Resonances Driven by a Neutrino Gyroscope and Collective Neutrino Oscillations in Supernovae

TL;DR

This paper models supernova neutrino flavor evolution using a gyroscope analogy, revealing resonance-driven collective oscillations and the effects of multi-angle damping, providing new insights into these complex phenomena.

Contribution

It introduces a gyroscope-based framework to understand collective neutrino oscillations, extending the analysis from two to four neutrino species and clarifying the impact of emission angles.

Findings

Resonances driven by precession and nutation govern flavor evolution.

Multi-angle effects damp nutation but preserve precession-driven resonances.

The gyroscope analogy offers pedagogical insights into collective oscillations.

Abstract

We show that flavor evolution of a system of neutrinos with continuous energy spectra as in supernovae can be understood in terms of the response of individual neutrino flavor-isospins (NFIS's) to the mean field. In the case of a system initially consisting of nu_e and anti-nu_e with the same energy spectrum but different number densities, the mean field is very well approximated by the total angular momentum of a neutrino gyroscope. Assuming that NFIS evolution is independent of the initial neutrino emission angle, the so-called single-angle approximation, we find that the evolution is governed by two types of resonances driven by precession and nutation of the gyroscope, respectively. The net flavor transformation crucially depends on the adiabaticity of evolution through these resonances. We show that the results for the system of two initial neutrino species can be extended to a system of four species with the initial number densities of nu_e and anti-nu_e significantly larger than those of nu_x and anti-nu_x. Further, we find that when the dependence on the initial neutrino emission angle is taken into account in the multi-angle approximation, nutation of the mean field is quickly damped out and can be neglected. In contrast, precession-driven resonances still govern the evolution of NFIS's with different energy and emission angles just as in the single-angle approximation. Our pedagogical and analytic study of collective neutrino oscillations in supernovae provides some insights into these seemingly complicated yet fascinating phenomena.