Effects of the magnetic fields on the protoneutron star structure

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

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/4178

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0202303
 http://arxiv.org/abs/astro-ph/0202303

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arXiv