The OPERA experiment: on the way to the direct observation of $\nu_\mu \to \nu_\tau$ oscillation

TL;DR

The OPERA experiment aims to directly observe $ u_ au$ appearance from $ u_$ oscillations using a specialized detector at CERN, with initial results supporting its capability to identify tau neutrino interactions.

Contribution

This paper introduces the OPERA detector setup and analysis methods for detecting $ u_ au$ events, marking a significant step towards direct observation of neutrino oscillations.

Findings

Initial data shows successful detection of $ u_ au$ candidates.

The detector effectively distinguishes $ u_ au$ interactions from background.

Preliminary results support the experiment's design goals.

Abstract

OPERA (\emph{O}scillation \emph{P}roject with \emph{E}mulsion t\emph{R}acking \emph{A}pparatus) is a long-baseline neutrino experiment, designed to provide the first direct proof of $\nu_\mu \to \nu_\tau$ oscillation in the atmospheric sector using the \emph{C}ERN \emph{N}eutrinos to \emph{G}ran \emph{S}asso (CNGS) $\nu_\mu$ beam. The detector, consisting of a modular target made of lead - nuclear emulsion units complemented by electronic trackers and muon spectrometers, has been conceived to select $\rm{\nu_\tau}$ charged current interactions, among all neutrino flavour events, through the observation of the outcoming tau leptons and subsequent decays. In this paper, the detector, the event analysis chain and the preliminary results from the first OPERA physics run are reported.