Sterile neutrinos for warm dark matter and the reactor anomaly in flavor symmetry models
Creators
- 1. Max-Planck-Institut für Kernphysik, Postfach 103980, 69029 Heidelberg (Germany)
Description
We construct a flavor symmetry model based on the tetrahedral group A4 in which the right-handed neutrinos from the seesaw mechanism can be both keV warm dark matter particles and eV-scale sterile neutrinos. This is achieved by giving the right-handed neutrinos appropriate charges under the same Froggatt-Nielsen symmetry responsible for the hierarchy of the charged lepton masses. We discuss the effect of next-to-leading order corrections to deviate the zeroth order tri-bimaximal mixing. Those corrections have two sources: (i) higher order seesaw terms, which are important when the seesaw particles are eV-scale, and (ii) higher-dimensional effective operators suppressed by additional powers of the cut-off scale of the theory. Whereas the mixing angles of the active neutrinos typically receive corrections of the same order, the mixing of the sterile neutrinos with the active ones is rather stable as it is connected with a hierarchy of mass scales. We also modify an effective A4 model to incorporate keV-scale sterile neutrinos
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2012/01/052Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2012
- Journal Issue
- 01
- Journal Page Range
- p. 052
- ISSN
- 1475-7516
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45101092
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CORRECTIONS; COSMOLOGICAL MODELS; COSMOLOGY; EV RANGE; FLAVOR MODEL; KEV RANGE; NEUTRINOS; NONLUMINOUS MATTER; REST MASS; SYMMETRY; WEINBERG ANGLE
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; LEPTONS; MASS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; QUARK MODEL