Refractive neutrino masses, ultralight dark matter and cosmology
Manibrata Sen, Alexei Y. Smirnov

TL;DR
This paper explores how ultralight scalar dark matter can cause neutrino oscillations through a refractive mass effect, which varies with energy and time, potentially avoiding cosmological mass bounds.
Contribution
It introduces the concept of refractive mass squared for neutrinos due to ultralight dark matter and analyzes its properties and implications for cosmology and neutrino physics.
Findings
Refractive mass squared shows resonance dependence on neutrino energy.
Below resonance, the effective mass decreases with energy, possibly avoiding cosmological bounds.
Refractive mass may depend on time if the background is a coherent classical field.
Abstract
We consider in detail a possibility that the observed neutrino oscillations are due to refraction on ultralight scalar boson dark matter. We introduce the refractive mass squared, , and study its properties: dependence on neutrino energy, state of the background, etc. If the background is in a state of cold gas of particles, shows a resonance dependence on energy. Above the resonance (), we find that has the same properties as usual vacuum mass squared. Below the resonance, decreases with energy, which (if realised) allows us to avoid the cosmological bound on the sum of neutrino masses. Also, may depend on time. We consider the validity of the results: effects of multiple interactions with scalars, and modification of the dispersion relation. We show that for values of parameters of the system required to…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Neutrino Physics Research
