Neutrino scattering off spin-polarized particles in supernovae

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dc.creatorMorley, P. D.
dc.creatorDib, C.
dc.creatorSchmidt, I.
dc.date1999-03-11
dc.date.accessioned2026-07-07T02:30:49Z
dc.date.available2026-07-07T02:30:49Z
dc.descriptionWe calculate neutrino and antineutrino scattering off electrons and nucleons in supernovae using a detailed Monte Carlo transport code incorporating realistic equations of state. The goal is to determine whether particles in a neutron star core, partially spin-aligned by the local magnetic field, can give rise to asymmetric neutrino emission via the standard parity breaking weak force. We conclude that electron scattering in a very high magnetic field does indeed give a net asymmetry, but that nucleon scattering, if present, removes the asymmetry.
dc.description11 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/9903186
dc.identifierhttp://arxiv.org/abs/astro-ph/9903186
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13944
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrino scattering off spin-polarized particles in supernovae
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