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Impact of semi-annihilation of ℤ3symmetric dark matter with radiative neutrino masses

Aoki, Mayumi; Toma, Takashi

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Authors

Mayumi Aoki

Takashi Toma



Abstract

We investigate a Bbb Z3 symmetric model with two-loop radiative neutrino masses. Dark matter in the model is either a Dirac fermion or a complex scalar as a result of an unbroken Bbb Z3 symmetry. In addition to standard annihilation processes, semi-annihilation of the dark matter contributes to the relic density. We study the effect of the semi-annihilation in the model and find that those contributions are important to obtain the observed relic density. The experimental signatures in dark matter searches are also discussed, where some of them are expected to be different from the signatures of dark matter in Bbb Z2 symmetric models.

Citation

Aoki, M., & Toma, T. (2014). Impact of semi-annihilation of ℤ3symmetric dark matter with radiative neutrino masses. Journal of Cosmology and Astroparticle Physics, 2014(09), Article 016. https://doi.org/10.1088/1475-7516/2014/09/016

Journal Article Type Article
Acceptance Date Aug 17, 2014
Online Publication Date Sep 8, 2014
Publication Date Sep 30, 2014
Deposit Date Apr 23, 2019
Publicly Available Date Apr 23, 2019
Journal Journal of Cosmology and Astroparticle Physics
Electronic ISSN 1475-7516
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2014
Issue 09
Article Number 016
DOI https://doi.org/10.1088/1475-7516/2014/09/016
Public URL https://durham-repository.worktribe.com/output/1303358

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Article funded by SCOAP. 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.





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