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A dense neutrino medium such as that inside a core-collapse supernova can experience collective flavor conversion or oscillations because of the neutral-current weak interaction among the neutrinos.
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G. Mangano, A. Mirizzi, N. Saviano, Damping the neutrino flavor pendulum by breaking homogeneity, Phys.Rev. D89 (7) (2014) 073017 · 2014
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H. Duan, S. Shalgar, Flavor instabilities in the neutrino line model, Phys.Lett. B747 (2015) 139–143 · 2015
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