Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam

The OPERA experiment, exposed to the CERN to Gran Sasso $\nu_\mu$ beam, collected data from 2008 to 2012. Four oscillated $\nu_\tau$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with $\nu_\mu \to \nu_\tau$ oscillations at the atmospheric $\Delta m^2$ within the "standard" three-neutrino framework. In this paper, the OPERA $\nu_\tau$ appearance results are used to derive limits on the mixing parameters of a massive sterile neutrino.The OPERA experiment, exposed to the CERN to Gran Sasso ν$_{μ}$ beam, collected data from 2008 to 2012. Four oscillated ν$_{τ}$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with ν$_{μ}$ → ν$_{τ}$ oscillations at the atmospheric Δm$^{2}$ within the “standard” three-neutrino framework. In this paper, the OPERA ν$_{τ}$ appearance results are used to derive limits on the mixing parameters of a massive sterile neutrino.The OPERA experiment, exposed to the CERN to Gran Sasso $\nu_\mu$ beam, collected data from 2008 to 2012. Four oscillated $\nu_\tau$ Charged Current interaction candidates have been detected in appearance mode, which are consistent with $\nu_\mu \to \nu_\tau$ oscillations at the atmospheric $\Delta m^2$ within the "standard" three-neutrino framework. In this paper, the OPERA $\nu_\tau$ appearance results are used to derive limits on the mixing parameters of a massive sterile neutrino