Density Dependent Quark Mass Model

2002-06-07

arxiv.org/abs/astro-ph/0206111v1

Int.J.Mod.Phys. D12 (2003) 583-595

Astronomy and Astrophysics

Astrophysics

LaTex2e file with four postscript figures

Scientific paper

10.1142/S0218271803003256

We report on the study of the mass-radius (M-R) relation and the radial oscillations of proto strange stars. For the quark matter we have employed the well known density dependent quark mass model and its very recent modification, the temperature and density dependent quark mass model. We find that the maximum mass the star can support increases significantly with the temperature of the star in this model which implies that transition to a black hole at the early stage of formation of the star is inhibited. As for the neutrinos, we find, contrary to the expectation that the M-R and oscillation frequencies are almost independent of the neutrino chemical potentials.

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