2020/09/30 by T. Hashimoto, Tsuyoshi Hashimoto, Daijiro Suematsu
Physics and Astronomy · #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Inflation (cosmology) #Inflaton #Leptogenesis #Lepton #Neutrino #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Phenomenology (philosophy) #Philosophy #Physics #Scalar (mathematics) #Singlet state #Theoretical physics #hep-ph
paper · pdf · doi:10.1103/physrevd.102.115041
published as Phys. Rev. D 102, 115041 (2020) · 31 pages, 6 figures, 2 tables, added some comments and references, published version
openalex created_date 2020/10/01 · openalex publication_date 2020/12/31 · arxiv created 2021/01/23 · arxiv updated 2021/01/26 · openalex updated_date 2026/08/05
We study an extension of the scotogenic model with a real singlet scalar. It gives an origin of the mass of right-handed neutrinos and plays a role of inflaton through a nonminimal coupling with Ricci scalar. While an inert doublet scalar is an indispensable ingredient for neutrino mass generation in the model, it is also a promising dark matter (DM) candidate. Introduction of the singlet scalar could affect its nature of DM if mass of the singlet scalar is in a resonance region. We focus our study on such a case where inflaton mass is expected to be in a TeV range and reheating temperature is less than 109 GeV. Thus the model requires low scale leptogenesis. After examining several effects brought about by the singlet scalar for the DM sector, we discuss DM phenomenology such as high energy neutrinos and monochromatic gammas caused by its annihilation.