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Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I

Y. AshieJ. HosakaK. IshiharaY. ItowJ. KamedaY. KoshioA. MinaminoC. MitsudaM. MiuraS. MoriyamaM. NakahataT. NambaR. NambuY. ObayashiM. ShiozawaY. SuzukiY. TakeuchiK. TakiS. YamadaM. IshitsukaT. KajitaK. KaneyukiS. NakayamaAtsushi OkadaK. OkumuraC. SajiY. TakenagaS. T. ClarkS. DesaiE. KearnsS. LikhodedJ. L. StoneLawrence SulakW. WangM. GoldhaberD. CasperJ. P. CravensW. GajewskiW. R. KroppD. W. LiuS. MineM. SmyH. W. SobelC. W. SternerM. R. VaginsK. S. GanezerJ. HillW. E. KeigJ. S. JangJ. Y. KimI. T. LimK. ScholbergC. W. WalterR. W. EllsworthS. TasakaG. GuillianA. KibayashiJ. G. LearnedS. MatsunoD. TakemoriM. D. MessierY. HayatoA. K. IchikawaToru IshidaT. IshiiT. IwashitaT. KobayashiT. MaruyamaK. NakamuraKoh‐hei NittaY. OyamaM. SakudaY. TotsukaY. SuzukiM. HasegawaKenji HayashiI. KatoH. MaesakaT. MoritaT. NakayaK. NishikawaT. SasakiS. UedaS. YamamotoT. J. HainesS. DazeleyS. HatakeyamaR. SvobodaE. BlaufussJ. A. GoodmanG. W. SullivanD. TurčanA. HabigY. FukudaC. K. JungT. KatoKazuyoshi KobayashiM. MalekC. MaugerC. McGrewA. SarratE. SharkeyC. YanagisawaT. ToshitoK. MiyanoN. TamuraJ. IshiiY. KunoM. YoshidaS. B. KimJ. YooH. OkazawaT. IshizukaY. ChoiH. K. SeoY. GandoT. HasegawaK. InoueJ. ShiraiY. SuzukiM. KoshibaY. NakajimaK. NishijimaTakaaki HaradaH. IshinoY. WatanabeD. KiełczewskaJ. ZalipskaH. BernsR. GranKiyoshi ShiraishiA. L. StachyraK. WashburnR. J. Wilkes

Abstract

We present a combined analysis of fully-contained, partially-contained and upward-going muon atmospheric neutrino data from a 1489 d exposure of the Super-Kamiokande detector. The data samples span roughly five decades in neutrino energy, from 100 MeV to 10 TeV. A detailed Monte Carlo comparison is described and presented. The data is fit to the Monte Carlo expectation, and is found to be consistent with neutrino oscillations of ${\ensuremath{\nu}}_{\ensuremath{\mu}}\ensuremath{\leftrightarrow}{\ensuremath{\nu}}_{\ensuremath{\tau}}$ with ${sin}^{2}2\ensuremath{\theta}>0.92$ and $1.5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}<\ensuremath{\Delta}{m}^{2}<3.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}3}\text{ }\text{ }{\mathrm{eV}}^{2}$ at 90% confidence level.

Neutrino Physics ResearchAstrophysics and Cosmic PhenomenaParticle physics theoretical and experimental studiesSuper-KamiokandePhysicsNeutrinoNeutrino oscillationMonte Carlo methodMuonSolar neutrinoParticle physicsNuclear physicsSolar neutrino problem
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