Effects of the magnetic fields on the protoneutron star structure

2002/02/15 by R. Manka, M. Zastawny-Kubica, Manka, R. +5
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0202303

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

arxiv created 2002/02/15 · arxiv updated 2009/12/01

Abstract

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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