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The dense neutrino medium in a core-collapse supernova or a neutron-star merger event can experience fast flavor conversions on time/distance scales that are much smaller than those of vacuum oscillations.
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John F. Beacom, “The Diffuse Supernova Neutrino Background,” Ann. Rev. Nucl. Part. Sci. 60
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2011
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Hans-Thomas Janka, “Explosion Mechanisms of Core-Collapse Supernovae,” Ann. Rev. Nucl. Part. Sci. 62
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2012
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2012
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Adam Burrows, “Colloquium: Perspectives on core-collapse supernova theory,” Rev. Mod. Phys. 85
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