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dc.contributor.author | Esteban Pretel, Andreu | |
dc.contributor.author | Pastor Carpi, Sergio | |
dc.contributor.author | Tomàs, Ricard | |
dc.contributor.author | Raffelt, Georg G. | |
dc.contributor.author | Sigl, Günter | |
dc.date.accessioned | 2014-09-01T12:26:05Z | |
dc.date.available | 2014-09-01T12:26:05Z | |
dc.date.issued | 2007 | |
dc.identifier.citation | Esteban Pretel, Andreu Pastor Carpi, Sergio Tomàs, Ricard Raffelt, Georg G. Sigl, Günter 2007 Decoherence in supernova neutrino transformations suppressed by deleptonization Physical Review D 76 12 125018-1 125018-16 | |
dc.identifier.uri | http://hdl.handle.net/10550/37474 | |
dc.description.abstract | In the dense-neutrino region at 50-400 km above the neutrino sphere in a supernova, neutrino-neutrino interactions cause large flavor transformations. We study when the multi-angle nature of the neutrino trajectories leads to flavor decoherence between different angular modes. We consider a two-flavor mixing scenario between nue and another flavor nux and assume the usual hierarchy F(nue)>F{antinue)>F(nux)=F(antinux) for the number fluxes. We define epsilon=(F(nue)-F(antinue))/(F(antinue)-F(antinux)) as a measure for the deleptonization flux which is the one crucial parameter. The transition between the quasi single-angle behavior and multi-angle decoherence is abrupt as a function of epsilon. For typical choices of other parameters, multi-angle decoherence is suppressed for epsilon>0.3, but a much smaller asymmetry suffices if the neutrino mass hierarchy is normal and the mixing angle small. The critical epsilon depends logarithmically on the neutrino luminosity. In a realistic supernova scenario, the deleptonization flux is probably enough to suppress multi-angle decoherence. | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D, 2007, vol. 76, num. 12, p. 125018-1-125018-16 | |
dc.subject | Física | |
dc.title | Decoherence in supernova neutrino transformations suppressed by deleptonization | |
dc.type | journal article | es_ES |
dc.date.updated | 2014-09-01T12:26:05Z | |
dc.identifier.doi | 10.1103/PhysRevD.76.125018 | |
dc.identifier.idgrec | 041307 | |
dc.rights.accessRights | open access | es_ES |