Gravitational waves from first-order phase transitions in Majoron models of neutrino mass
Pasquale Di Bari, Danny Marfatia, Ye-Ling Zhou

TL;DR
This paper investigates how first-order phase transitions in Majoron models of neutrino mass can produce detectable gravitational waves across various energy scales, offering new ways to probe neutrino physics and cosmology.
Contribution
It demonstrates the connection between right-handed neutrino mass generation and gravitational wave production in Majoron models, analyzing signals across different energy scales and their detectability.
Findings
High-scale phase transitions produce signals testable by future interferometers.
Low-scale phase transitions at GeV energies can be probed by LISA and complement neutrino searches.
Very low-scale transitions below 100 keV produce signals within reach of SKA and THEIA experiments.
Abstract
We show how the generation of right-handed neutrino masses in Majoron models may be associated with a first-order phase transition and accompanied by the production of a stochastic background of gravitational waves (GWs). We explore different energy scales with only renormalizable operators in the effective potential. If the phase transition occurs above the electroweak scale, the signal can be tested by future interferometers. We consider two possible energy scales for phase transitions below the electroweak scale. If the phase transition occurs at a GeV, the signal can be tested at LISA and provide a complementary cosmological probe to right-handed neutrino searches at the FASER detector. If the phase transition occurs below 100 keV, we find that the peak of the GW spectrum is two or more orders of magnitude below the putative NANOGrav GW signal at low frequencies, but well within…
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