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The prompt nu_e burst from a core-collapse supernova (SN) is subject to both matter-induced flavor conversions and strong neutrino-neutrino refractive effects.
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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. I: Correlated neutrino trajectories,” Phys. Rev. D 74
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S. Pastor and G. Raffelt, “Flavor oscillations in the supernova hot bubble region: Nonlinear effects of neutrino background,” Phys. Rev. Lett. 89
2002
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2003
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2004
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G. L. Fogli, E. Lisi, A. Mirizzi and D. Montanino, “Probing supernova shock waves and neutrino flavor transitions in next-generation water-Cherenkov detectors,” JCAP 0504
2005
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R. F. Sawyer, “Speed-up of neutrino transformations in a supernova environment,” Phys. Rev. D 72
2005
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2007
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G.G. Raffelt and G. Sigl, “Self-induced decoherence in dense neutrino gases,” Phys. Rev. D 75
2007
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2007
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2007
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2008
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