Enabling Strong Neutrino Self-interaction with an Unparticle Mediator
Saeid Foroughi-Abari, Kevin J. Kelly, Mudit Rai, Yue Zhang

TL;DR
This paper proposes a novel neutrino self-interaction model using unparticles as mediators, which can evade existing constraints and support strong interactions relevant to cosmology, opening new experimental possibilities.
Contribution
It introduces a continuous spectral density unparticle mediator for neutrino interactions, mitigating key constraints and expanding viable parameter space.
Findings
Unparticle mediators can pass cosmological constraints on neutrino number.
Unparticle interactions are less resonant, easing IceCube constraints.
Model supports strong neutrino self-interactions relevant for cosmology.
Abstract
Recent explorations of the cosmic microwave background and the large-scale structure of the universe have indicated a preference for sizable neutrino self-interactions, much stronger than what the Standard Model offers. When interpreted in the context of simple particle-physics models with a light, neutrinophilic scalar mediator, some of the hints are already in tension with the combination of terrestrial, astrophysical and cosmological constraints. We take a novel approach by considering neutrino self-interactions through a mediator with a smooth, continuous, spectral density function. We consider Georgi's unparticle with a mass gap as a concrete example and point out two useful effects for mitigating two leading constraints. 1) The Unparticle is ``broadband'' -- it occupies a wide range of masses which allows it to pass the early universe constraint on effective number of extra…
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Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
