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Mass varying neutrinos in the Sun

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Mass varying neutrinos in the Sun

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dc.contributor.author Cirelli, Marco
dc.contributor.author González García, Mª Concepción
dc.contributor.author Peña Garay, Carlos
dc.date.accessioned 2014-11-03T11:23:11Z
dc.date.available 2014-11-03T11:23:11Z
dc.date.issued 2005
dc.identifier.citation Cirelli, Marco González García, Mª Concepción Peña Garay, Carlos 2005 Mass varying neutrinos in the Sun Nuclear Physics B 719 1-2 219 233
dc.identifier.uri http://hdl.handle.net/10550/39533
dc.description.abstract In this work we study the phenomenological consequences of the dependence of mass varying neutrinos on the neutrino density in the Sun, which we precisely compute in each point along the neutrino trajectory. We find that a generic characteristic of these scenarios is that they establish a connection between the effective Delta m(2) in the Sun and the absolute neutrino mass scale. This does not lead to any new allowed region in the oscillation parameter space. On the contrary, due to this effect, the description of solar neutrino data worsens for large absolute mass. As a consequence a lower bound on the level of degeneracy can be derived from the combined analysis of the solar and KamLAND data. In particular this implies that the analysis favours normal over inverted mass orderings. These results, in combination with a positive independent determination of the absolute neutrino mass, can be used as a test of these scenarios together with a precise determination of the energy dependence of the survival probability of solar neutrinos, in particular for low energies.
dc.language.iso eng
dc.relation.ispartof Nuclear Physics B, 2005, vol. 719, num. 1-2, p. 219-233
dc.subject Física
dc.title Mass varying neutrinos in the Sun
dc.type journal article es_ES
dc.date.updated 2014-11-03T11:23:11Z
dc.identifier.doi 10.1016/j.nuclphysb.2005.04.034
dc.identifier.idgrec 097444
dc.rights.accessRights open access es_ES

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