Abstract
Electron antineutrinos with energy 7 × 106 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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1252-1253 |
| Number of pages | 2 |
| Journal | Physical Review Letters |
| Volume | 55 |
| Issue number | 12 |
| DOIs | |
| State | Published - 1985 |
| Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy(all)