A TeV scale model for neutrino mass, dark matter and baryon asymmetry
High Energy Physics - Phenomenology
2009-05-26 v1
Abstract
We discuss a TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos with imposed an exact symmetry. Tiny neutrino masses are generated at the three loop level, a singlet scalar field is a candidate of dark matter, and a strong first order phase transition is realized for successful electroweak baryogenesis. The model provides various discriminative predictions, so that it is testable at the current and future experiments.
Keywords
Cite
@article{arxiv.0905.3958,
title = {A TeV scale model for neutrino mass, dark matter and baryon asymmetry},
author = {Mayumi Aoki and Shinya Kanemura and Osamu Seto},
journal= {arXiv preprint arXiv:0905.3958},
year = {2009}
}
Comments
4 pages. 3 figures, talk at Rencontres de Moriond 2009, QCD and High Energy Interaction, March 14 - 21 (2009), Le Thuile, Italy