WIMP dark matter as radiative neutrino mass messenger
Abstract
The minimal seesaw extension of the Standard SU(3) x SU(2) x U(1) Model requires two electroweak singlet fermions in order to accommodate the neutrino oscillation parameters at tree level. Here we consider a next to minimal extension where light neutrino masses are generated radiatively by two electroweak fermions: one singlet and one triplet under SU(2). These should be odd under a parity symmetry and their mixing gives rise to a stable weakly interactive massive particle (WIMP) dark matter candidate. For mass in the GeV-TeV range, it reproduces the correct relic density, and provides an observable signal in nuclear recoil direct detection experiments. The fermion triplet component of the dark matter has gauge interactions, making it also detectable at present and near future collider experiments.
Keywords
Cite
@article{arxiv.1307.8134,
title = {WIMP dark matter as radiative neutrino mass messenger},
author = {M. Hirsch and R. A. Lineros and S. Morisi and J. Palacio and N. Rojas and J. W. F. Valle},
journal= {arXiv preprint arXiv:1307.8134},
year = {2013}
}
Comments
18 pages, 6 figures. Published version in JHEP