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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

A model for mixed warm and hot right-handed neutrino dark matter

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Author(s):
Dutra, Maira [1] ; Oliveira, Vinicius [2] ; Pires, C. A. de S. [2] ; Queiroz, Farinaldo S. [3, 4]
Total Authors: 4
Affiliation:
[1] Carleton Univ, Ottawa Carleton Inst Phys, 1125 Colonel By Dr, Ottawa, ON K1S 5B6 - Canada
[2] Univ Fed Paraiba, Dept Fis, Caixa Postal 5008, BR-58051970 Joao Pessoa, Paraiba - Brazil
[3] Univ Fed Rio Grande do Norte, Int Inst Phys, Campus Univ, BR-59078970 Natal, RN - Brazil
[4] Univ Fed Rio Grande do Norte, Dept Fis, BR-59078970 Natal, RN - Brazil
Total Affiliations: 4
Document type: Journal article
Source: Journal of High Energy Physics; n. 10 OCT 1 2021.
Web of Science Citations: 0
Abstract

We discuss a model where a mixed warm and hot keV neutrino dark matter rises naturally. We arrange active and sterile neutrinos in the same SU(3)(L) multiplet, with the lightest sterile neutrino being dark matter. The other two heavy sterile neutrinos, through their out-of-equilibrium decay, contribute both to the dilution of dark matter density and its population, after freeze-out. We show that this model features all ingredients to overcome the overproduction of keV neutrino dark matter, and explore the phenomenological implications for Big Bang Nucleosynthesis and the number of relativistic degrees of freedom. (AU)

FAPESP's process: 16/01343-7 - ICTP South American Institute for Fundamental Research: a regional center for theoretical physics
Grantee:Nathan Jacob Berkovits
Support Opportunities: Special Projects