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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){sub D} symmetry which breaks softly to Z{sub 2}. We study in detail the scalar sector which supports this specific scenario and its rich phenomenology.

Authors:
 [1];  [2];  [3];  [4];  [5]
  1. Département de Mathématique, Faculté des Sciences et Techniques,Université Abdelmalek Essaadi,B. 416, Tangier (Morocco)
  2. LAPTH, UMR 5108,9 chemin de Bellevue, BP 110, 74941 Annecy-Le-Vieux (France)
  3. Department of Physics and Astronomy, University of California,Riverside, California 92521 (United States)
  4. Institute of Physics, Academia Sinica,Nangang, Taipei 11529, Taiwan (China)
  5. (China)
Publication Date:
Sponsoring Org.:
SCOAP3, CERN, Geneva (Switzerland)
OSTI Identifier:
22572067
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2016; Journal Issue: 04; Other Information: PUBLISHER-ID: JCAP04(2016)049; OAI: oai:repo.scoap3.org:15364; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; MAJORANA FERMIONS; MEV RANGE; NEUTRINOS; NONLUMINOUS MATTER; PARTICLE INTERACTIONS; RENORMALIZATION; REST MASS; STANDARD MODEL; U-1 GROUPS

Citation Formats

Arhrib, Abdesslam, Boehm, Céline, Ma, Ernest, Yuan, Tzu-Chiang, and Physics Division, National Center for Theoretical Sciences,Hsinchu, Taiwan. 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, Boehm, Céline, Ma, Ernest, Yuan, Tzu-Chiang, & Physics Division, National Center for Theoretical Sciences,Hsinchu, Taiwan. Radiative model of neutrino mass with neutrino interacting MeV dark matter. United States. doi:10.1088/1475-7516/2016/04/049.
Arhrib, Abdesslam, Boehm, Céline, Ma, Ernest, Yuan, Tzu-Chiang, and Physics Division, National Center for Theoretical Sciences,Hsinchu, Taiwan. Tue . "Radiative model of neutrino mass with neutrino interacting MeV dark matter". United States. doi:10.1088/1475-7516/2016/04/049.
@article{osti_22572067,
title = {Radiative model of neutrino mass with neutrino interacting MeV dark matter},
author = {Arhrib, Abdesslam and Boehm, Céline and Ma, Ernest and Yuan, Tzu-Chiang and Physics Division, National Center for Theoretical Sciences,Hsinchu, Taiwan},
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){sub D} symmetry which breaks softly to Z{sub 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 = {Tue Apr 26 00:00:00 EDT 2016},
month = {Tue Apr 26 00:00:00 EDT 2016}
}