Renormalization Group Study of the Minimal Majoronic Dark Radiation and Dark Matter Model
arXiv:1604.02017 · doi:10.1088/1475-7516/2016/07/027
Abstract
We study the 1-loop renormalization group equation running in the simplest singlet Majoron model constructed by us earlier to accommodate the dark radiation and dark matter content in the universe. A comprehensive numerical study was performed to explore the whole model parameter space. A smaller effective number of neutrinos , or a Majoron decoupling temperature higher than the charm quark mass, is preferred. We found that a heavy scalar dark matter, , of mass TeV is required by the stability of the scalar potential and an operational type-I see-saw mechanism for neutrino masses. A neutral scalar, , of mass in the GeV range and its mixing with the standard model Higgs as large as is also predicted. The dominant decay modes are into and/or . A sensitive search will come from rare decays via the chain , where is a Standard Model fermion, followed by into a pair of Majoron and/or b-quarks. The interesting consequences of dark matter bound state due to the sizable -coupling are discussed as well. In particular, shower-like events with an apparent neutrino energy at could contribute to the observed effective neutrino flux in underground neutrino detectors such as IceCube.
33 pages,11 figures, published version
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