Majorana CP violation in approximately μ-τ symmetric models with det (Mv)=0
Description
We discuss effects of Majorana CP violation in a model-independent way for a given phase structure of flavor neutrino masses. To be more predictive, we confine ourselves to models with det(Mv)=0, where Mv is a flavor neutrino mass matrix, and to be consistent with observed results of the neutrino oscillation, the models are subject to an approximate μ-τ symmetry. There are two categories of approximately μ-τ symmetric models classified as (C1) yielding sin2 2θ23 approx. = 1 and sin2 θ13 << 1 and (C2) yielding sin2 2θ23 approx. = 1 and Δ(solar mass)2/|Δmatm2| << 1, were θ23(13) stands for the mixing of massive neutrinos v2 and v3 (v1 and v3) and Δ(solar mass)2 (Δmatm2) stands for the mass squared difference for atmospheric (solar) neutrinos. The Majorana phase can be large for the normal mass hierarchy and for the inverted mass hierarchy with m1 approx. = -m2 only realized in (C1) while they are generically small for the inverted mass hierarchy with m1 approx. = m2 in both (C1) and (C2). These results do not depend on a specific choice of phases in Mv but hold true in any models with det (Mv)=0 because of the rephasing invariance. (author)
Availability note (English)
Available from http://dx.doi.org/10.1143/PTP.123.659Additional details
Identifiers
- DOI
- 10.1143/PTP.123.659;
Publishing Information
- Journal Title
- Progress of Theoretical Physics (Kyoto)
- Journal Volume
- 123
- Journal Issue
- 4
- Journal Page Range
- p. 659-686
- ISSN
- 0033-068X
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 41114814
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CABIBBO ANGLE; CP INVARIANCE; FLAVOR MODEL; KOBAYASHI-MASKAWA MATRIX; MAJORANA THEORY; MASS; MIXING RATIO; NEUTRINO OSCILLATION; PHASE TRANSFORMATIONS; SOLAR NEUTRINOS; SYMMETRY BREAKING
- Descriptors DEC
- COMPOSITE MODELS; DIMENSIONLESS NUMBERS; ELEMENTARY PARTICLES; FERMIONS; INVARIANCE PRINCIPLES; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATRICES; NEUTRINOS; PARTICLE MODELS; QUARK MODEL; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION
Optional Information
- Notes
- 24 refs., 7 figs.