MACRO results on atmospheric neutrinos

dc.creatorGiacomelli, G.
dc.creatorMargiotta, A.
dc.date2005-04-16
dc.date2005-04-19
dc.date.accessioned2026-07-07T06:38:14Z
dc.date.available2026-07-07T06:38:14Z
dc.descriptionWe discuss the final results of the MACRO experiment on atmospheric neutrino oscillations. The data concern event topologies with average neutrino energies of ~3 and ~50 GeV. Multiple Coulomb Scattering of the high energy muons was used to estimate the neutrino energy event by event. The angular distributions, the L/E_nu distribution, the particle ratios and the absolute fluxes all favor nu_mu --> nu_tau oscillations with maximal mixing and Delta m^2 ~0.0023 eV^2. Emphasis is given to measured ratios which are not affected by Monte Carlo (MC) absolute normalization; a discussion is made on MC uncertainties. A preliminary search for possible Lorentz invariance violation contributions to atmospheric neutrino oscillations is presented and discussed.
dc.description4 pages, 6 figures. Paper presented at the NOW 2004 Workshop, Conca Specchiulla, Otranto, Italy, September 2004
dc.identifierhttps://arxiv.org/abs/hep-ex/0504029
dc.identifierhttp://arxiv.org/abs/hep-ex/0504029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/100667
dc.subjectHigh Energy Physics - Experiment
dc.subjectAstrophysics
dc.titleMACRO results on atmospheric neutrinos
dc.typetext

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