Effects of the magnetic fields on the protoneutron star structure

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dc.creatorManka, R.
dc.creatorZastawny-Kubica, M.
dc.creatorBrzezina, A.
dc.creatorBednarek, I.
dc.date2002-02-15
dc.date.accessioned2026-07-07T02:02:49Z
dc.date.available2026-07-07T02:02:49Z
dc.descriptionThe 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.
dc.description7 pages, latex2e, 3 figures, submitted to J. Phys. G: Nucl. Phys
dc.identifierhttps://arxiv.org/abs/astro-ph/0202303
dc.identifierhttp://arxiv.org/abs/astro-ph/0202303
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4178
dc.subjectAstrophysics
dc.titleEffects of the magnetic fields on the protoneutron star structure
dc.typetext

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