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- W2087508032 abstract "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." @default.
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- W2087508032 date "1985-09-16" @default.
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- W2087508032 title "Resonant Scattering and Charm Showers in Ultrahigh-Energy Neutrino Interactions" @default.
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- W2087508032 doi "https://doi.org/10.1103/physrevlett.55.1252" @default.
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