Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-02-15
Astronomy and Astrophysics
Astrophysics
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.
Bednarek Ilona
Brzezina A.
Mańka Ryszard
Zastawny-Kubica M.
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