D. Autiero

Measurement of the neutrino velocity with the OPERA detector in the CNGS beam

A bstractThe OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km. The measurement is based on data taken by OPERA in the years 2009, 2010 and 2011. Dedicated upgrades of the CNGS timing system and of the OPERA detector, as well as a high precision geodesy campaign for the measurement of the neutrino baseline, allowed reaching comparable systematic and statistical accuracies.An arrival time of CNGS muon neutrinos with respect to the one computed assuming the speed of light in vacuum of

The Synergy of the golden and silver channels at the neutrino factory

\left( {6.5\pm 7.4\left( {\mathrm{stat}.} \right)_{-8.0}^{+8.3}\left( {\mathrm{sys}.} \right)} \right)\mathrm{ns}

The synergy of the golden and silver channels at the Neutrino Factory

was measured corresponding to a relative difference of the muon neutrino velocity with respect to the speed of light

Electron/pion separation with an emulsion cloud chamber by using a neural network.

{{{\left( {\upsilon -c} \right)}} \left/ {c} \right.}=\left( {2.7\pm 3.1\left( {\mathrm{stat}.} \right)_{-3.3}^{+3.4}\left( {\mathrm{sys}.} \right)} \right)\times {10^{-6 }}

The neutrino velocity anomaly as an explanation of the missing observation of neutrinos in coincidence with GRB

. The above result, obtained by comparing the time distributions of neutrino interactions and of protons hitting the CNGS target in 10.5 μs long extractions, was confirmed by a test performed at the end of 2011 using a short bunch beam allowing to measure the neutrino time of flight at the single interaction level.

Measurement of low-energy neutrino cross-sections with the PEANUT experiment

Abstract.We deepen the study of the so-called “silver channel”

Search for Solar Axions with the CAST-Experiment

\nu_e \to \nu_\tau

Search for Solar Axions: CAST

[1] and of its relevance to solve some of the ambiguities that can arise in the simultaneous measurement of

Expression of Interest for a very long baseline neutrino oscillation experiment (LBNO)

(\theta_{13},\delta)

A Proposal for a Detector 2 km Away From the T2K Neutrino Source

at the Neutrino Factory by presenting in full detail the characteristics of the considered OPERA-like detector and the experimental treatment of the different backgrounds and signals. Furthermore, we perform a detailed study of the systematic errors associated both with the OPERA-like and the magnetized-iron detectors and their effects on the sensitivity. Finally, we also apply a refined statistical analysis of the simulated events based on the frequentist approach.