Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4347
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dc.contributor.authorde Sabbata, V-
dc.contributor.authorSivaram, C-
dc.date.accessioned2009-02-06T11:28:33Z-
dc.date.available2009-02-06T11:28:33Z-
dc.date.issued1990-
dc.identifier.citationProceedings of the 21st International Cosmic Ray Conference. Vol. 10 (HE Sessions), pp. 51 - 53en
dc.identifier.urihttp://hdl.handle.net/2248/4347-
dc.description.abstractIf neutrinos couple to torsion in the frame work of the Einstein-Cartan theory, with a strength about that of the weak interaction, then the spin-torsion interaction can induce an effective neutrino magnetic moment. We explore the emission and propagation of neutrinos in a hot dense medium of neutron matter in the presence of large magnetic fields. These effects could be significant for neutrino production in dense collapsing cores.en
dc.language.isoenen
dc.publisherInternational Cosmic Rayen
dc.relation.ispartofseriesInternational Cosmic Ray Conference, Vol. 10-
dc.relation.urihttp://adsabs.harvard.edu/abs/1990ICRC...10...51Den
dc.subjectNeutrino Magnetic Momenten
dc.subjectTorsionen
dc.subjectSupernova Neutrinosen
dc.titleNeutrino magnetic moment induced by torsion and consequences for supernova neutrinosen
dc.typeArticleen
Appears in Collections:IIAP Publications

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