Effects of the magnetic fields on the protoneutron star structure
classification
🌌 astro-ph
keywords
protoneutronstarmagneticasymmetryeffectsequationfieldnuclear
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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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