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    Resonant scattering and charm showers in ultrahigh-energy neutrino interactions (1985)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: Electron antineutrinos with energy of about 7 x 10 to the 6th GeV have much-enhanced cross sections due to W-boson production off electrons. Possible signals due to cosmic-ray sources are estimated. Higher-energy antineutrinos can efficiently produce a W accompanied by radiation. Another possibility, which could lead to shadowing at modest depths, is resonant production of a charged Higgs particle. The importance of muon production by charm showers in rock is pointed out.
    Keywords: SPACE RADIATION
    Type: Physical Review Letters (ISSN 0031-9007); 55; 1252
    Format: text
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