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Limits on dark matter WIMPs using upward-going muons in the MACRO detector
The MACRO Collaboration, M. Ambrosio et al
We perform an indirect search for Weakly Interacting Massive Particles (WIMPs) using the MACRO detector to look for neutrino-induced upward-going muons resulting from the annihilat…
Measurement of the solar neutrino energy spectrum using neutrino-electron scattering
Kamiokande collaboration
A measurement of the energy spectrum of recoil electrons from solar neutrino scattering in the Super--Kamiokande detector is presented. The results shown here are obtained from 504…
Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super-Kamiokande
Kamiokande Collaboration, Y. Fukuda, T. Hayakawa +2
A search for day-night variations in the solar neutrino flux resulting from neutrino oscillations has been carried out using the 504 day sample of solar neutrino data obtained at S…
The Observation of Up-going Charged Particles Produced by High Energy Muons in Underground Detectors
The MACRO Collaboration, M. Ambrosio et al
An experimental study of the production of up-going charged particles in inelastic interactions of down-going underground muons is reported, using data obtained from the MACRO dete…
Measurement of the energy spectrum of underground muons at Gran Sasso with a transition radiation detector
The MACRO Collaboration, M. Ambrosio et al
We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the Gran Sasso Laboratory. For this measurement we have used a transition radiation…
Observation of the Shadowing of Cosmic Rays by the Moon using a Deep Underground Detector
The MACRO Collaboration, M. Ambrosio et al
Using data collected by the MACRO experiment during the years 1989-1996, we show evidence for the shadow of the moon in the underground cosmic ray flux with a significance of 3.6 s…
Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO
The MACRO Collaboration, M. Ambrosio et al
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…
Search for Proton Decay via p -> e+ pi0 in a Large Water Cherenkov Detector
Kamiokande Collaboration, M. Shiozawa
We have searched for proton decay via p -> e+ pi0 using data from a 25.5 kton-year exposure of the Super-Kamiokande detector. We find no candidate events with an expected backgroun…
Study of the atmospheric neutrino flux in the multi-GeV energy range
Kamiokande Collaboration, Y. Fukuda et al
The flavor ratio of the atmospheric neutrino flux and its zenith angle dependence have been studied in the multi-GeV energy range using an exposure of 25.5 kiloton-years of the Sup…