Published June 20, 2003 | Version v1
Journal article

Neutrino mass matrix and hierarchy

  • 1. California Institute of Technology, Pasadena, CA 91125 (United States)
  • 2. Physics Department, University of California, Riverside, CA 92521 (United States)

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 4 x 10-3eV if s13 = 0 and 6 x 10-3eV 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

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
672
Journal Issue
1
Journal Page Range
p. 117-125
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
31. Coral Gables conference on high energy physics and cosmology
Dates
11-14 Dec 2002
Place
Fort Lauderdale, FL (United States)

Optional Information

Notes
(c) 2003 American Institute of Physics