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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 $\delta$...
Autores principales: | , , , |
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Lenguaje: | eng |
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2000
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0370-2693(00)01067-4 http://cds.cern.ch/record/448613 |
_version_ | 1780896041576431616 |
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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. |
id | cern-448613 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2000 |
record_format | invenio |
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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