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Common framework for dark matter, leptogenesis, and neutrino masses

2011/08/31 by François-Xavier Josse-Michaux, Emiliano Molinaro
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Particle physics theoretical and experimental studies #hep-ph

paper · pdf · doi:10.1103/physrevd.84.125021

published as Phys. Rev. D 84, 125021 (2011) · v4: Published version. No changes w.r.t. v3

openalex publication_date 2011/12/14 · arxiv created 2011/12/16 · arxiv updated 2011/12/19 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We study a seesaw-type extension of the standard model in which the symmetry group is enlarged by a global U(1). We introduce adequate scalar and fermion representations which naturally explain the smallness of neutrino masses. With the addition of a viable scalar dark matter candidate, an original scenario of leptogenesis emerges. We solve the relevant set of Boltzmann equations and show how leptogenesis can be successfully implemented at the TeV scale. The constraints on the scalar mass spectrum are derived and the dark matter phenomenology is discussed.

Citations