Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO
The MACRO Collaboration, M. Ambrosio et al

TL;DR
This paper reports on the MACRO detector's measurement of atmospheric neutrino-induced upgoing muons, providing evidence for neutrino oscillations through analysis of flux and zenith distribution discrepancies.
Contribution
First measurement of upgoing muon flux with MACRO, showing evidence for neutrino oscillations through flux suppression and zenith angle distribution analysis.
Findings
Observed flux ratio of 0.74 compared to expectations.
Zenith distribution inconsistent with no oscillation hypothesis.
Best-fit oscillation parameters: sin^2(2θ)=1.0, Δm^2≈few×10^-3 eV^2.
Abstract
We present a measurement of the flux of neutrino-induced upgoing muons (<E_nu>~100 GeV) using the MACRO detector. The ratio of the number of observed to expected events integrated over all zenith angles is 0.74 +/- 0.036 (stat) +/- 0.046(systematic) +/- 0.13 (theoretical). The observed zenith distribution for -1.0 < cos(theta) < -0.1 does not fit well with the no oscillation expectation, giving a maximum probability for chi^2 of 0.1%. The acceptance of the detector has been extensively studied using downgoing muons, independent analyses and Monte-Carlo simulations. The other systematic uncertainties cannot be the source of the discrepancies between the data and expectations. We have investigated whether the observed number of events and the shape of the zenith distribution can be explained by a neutrino oscillation hypothesis. Fitting either the flux or zenith distribution independently…
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