Evidence for $\nu_\mu \to \nu_\tau$ appearance in the CNGS neutrino beam with the OPERA experiment
Phys. Rev. D 89, 051102 (2014) The OPERA experiment is designed to search for $\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations in appearance mode i.e. through the direct observation of the $\tau$ lepton in $\nu_{\tau}$ charged current interactions. The experiment has taken data for five years, since...
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Journal Article |
Language: | English |
Published: |
09-01-2014
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Subjects: | |
Online Access: | Get full text |
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Summary: | Phys. Rev. D 89, 051102 (2014) The OPERA experiment is designed to search for $\nu_{\mu} \rightarrow
\nu_{\tau}$ oscillations in appearance mode i.e. through the direct observation
of the $\tau$ lepton in $\nu_{\tau}$ charged current interactions. The
experiment has taken data for five years, since 2008, with the CERN Neutrino to
Gran Sasso beam. Previously, two $\nu_{\tau}$ candidates with a $\tau$ decaying
into hadrons were observed in a sub-sample of data of the 2008-2011 runs. Here
we report the observation of a third $\nu_\tau$ candidate in the
$\tau^-\to\mu^-$ decay channel coming from the analysis of a sub-sample of the
2012 run. Taking into account the estimated background, the absence of
$\nu_{\mu} \rightarrow \nu_{\tau}$ oscillations is excluded at the 3.4 $\sigma$
level. |
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DOI: | 10.48550/arxiv.1401.2079 |