Published March 20, 2003 | Version v1
Journal article

Atmospheric neutrino mixing and b-τ unification

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.