Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-12
Int.J.Mod.Phys. D11 (2002) 545-560
Astronomy and Astrophysics
Astrophysics
LaTex2e file with four postscript figures
Scientific paper
10.1142/S0218271802001731
We have studied phase transition from hadron matter to quark matter in the presence of high magnetic fields incorporating the trapped electron neutrinos at finite temperatures. We have used the density dependent quark mass (DDQM) model for the quark phase while the hadron phase is treated in the frame-work of relativistic mean field theory. It is seen that the nuclear energy at phase transition decreases with both magnetic field and temperature. A brief discussion of the effect of magnetic field in supernova explosions and proto-neutron star evolution is given.
Anand J. D.
Gupta Asha
Gupta Vijay K.
Singh Sumeetpal S.
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