The OPERA experiment reached its main goal by proving the appearance of ντ in the CNGS νμ beam. A sample of five ντ candidates was collected allowing to reject the null hypothesis at 5.1σ. The estimation of Δm232 in "appearance mode" has been obtained. Updates on the search for νμ→νe oscillations and on the search for sterile neutrino mixing in the νμ→νe and νμ→ντ channels are also reported.
@article{arxiv.1705.02454,
title = {Results from the OPERA Experiment},
author = {L. Patrizii},
journal= {arXiv preprint arXiv:1705.02454},
year = {2017}
}
Comments
Poster presented at NuPhys2016 (London, 12-14 December 2016). 5 pages, LaTeX