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Collective pair conversion $\nu_e\bar\nu_e\leftrightarrow \nu_{x}\bar\nu_{x}$ by forward scattering, where $x=\mu$ or $\tau$, may be generic for supernova neutrino transport.
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J. P. Kneller, Turbulence and neutrinos during the accretion phase, Talk at the INT Program Flavor Observations with Supernova Neutrinos
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