Effects of the magnetic fields on the protoneutron star structure

Astronomy and Astrophysics – Astrophysics

Scientific paper

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7 pages, latex2e, 3 figures, submitted to J. Phys. G: Nucl. Phys

Scientific paper

The equation of state of a protoneutron star matter including the effects of
magnetic field, temperature, nuclear asymmetry and trapped neutrinos are
studied. Using the Oppenheimer-Volkoff-Tolman equation global parameters of the
protoneutron star are obtained. Presence of the nuclear asymmetry and magnetic
field make the protoneutron star more compact.

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