An estimate of the energy of neutrino-induced muons in MACRO is provided by a multiple Coulomb scattering measurement. The MACRO original upward-muon data sample has been subdivided according to the reconstructed muon energy. Data in each subset are then compared with expected fluxes from atmospheric neutrinos. The results are interpreted in terms of neutrino oscillations.
- Pub Date:
- January 2002
- High Energy Physics - Experiment
- 4 pages, 5 EPS figures included with includegraphics, uses icrc.cls Talk given at the 27th International Cosmic Ray Conference, Hamburg, Germany 07-15 Aug 2001