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Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework

We study extensions of supersymmetric models without R-parity which include an anomalous U(1)_H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level of approximately $(\theta^2)^\delta$ eV where $\theta\approx 0.22$ is the U(1)_H breaking parameter and $\delta$...

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Autores principales: Mira, J.M., Nardi, E., Restrepo, D.A., Valle, J.W.F.
Lenguaje:eng
Publicado: 2000
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(00)01067-4
http://cds.cern.ch/record/448613
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author Mira, J.M.
Nardi, E.
Restrepo, D.A.
Valle, J.W.F.
author_facet Mira, J.M.
Nardi, E.
Restrepo, D.A.
Valle, J.W.F.
author_sort Mira, J.M.
collection CERN
description We study extensions of supersymmetric models without R-parity which include an anomalous U(1)_H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level of approximately $(\theta^2)^\delta$ eV where $\theta\approx 0.22$ is the U(1)_H breaking parameter and $\delta$ is an integer number that depends on the horizontal charges of the leptons. For $\delta=1$ a unique self-consistent model arises in which i) all the superpotential trilinear R-parity violating couplings are forbidden by holomorphy; ii) the tree level neutrino mass falls in the range suggested by the atmospheric neutrino problem; iii) radiative contributions to neutrino masses are strongly suppressed resulting in a squared solar mass difference of few 10^{-8} eV^2 which only allows for the LOW (or quasi-vacuum) solution to the solar neutrino problem; iv) the neutrino mixing angles are not suppressed by powers of $\theta$ and can naturally be large.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
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spelling cern-4486132023-03-14T20:02:15Zdoi:10.1016/S0370-2693(00)01067-4http://cds.cern.ch/record/448613engMira, J.M.Nardi, E.Restrepo, D.A.Valle, J.W.F.Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent FrameworkParticle Physics - PhenomenologyWe study extensions of supersymmetric models without R-parity which include an anomalous U(1)_H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level of approximately $(\theta^2)^\delta$ eV where $\theta\approx 0.22$ is the U(1)_H breaking parameter and $\delta$ is an integer number that depends on the horizontal charges of the leptons. For $\delta=1$ a unique self-consistent model arises in which i) all the superpotential trilinear R-parity violating couplings are forbidden by holomorphy; ii) the tree level neutrino mass falls in the range suggested by the atmospheric neutrino problem; iii) radiative contributions to neutrino masses are strongly suppressed resulting in a squared solar mass difference of few 10^{-8} eV^2 which only allows for the LOW (or quasi-vacuum) solution to the solar neutrino problem; iv) the neutrino mixing angles are not suppressed by powers of $\theta$ and can naturally be large.We study extensions of supersymmetric models without R-parity which include an anomalous U(1)_H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level of approximately $(\theta^2)^\delta$ eV where $\theta\approx 0.22$ is the U(1)_H breaking parameter and $\delta$ is an integer number that depends on the horizontal charges of the leptons. For $\delta=1$ a unique self-consistent model arises in which i) all the superpotential trilinear R-parity violating couplings are forbidden by holomorphy; ii) the tree level neutrino mass falls in the range suggested by the atmospheric neutrino problem; iii) radiative contributions to neutrino masses are strongly suppressed resulting in a squared solar mass difference of few 10^{-8} eV^2 which only allows for the LOW (or quasi-vacuum) solution to the solar neutrino problem; iv) the neutrino mixing angles are not suppressed by powers of $\theta$ and can naturally be large.We study extensions of supersymmetric models without R-parity which include an anomalous U (1) H horizontal symmetry. Bilinear R-parity violating terms induce a neutrino mass at tree level m ν tree ≈( θ 2 ) δ  eV where θ ≃0.22 is the U (1) H breaking parameter and δ is an integer number that depends on the horizontal charges of the leptons. For δ =1 a unique self-consistent model arises in which (i) all the superpotential trilinear R-parity violating couplings are forbidden by holomorphy; (ii) m ν tree falls in the range suggested by the atmospheric neutrino problem; (iii) radiative contributions to neutrino masses are strongly suppressed resulting in Δm 2 solar ≈ few 10 −8  eV 2 which only allows for the LOW (or quasi-vacuum) solution to the solar neutrino problem; (iv) the neutrino mixing angles are not suppressed by powers of θ and can naturally be large.hep-ph/0007266CERN-TH-2000-218IFIC-00-46UDEA-PE-00-04CERN-TH-2000-218IFIC-2000-46UDEA-PE-2000-04oai:cds.cern.ch:4486132000-07-24
spellingShingle Particle Physics - Phenomenology
Mira, J.M.
Nardi, E.
Restrepo, D.A.
Valle, J.W.F.
Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title_full Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title_fullStr Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title_full_unstemmed Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title_short Bilinear R-parity Violation and Small Neutrino Masses: a Self-consistent Framework
title_sort bilinear r-parity violation and small neutrino masses: a self-consistent framework
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/S0370-2693(00)01067-4
http://cds.cern.ch/record/448613
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