Imprint of the Seesaw Mechanism on Feebly Interacting Dark Matter and the Baryon Asymmetry.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
03 Dec 2021
Historique:
received: 13 04 2021
revised: 24 09 2021
accepted: 25 10 2021
entrez: 22 12 2021
pubmed: 23 12 2021
medline: 23 12 2021
Statut: ppublish

Résumé

We show that the type-I seesaw, responsible for generating the light neutrino mass, itself is capable of accommodating one of the three right handed neutrinos as a freeze-in type of dark matter where the required smallness of the associated coupling is connected to the lightness of the (smallest) active neutrino mass. It turns out that (a) the nonthermal production of dark matter having mass ≲O(1)  MeV (via decays of W, Z bosons and standard model Higgs) consistent with relic density and (b) its stability determine this smallest active neutrino mass uniquely ∼O(10^{-12})  eV. On the other hand, the study of flavor leptogenesis in this scenario (taking into account the latest neutrino data and Higgs vacuum stability issue) fixes the scale of two other right handed neutrinos.

Identifiants

pubmed: 34936780
doi: 10.1103/PhysRevLett.127.231801
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

231801

Auteurs

Arghyajit Datta (A)

Department of Physics, Indian Institute of Technology Guwahati, Assam-781039, India.

Rishav Roshan (R)

Department of Physics, Indian Institute of Technology Guwahati, Assam-781039, India.

Arunansu Sil (A)

Department of Physics, Indian Institute of Technology Guwahati, Assam-781039, India.

Classifications MeSH