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- W2095611690 abstract "We derive semiclassical neutrino-electron transport equations in the collisionless (Vlasov) limit from the coupled Dirac equations, incorporating the charged and neutral weak current-current as well as electromagnetic interactions. A corresponding linear response theory is derived. In particular, we calculate the response functions for a variety of beam-plasma geometries, which are of interest in a supernova scenario. We apply this to the study of plasmons and to a new class of collective pharon resonance modes, which are characterized by $ensuremath{omega}<q.$ We find that the growth rates of the unstable modes correspond to a strongly temperature $(ensuremath{propto}{T}_{ensuremath{nu}}^{2}{T}_{e}^{3})$ and linearly momentum dependent e-folding length of about ${10}^{10} mathrm{km}$ under typical conditions for type II supernovas. This appears to rule out such long-wavelength collective modes as an efficient means of depositing neutrino energy into the plasma sphere." @default.
- W2095611690 created "2016-06-24" @default.
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- W2095611690 date "2000-12-08" @default.
- W2095611690 modified "2023-09-27" @default.
- W2095611690 title "Collective modes in neutrino “beam” electron-positron plasma interactions" @default.
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- W2095611690 doi "https://doi.org/10.1103/physrevd.63.013008" @default.
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