Published February 5, 2004 | Version v1
Journal article

Neutrino masses, mixing and hierarchy

Description

We build a model to describe neutrinos based on strict hierarchy, incorporating as much as possible, the latest known data, for Δsol and Δatm, and for the mixing angles determined from neutrino oscillation experiments, including that from KamLAND. Since the hierarchy assumption is a statement about mass ratios, it lets us obtain all three neutrino masses. We obtain a mass matrix, Mν and a mixing matrix, U, where both Mν and U are given in terms of powers of Λ, the analog of the Cabibbo angle λ in the Wolfenstein representation, and two parameters, ρ and κ, each of order one. The expansion parameter, Λ, is defined by Λ2=m2/m3=√(Δsol/Δatm)∼0.16, and ρ expresses our ignorance of the lightest neutrino mass m1, (m1=ρΛ4m3), while κ scales s13 to the experimental upper limit, s13=κΛ2∼0.16κ. These matrices are similar in structure to those for the quark and lepton families, but with Λ about 1.6 times larger than the λ for the quarks and charged leptons. The upper limit for the effective neutrino mass in double β-decay experiments is 4x10-3 eV if s13=0 and 6x10-3 eV if s13 is maximal. The model, which is fairly unique, given the hierarchy assumption and the data, is compared to supersymmetric extension and texture zero models of mass generation

Additional details

Identifiers

DOI
10.1016/j.physletb.2003.06.068;
PII
S0370269303018537;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
580
Journal Issue
3-4
Journal Page Range
p. 236-242
ISSN
0370-2693
CODEN
PYLBAJ

INIS

Country of Publication
Netherlands
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
37108769
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
CABIBBO ANGLE; DOUBLE BETA DECAY; MASS; MATRICES; MILLI EV RANGE; NEUTRINO OSCILLATION; NEUTRINOS; QUARKS; SUPERSYMMETRY; WEINBERG ANGLE
Descriptors DEC
BETA DECAY; BETA-MINUS DECAY; DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; LEPTONS; MASSLESS PARTICLES; NUCLEAR DECAY; SYMMETRY

Optional Information

Copyright
Copyright (c) 2003 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.