Renormalization Group Study of the Minimal Majoronic Dark Radiation and Dark Matter Model
We-Fu Chang, John N. Ng

TL;DR
This paper investigates the renormalization group evolution of a minimal Majoron model that explains dark radiation and dark matter, predicting specific particle masses, mixing angles, and potential signals in neutrino detectors.
Contribution
It provides a comprehensive numerical analysis of the model's parameter space, identifying viable dark matter and neutrino mass scenarios, and explores potential experimental signatures.
Findings
Heavy scalar dark matter mass 1.5-4 TeV for stability
Predicted scalar S mass 10-100 GeV with large Higgs mixing
Potential signals in rare Z decays and neutrino detectors
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…
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