English

Scalar Multiplet Dark Matter

High Energy Physics - Phenomenology 2010-12-15 v1 Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena

Abstract

We perform a systematic study of the phenomenology associated to models where the dark matter consists in the neutral component of a scalar SU(2)_L n-uplet, up to n=7. If one includes only the pure gauge induced annihilation cross-sections it is known that such particles provide good dark matter candidates, leading to the observed dark matter relic abundance for a particular value of their mass around the TeV scale. We show that these values actually become ranges of values -which we determine- if one takes into account the annihilations induced by the various scalar couplings appearing in these models. This leads to predictions for both direct and indirect detection signatures as a function of the dark matter mass within these ranges. Both can be largely enhanced by the quartic coupling contributions. We also explain how, if one adds right-handed neutrinos to the scalar doublet case, the results of this analysis allow to have altogether a viable dark matter candidate, successful generation of neutrino masses, and leptogenesis in a particularly minimal way with all new physics at the TeV scale.

Keywords

Cite

@article{arxiv.0903.4010,
  title  = {Scalar Multiplet Dark Matter},
  author = {T. Hambye and F. -S. Ling and L. Lopez Honorez and J. Rocher},
  journal= {arXiv preprint arXiv:0903.4010},
  year   = {2010}
}

Comments

43 pages, 20 figures

R2 v1 2026-06-21T12:43:39.660Z