Speaker
Svetlana Zemskova
(JINR)
Description
The main goal of the OPERA experiment is the direct observation of $\nu_{\mu} \to \nu_{\tau}$ oscillations in the appearance mode in the quasi pure $\nu_{\mu}$ CNGS beam. Profiting of the tracking capabilities of the OPERA active target it is possible to detect and reconstruct $\nu_e$ interactions and, therefore, study the subdominant $\nu_{\mu} \to \nu_e$ oscillation channel. Current results on this channel in the three-flavour mixing model are presented. The same data allow to constrain the non-standard oscillation parameters indicated by the LSND and MiniBooNE experiments.
