The OPERA experiment in the CERN to Gran Sasso neutrino beam

By R. Acquafredda, T. Adam, N. Agafonova, P. A. Sanchez, M. Ambrosio, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, L. Arrabito and 252 more. 2009

249 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

A facility to Search for Hidden Particles (SHiP) at the CERN SPS (2015, methodology): “The use of such detector made it possible to observe ντ charged current interactions in DONUT [56] and OPERA [48] experiments.”
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam (2011, methodology): “The relative fraction of cosmic ray events accidentally falling in this window is 10−4 and it is therefore negligible [1, 46].”
Geophysical muon imaging: feasibility and limits (2010, background): “This choice was also guided by the strong experience acquired by several authors of the present paper who participate to the OPERA experiment (Acquafredda et al. 2009).”
New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam (2013, unknown): “The OPERA detector [41] is designed to tackle a challenging task: achieving micro-metric tracking accuracy over a very large detector volume spanning about (6.”