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Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam
N. Agafonova, A. Alexandrov, A. Anokhina +132
OPERA is a long-baseline experiment designed to search for oscillations in appearance mode. It was based at the INFN Gran Sasso laboratory (LNGS) and took data from 200…
Sensitivity of the SHiP experiment to Heavy Neutral Leptons
SHiP Collaboration
Heavy Neutral Leptons (HNLs) are hypothetical particles predicted by many extensions of the Standard Model. These particles can, among other things, explain the origin of neutrino…
Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
N. Agafonova, A. Alexandrov, A. Anokhina +125
The OPERA experiment discovered muon neutrino into tau neutrino oscillations in appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus was also en…
Modulations of the Cosmic Muon Signal in Ten Years of Borexino Data
The Borexino Collaboration, M. Agostini, K. Altenmüller +113
We have measured the flux of cosmic muons in the Laboratori Nazionali del Gran Sasso at 3800\,m\,w.e. to be based on ten y…
Speeding up complex multivariate data analysis in Borexino with parallel computing based on Graphics Processing Unit
X. F. Ding, M. Agostini, K. Altenmuller +104
A spectral fitter based on the graphics processor unit (GPU) has been developed for Borexino solar neutrino analysis. It is able to shorten the fitting time to a superior level com…
Final results of the OPERA experiment on appearance in the CNGS beam
OPERA Collaboration, N. Agafonova, A. Alexandrov +134
The OPERA experiment was designed to study oscillations in appearance mode in the CNGS neutrino beam. In this letter we report the final analysis of the full data sampl…