Journal article
Two radiative inverse seesaw models, dark matter, and baryogenesis
I Baldes, NF Bell, K Petraki, RR Volkas
Journal of Cosmology and Astroparticle Physics | Published : 2013
Abstract
The inverse seesaw mechanism allows the neutrino masses to be generated by new physics at an experimentally accessible scale, even with O(1) Yukawa couplings. In the inverse seesaw scenario, the smallness of neutrino masses is linked to the smallness of a lepton number violating parameter. This parameter may arise radiatively. In this paper, we study the cosmological implications of two contrasting radiative inverse seesaw models, one due to Ma and the other to Law and McDonald. The former features spontaneous, the latter explicit lepton number violation. First, we examine the effect of the lepton-number violating interactions introduced in these models on the baryon asymmetry of the univers..
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Funding Acknowledgements
We thank S.S.C. Law and K.L. McDonald for their useful comments. IB was supported by the Commonwealth of Australia. NFB, KP, and RRV were supported by the Australian Research Council. KP was also supported by the Netherlands Foundation for Fundamental Research of Matter (FOM) and the Netherlands Organisation for Scientific Research (NWO).