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In the dense-neutrino region above the neutrino sphere of a supernova (r > 400 km), neutrino-neutrino refraction causes collective flavor transformations.
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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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H. Duan, G. M. Fuller, J. Carlson and Y. Z. Qian, “Coherent development of neutrino flavor in the supernova environment,” Phys. Rev. Lett. 97
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2006
Cited alongside, same era.
H. Duan, G. M. Fuller, J. Carlson and Y. Z. Qian, “Analysis of collective neutrino flavor transformation in supernovae,” arXiv:astro-ph/0703776
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