1999
DOI: 10.1088/1126-6708/1999/05/023
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Neutrino masses and mixing with non-anomalous abelian flavor symmetries

Abstract: The experimental data on atmospheric and solar neutrinos are used to test the framework of non-anomalous Abelian horizontal gauge symmetries with only three light active neutrinos.We assume that the hierarchy in mass-squared splittings is not accidental and that the small breaking parameters are not considerably larger than 0.2. We find that the small angle MSW solution of the solar neutrino problem can only be accommodated if the ν µ −ν τ mass hierarchy depends on the charges of at least three sterile neutrin… Show more

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Cited by 25 publications
(11 citation statements)
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“…Equal VEVs S L = SL would be necessary to preserve supersymmetry with a gauged, non-anomalous U (1) L . Similarly, two spurions of equal VEVs and opposite U (1) H charges would be necessary if U (1) H is a gauged, non-anomalous symmetry [9]. Neither ingredient is important for our purposes.…”
mentioning
confidence: 99%
“…Equal VEVs S L = SL would be necessary to preserve supersymmetry with a gauged, non-anomalous U (1) L . Similarly, two spurions of equal VEVs and opposite U (1) H charges would be necessary if U (1) H is a gauged, non-anomalous symmetry [9]. Neither ingredient is important for our purposes.…”
mentioning
confidence: 99%
“…In Ref. [16] it was argued, however, that in Abelian flavor models that satisfy both (1.1) and (1.2), the pseudo-Dirac structure cannot apply to the 23 subspace. It can only be relevant then to the 12 subspace, corresponding to either the MSW(LA) or the VO solution of the SN problem.…”
Section: Pseudo-dirac Neutrinosmentioning
confidence: 99%
“…(In Ref. [16], these models are called (2,0) models, where the first integer refers to the number of active neutrinos, and the second to the number of sterile.) In such models, the selection rules apply directly to the Majorana mass matrix of the active neutrinos, and it is easy to see that the neutrino mass matrix cannot give both large mixing and hierarchically separated masses: Large 23 mixing would require (M ν ) 23 ∼ (M ν ) 33 .…”
Section: Avoidingmentioning
confidence: 99%
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