Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-06-07
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.
Anand J. D.
Gupta Asha
Gupta Vijay K.
Singh Sumeetpal S.
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