Neutrino flavour transformation in supernovae

Abstract

Rapid progress has been made during recent years in the understanding of the flavour oscillations that occur as neutrinos traverse through supernova. The previous paradigm has given way and it is now clear that the neutrino signals we shall receive from future Galactic supernovae will allow us both to peer inside these extraordinary cosmic events and to probe some of the fundamental properties of these elusive particles. In this review we aim to distill the progress that has been made focusing upon the effects of the dynamic density profile and the emergence of collective flavour oscillations due to neutrino self-interactions.

48 pages, 14 figures

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• Collective Neutrino Oscillations and Nucleosynthesis
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• Neutrino non-radiative decay and the diffuse supernova neutrino background
• The Neutrino Signal From Pair Instability Supernovae
• Chaos in Inhomogeneous Neutrino Fast Flavor Instability
• Finite size source effects and the correlation of neutrino transition probabilities through supernova turbulence
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• Neutrinos and Symmetries
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• Equation of state in neutron stars and supernovae
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