Publication | Open Access
Measurement of neutrino and antineutrino neutral-current quasielasticlike interactions on oxygen by detecting nuclear deexcitation <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>γ</mml:mi></mml:math> rays
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Citations
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References
2019
Year
Neutrino PropertyT2k NeutrinoEngineeringNuclear PhysicsNuclear DataNeutrino PhysicMath XmlnsLong Baseline Neutrino ExperimentLepton-nucleon ScatteringNuclear DeexcitationHigh-energy Nuclear ReactionPhysicsNuclear TheoryNeutrino AstronomyCosmic RaySynchrotron RadiationNuclear AstrophysicsAntineutrino ResultExperimental Nuclear PhysicsNatural SciencesParticle PhysicsApplied Physics
Neutrino- and antineutrino-oxygen neutral-current quasielasticlike interactions are measured at Super-Kamiokande using nuclear deexcitation $\ensuremath{\gamma}$ rays to identify signal-like interactions in data from a $14.94(16.35)\ifmmode\times\else\texttimes\fi{}{10}^{20}$ protons-on-target exposure of the T2K neutrino (antineutrino) beam. The measured flux-averaged cross sections on oxygen nuclei are $⟨{\ensuremath{\sigma}}_{\ensuremath{\nu}\text{\ensuremath{-}}\mathrm{NCQE}}⟩=1.70\ifmmode\pm\else\textpm\fi{}0.17(\mathrm{stat}.{)}_{\ensuremath{-}0.38}^{+0.51}(\mathrm{syst}.)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}38}\text{ }\text{ }{\mathrm{cm}}^{2}/\text{oxygen}$ with a flux-averaged energy of 0.82 GeV and $⟨{\ensuremath{\sigma}}_{\overline{\ensuremath{\nu}}\text{\ensuremath{-}}\mathrm{NCQE}}⟩=0.98\ifmmode\pm\else\textpm\fi{}0.16(\mathrm{stat}.{)}_{\ensuremath{-}0.19}^{+0.26}(\mathrm{syst}.)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}38}\text{ }\text{ }{\mathrm{cm}}^{2}/\text{oxygen}$ with a flux-averaged energy of 0.68 GeV, for neutrinos and antineutrinos, respectively. These results are the most precise to date, and the antineutrino result is the first cross section measurement of this channel. They are compared with various theoretical predictions. The impact on evaluation of backgrounds to searches for supernova relic neutrinos at present and future water Cherenkov detectors is also discussed.
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