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Fitting Simpson's neutrino into the standard model

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Fitting Simpson's neutrino into the standard model

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dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-24T10:25:35Z
dc.date.available 2015-09-24T10:25:35Z
dc.date.issued 1985
dc.identifier.citation Furtado Valle, José Wagner 1985 Fitting Simpson's neutrino into the standard model Physics Letters B 159 1 49 56
dc.identifier.uri http://hdl.handle.net/10550/47209
dc.description.abstract I show how to accomodate the 17 keV state recently reported by Simpson as one of the neutrinos of the standard model. Experimental constraints can only be satisfied if the μ and τ neutrino combine to a very good approximation to form a Dirac neutrino of 17 keV leaving a light νe. Neutrino oscillations will provide the most stringent test of the model. The cosmological bounds are also satisfied in a natural way in models with Goldstone bosons. Explicit examples are given in the framework of majoron-type models. Constraints on the lepton symmetry breaking scale which follow from astrophysics, cosmology and laboratory experiments are discussed.
dc.language.iso eng
dc.relation.ispartof Physics Letters B, 1985, vol. 159, num. 1, p. 49-56
dc.subject Física
dc.title Fitting Simpson's neutrino into the standard model
dc.type journal article es_ES
dc.date.updated 2015-09-24T10:25:36Z
dc.identifier.doi 10.1016/0370-2693(85)90118-2
dc.identifier.idgrec 073621
dc.rights.accessRights open access es_ES

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