Completing RHINO
Pasquale Di Bari, Adam Murphy

TL;DR
The RHINO model unifies neutrino mass generation and matter origin, showing how Higgs portal interactions can produce dark neutrinos that explain dark matter and neutrino flux anomalies, with implications for high-scale physics.
Contribution
This work introduces a comprehensive RHINO framework that links neutrino masses, dark matter production, and matter-antimatter asymmetry within a grand unified context.
Findings
Dark neutrinos can serve as decaying dark matter up to 100 TeV.
Enhanced dark neutrino production can occur via thermalisation before oscillations.
Decays of dark neutrinos may explain IceCube high-energy neutrino excess.
Abstract
The right-handed (RH) Higgs-induced neutrino mixing (RHINO) model explains neutrino masses and origin of matter in the universe within a unified picture. The mixing, effectively described by a dimension five operator, is responsible both for the production of dark neutrinos, converting a small fraction of seesaw neutrinos acting as source, and for their decays. We show that including the production of source neutrinos from Higgs portal interactions, their abundance can thermalise prior to the onset of source-dark neutrino oscillations, resulting into an enhanced production of dark neutrinos that thus can play the role of decaying dark matter (DM) for a much higher seesaw scale. This can be above the sphaleron freeze-out temperature and as high as , so that strong thermal resonant leptogenesis for the generation of the matter-antimatter asymmetry is viable. We obtain…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
