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Title: Radiative model of neutrino mass with neutrino interacting MeV dark matter

Abstract

We consider the radiative generation of neutrino mass through the interactions of neutrinos with MeV dark matter. We construct a realistic renormalizable model with one scalar doublet (in additional to the standard model doublet) and one complex singlet together with three light singlet Majorana fermions, all transforming under a dark U(1)(D) symmetry which breaks softly to Z(2). We study in detail the scalar sector which supports this specific scenario and its rich phenomenology.

Authors:
 [1];  [2];  [3];  [4]
  1. Univ. Abdelmalek Essaadi, Tangier, (Morocco)
  2. Centre National de la Recherche Scientifique (CNRS), Annecy-le-Vieux (France). Lab. D' Annecy-le-Vieux de Physique Theorique (LAPth)
  3. Univ. of California, Riverside, CA (United States)
  4. National Center for Theoretical Sciences, Hsinchu (Taiwan); Academia Sinica, Taipei (Taiwan)
Publication Date:
Research Org.:
Univ. Abdelmalek Essaadi, Tangier, (Morocco)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1437996
Grant/Contract Number:  
SC0008541
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Cosmology and Astroparticle Physics
Additional Journal Information:
Journal Volume: 2016; Journal Issue: 04; Journal ID: ISSN 1475-7516
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS

Citation Formats

Arhrib, Abdesslam, Bohm, Celine, Ma, Ernest, and Yuan, Tzu -Chiang. Radiative model of neutrino mass with neutrino interacting MeV dark matter. United States: N. p., 2016. Web. doi:10.1088/1475-7516/2016/04/049.
Arhrib, Abdesslam, Bohm, Celine, Ma, Ernest, & Yuan, Tzu -Chiang. Radiative model of neutrino mass with neutrino interacting MeV dark matter. United States. doi:10.1088/1475-7516/2016/04/049.
Arhrib, Abdesslam, Bohm, Celine, Ma, Ernest, and Yuan, Tzu -Chiang. Tue . "Radiative model of neutrino mass with neutrino interacting MeV dark matter". United States. doi:10.1088/1475-7516/2016/04/049. https://www.osti.gov/servlets/purl/1437996.
@article{osti_1437996,
title = {Radiative model of neutrino mass with neutrino interacting MeV dark matter},
author = {Arhrib, Abdesslam and Bohm, Celine and Ma, Ernest and Yuan, Tzu -Chiang},
abstractNote = {We consider the radiative generation of neutrino mass through the interactions of neutrinos with MeV dark matter. We construct a realistic renormalizable model with one scalar doublet (in additional to the standard model doublet) and one complex singlet together with three light singlet Majorana fermions, all transforming under a dark U(1)(D) symmetry which breaks softly to Z(2). We study in detail the scalar sector which supports this specific scenario and its rich phenomenology.},
doi = {10.1088/1475-7516/2016/04/049},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 04,
volume = 2016,
place = {United States},
year = {2016},
month = {4}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 17 works
Citation information provided by
Web of Science

Figures / Tables:

Figure 1 Figure 1: One-loop scotogenic neutrino mass from U(1)D breaking to Z2.

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    Works referencing / citing this record:

    Parametrization of the Yukawa matrix in the scotogenic model and single-zero textures of the neutrino mass matrix
    journal, July 2019


    Parametrization of the Yukawa matrix in the scotogenic model and single-zero textures of the neutrino mass matrix
    journal, July 2019


      Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.