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Supersymmetric majoron signatures and solar neutrino oscillations

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Supersymmetric majoron signatures and solar neutrino oscillations

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dc.contributor.author Santamaria, Arcadi
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2017-07-28T17:48:53Z
dc.date.available 2017-07-28T17:48:53Z
dc.date.issued 1988
dc.identifier.citation Santamaria, Arcadi Furtado Valle, José Wagner 1988 Supersymmetric majoron signatures and solar neutrino oscillations Physical Review Letters 60 5 397 400
dc.identifier.uri http://hdl.handle.net/10550/60447
dc.description.abstract Spontaneous R-parity breaking in supergravity solves the solar neutrino problem through matter-enhanced neutrino oscillations. The model may be tested in collider experiments and through ''dynamical'' effects associated with the existence of a weakly interacting majoron. Apart from astrophysical effects, majoron emission can produce observable changes in μ and τ decay spectra for parameter values that substantially reduce the solar neutrino flux. A signature of the model is the possible observation of the decay μ→e+majoron.
dc.language.iso eng
dc.relation.ispartof Physical Review Letters, 1988, vol. 60, num. 5, p. 397-400
dc.subject Partícules (Física nuclear)
dc.title Supersymmetric majoron signatures and solar neutrino oscillations
dc.type journal article es_ES
dc.date.updated 2017-07-28T17:48:54Z
dc.identifier.doi 10.1103/PhysRevLett.60.397
dc.identifier.idgrec 073609
dc.rights.accessRights open access es_ES

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