Collective three-flavor oscillations of supernova neutrinos
Basudeb Dasgupta, Amol Dighe

TL;DR
This paper develops a comprehensive three-flavor formalism for supernova neutrino oscillations, revealing how collective effects can be understood through factorization into two-flavor oscillations and visualized with a triangle diagram.
Contribution
It introduces a generalized formalism for three-flavor neutrino oscillations in supernovae, enabling analytical descriptions of complex collective phenomena and their interplay with MSW effects.
Findings
Flavor conversions can be factorized into two-flavor oscillations.
The formalism describes phenomena like bipolar and spectral split.
The triangle diagram visualizes three-flavor effects.
Abstract
Neutrinos and antineutrinos emitted from a core collapse supernova interact among themselves, giving rise to collective flavor conversion effects that are significant near the neutrinosphere. We develop a formalism to analyze these collective effects in the complete three-flavor framework. It naturally generalizes the spin-precession analogy to three flavors and is capable of analytically describing phenomena like vacuum/MSW oscillations, synchronized oscillations, bipolar oscillations and spectral split. Using the formalism, we demonstrate that the flavor conversions may be "factorized" into two-flavor oscillations with hierarchical frequencies. We explicitly show how the three-flavor solution may be constructed by combining two-flavor solutions. For a typical supernova density profile, we identify an approximate separation of regions where distinctly different flavor conversion…
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