Resonant scattering and charm showers in ultrahigh-energy neutrino interactions

Details Resonant scattering and charm showers in ultrahigh-energy neutrino interactions Resonant scattering and charm showers in ultrahigh-energy neutrino interactions

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55.1252w&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, Sept. 16, 1985, p. 1252, 1253. NASA-supported research.

Physics

13

Antineutrinos, Cosmic Ray Showers, High Energy Interactions, Neutrinos, Particle Production, Resonance Scattering, Bosons, Charm (Particle Physics), Muons, Scattering Cross Sections

Scientific paper

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.

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