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Neutrinos in supernovae, neutron stars, and in the early Universe may change flavor collectively and unstably, due to neutrino-neutrino forward-scattering.
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R. Sawyer, Speed-up of neutrino transformations in a supernova environment , Phys. Rev. D 72
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H. Duan, G. M. Fuller and Y.-Z. Qian, Collective neutrino flavor transformation in supernovae , Phys. Rev. D 74
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H. Duan, G. M. Fuller, J. Carlson and Y.-Z. Qian, Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the Supernova Environment. 1. Correlated Neutrino Trajectories , Phys. Rev. D 74
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A. Burrows and D. Vartanyan, Core-Collapse Supernova Explosion Theory , Nature 589
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M. Sen, New Aspects of Supernova Neutrino Flavor Conversions: In the Standard Model and Beyond , Ph.D. thesis, Tata Institute of Fundamental Research, 8, 2018
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