Self-induced neutrino flavor conversion without flavor mixing
Sovan Chakraborty, Rasmus Sloth Hansen, Ignacio Izaguirre, Georg, Raffelt

TL;DR
This paper demonstrates that neutrino flavor conversion can occur rapidly through collective effects independent of neutrino mass differences, driven by neutrino-neutrino interactions and angular distributions, especially in dense astrophysical environments.
Contribution
It introduces the concept of fast flavor conversion driven by neutrino interactions, occurring without neutrino mass or mixing, and explores simplified models to understand this phenomenon.
Findings
Fast flavor conversion rates are much higher than vacuum oscillation frequencies.
Flavor conversion can occur even with zero neutrino mass differences.
Angular distributions of neutrinos are key to triggering fast conversion.
Abstract
Neutrino-neutrino refraction in dense media can cause self-induced flavor conversion triggered by collective run-away modes of the interacting flavor oscillators. The growth rates were usually found to be of order a typical vacuum oscillation frequency . However, even in the simple case of a beam interacting with an opposite-moving beam, and allowing for spatial inhomogeneities, the growth rate of the fastest-growing Fourier mode is of order , a typical -- interaction energy. This growth rate is much larger than the vacuum oscillation frequency and gives rise to flavor conversion on a much shorter time scale. This phenomenon of "fast flavor conversion" occurs even for vanishing and thus does not depend on energy, but only on the angle distributions. Moreover, it does not require neutrinos to mix…
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