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Neutrino conversions in a polarized medium

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Neutrino conversions in a polarized medium

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dc.contributor.author Nunokawa, Hiroshi
dc.contributor.author Semikoz, Victor B.
dc.contributor.author Smirnov, Alexei Yu
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-28T07:54:56Z
dc.date.available 2015-09-28T07:54:56Z
dc.date.issued 1997
dc.identifier.citation Nunokawa, Hiroshi Semikoz, Victor B. Smirnov, Alexei Yu Furtado Valle, José Wagner 1997 Neutrino conversions in a polarized medium Nuclear Physics B 501 1 17 40
dc.identifier.uri http://hdl.handle.net/10550/47306
dc.description.abstract Electron polarization induced by magnetic fields can modify the potentials relevant for describing neutrino conversions in media with magnetic fields. The magnitudes of polarization potentials are determined for different conditions. We show that variations of the electron polarization along the neutrino trajectory can induce resonant conversions in the active-sterile neutrino system, but cannot lead to level crossing in the active-active neutrino system. For neutrino flavour conversions the polarisation leads only to a shift of the standard MSW resonance. For polarizations $\lambda \lsim 0.04$ the direct modifications of the potential (density) due to the magnetic field pressure are smaller than the modifications due to the polarization effect. We estimate that indeed the typical magnitude of the polarization in the sun or in a supernova are not expected to exceed 10−2. However even such a small polarization may lead to interesting consequences for supernova physics and for properties of neutrino signals from collapsing stars.
dc.language.iso eng
dc.relation.ispartof Nuclear Physics B, 1997, vol. 501, num. 1, p. 17-40
dc.subject Física
dc.title Neutrino conversions in a polarized medium
dc.type journal article es_ES
dc.date.updated 2015-09-28T07:54:56Z
dc.identifier.doi 10.1016/S0550-3213(97)00366-0
dc.identifier.idgrec 073547
dc.rights.accessRights open access es_ES

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