Published March 20, 2003
| Version v1
Journal article
Atmospheric neutrino mixing and b-τ unification
Creators
Description
Extrapolating the τ and b masses in the MSSM tends to give for their ratio at the GUT scale a number around 1.2, for most viable values tanβ, rather than the minimal SU(5) prediction of 1. We suggest that this may be due to large off-diagonal elements in the charged lepton mass matrix ML that can also explain the large atmospheric neutrino mixing angle. Several simple models with definite predictions for mτ/mb(MGUT) are presented
Additional details
Identifiers
- DOI
- 10.1016/S0370-2693;
- PII
- S0370269303001321;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 556
- Journal Issue
- 3-4
- Journal Page Range
- p. 185-191
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37074908
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- FORECASTING; MASS; NEUTRINOS; SU-5 GROUPS; WEINBERG ANGLE
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; LEPTONS; LIE GROUPS; MASSLESS PARTICLES; SU GROUPS; SYMMETRY GROUPS
Optional Information
- Copyright
- Copyright (c) 2003 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.