Affordable Access

deepdyve-link deepdyve-link
Publisher Website

Neutrino Textures in the Light of Super-Kamiokande Data and a Realistic String Model

Authors
  • Ellis, J.
  • Leontaris, G. K.
  • Lola, S.
  • Nanopoulos, D. V.
Type
Published Article
Publication Date
Aug 06, 1998
Submission Date
Aug 06, 1998
Identifiers
DOI: 10.1007/s100529900001
arXiv ID: hep-ph/9808251
Source
arXiv
License
Unknown
External links

Abstract

Motivated by the Super-Kamiokande atmospheric neutrino data, we discuss possible textures for Majorana and Dirac neutrino masses within the see-saw framework. The main purposes of this paper are twofold: first to obtain intuition from a purely phenomenological analysis, and secondly to explore to what extent it may be realized in a specific model. We comment initially on the simplified two-generation case, emphasizing that large mixing is not incompatible with a large hierarchy of mass eigenvalues. We also emphasize that renormalization-group effects may amplify neutrino mixing, presenting semi-analytic expressions for estimating this amplification. Several examples are then given of three-family neutrino mass textures which may also accommodate the persistent solar neutrino deficit, with different assumptions for the neutrino Dirac mass matrices. We comment on a few features of neutrino mass textures arising in models with a U(1) flavour symmetry. Finally, we discuss the possible pattern of neutrino masses in a `realistic' flipped SU(5) model derived from string theory, illustrating how a desirable pattern of mixing may emerge. Both small- or large-angle MSW solutions are possible, whilst a hierarchy of neutrino masses appears more natural than near-degeneracy. This model contains some unanticipated features that may also be relevant in other models: the neutrino Dirac matrices may not be related closely to the quark mass matrices, and the heavy Majorana states may include extra gauge-singlet fields.

Report this publication

Statistics

Seen <100 times