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Cerenkov radiation of longitudinal photons by neutrinos
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Cerenkov radiation of longitudinal photons by neutrinos
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In a relativistic plasma neutrino can emit plasmons by the Cerenkov process which is kinematically allowed for a range of frequencies for which refractive index is greater than one. We have calculated the rate of energy emission by this process. We compute the energy deposited in a stalled supernova shock wave by the Cerenkov process and find that it is much smaller than the Bethe-Wilson mechanism.
Forward citations
Cited by 1 Pith paper
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Cherenkov plasmons emission by primordial neutrinos
A neutrino gas in a cold plasma emits longitudinal Cherenkov plasmons; this can cool scalar-bound neutrino clusters only if they formed at T ≳ 220 keV.
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