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Low-energy anti-neutrinos from the Sun

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Low-energy anti-neutrinos from the Sun

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dc.contributor.author Pastor Carpi, Sergio
dc.contributor.author Semikoz, Victor B.
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-28T08:00:24Z
dc.date.available 2015-09-28T08:00:24Z
dc.date.issued 1998
dc.identifier.citation Pastor Carpi, Sergio Semikoz, Victor B. Furtado Valle, José Wagner 1998 Low-energy anti-neutrinos from the Sun Physics Letters B 423 1-2 118 125
dc.identifier.uri http://hdl.handle.net/10550/47310
dc.description.abstract We consider the sensitivity of future neutrino experiments in the low energy region, such as BOREXINO or HELLAZ, to a solar electron antineutrino signal. We show that, if neutrino conversions within the Sun result in partial polarization of initial solar neutrino fluxes, then a new opportunity arises to observe the electron antineutrinos and thus to probe the Majorana nature of the neutrinos. This is achieved by comparing the slopes of the energy dependence of the differential neutrino electron scattering cross section for different neutrino conversion scenarios. We also show how the \nu_e -> \bar{\nu}_e conversions may take place for low energy solar neutrinos while being unobservable at the Kamiokande and Super-Kamiokande experiments.
dc.language.iso eng
dc.relation.ispartof Physics Letters B, 1998, vol. 423, num. 1-2, p. 118-125
dc.subject Física
dc.title Low-energy anti-neutrinos from the Sun
dc.type journal article es_ES
dc.date.updated 2015-09-28T08:00:24Z
dc.identifier.doi 10.1016/S0370-2693(98)00122-1
dc.identifier.idgrec 073533
dc.rights.accessRights open access es_ES

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