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- W2019425374 abstract "Various current models and generalizations of a universal weak Fermi interaction predict a first-order weak coupling between electrons and $ensuremath{nu}ensuremath{-}overline{ensuremath{nu}}$ pairs. The radiation of such pairs by a hot, partially degenerate relativistic plasma is calculated for temperatures and densities that appear to be relevant for stellar evolution. Neutrino-pair emission by collective electron modes, especially transverse plasma excitations, is found to be the main mechanism for neutrino radiation by a dense stellar plasma when electron-positron production is small either because the temperature is too low ($Tensuremath{lesssim}{10}^{8}$ ifmmode^circelsetextdegreefi{}K) or degeneracy supresses it. The neutrino luminosity of a star can greatly exceed its photon luminosity for a central core temperature greater than ${10}^{8}$ ifmmode^circelsetextdegreefi{}K." @default.
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- W2019425374 date "1963-02-01" @default.
- W2019425374 modified "2023-10-14" @default.
- W2019425374 title "Neutrino Pair Emission by a Stellar Plasma" @default.
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- W2019425374 doi "https://doi.org/10.1103/physrev.129.1383" @default.
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