Journal
PHYSICS LETTERS B
Volume 726, Issue 4-5, Pages 744-746Publisher
ELSEVIER
DOI: 10.1016/j.physletb.2013.09.049
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Funding
- US Department of Energy [DE-FG03-94ER40837]
- Croatian Ministry of Science, Education and Sports [119-0982930-1016]
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We propose a new realization of the one-loop radiative model of neutrino mass generated by dark matter (scotogenic), where the particles in the loop have an additional U(1)(D) gauge symmetry, which may be exact or broken to Z(2). This model is relevant to a number of astrophysical observations, including AMS-02 and the dark-matter distribution in dwarf galactic halos. (C) 2013 Elsevier B.V. All rights reserved.
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