6533b82efe1ef96bd1293265
RESEARCH PRODUCT
Observation of Electron Neutrino Appearance in a Muon Neutrino Beam
Y. YamadaE. RondioN. MccauleyK. HuangM. BassS. L. CartwrightK. ConnollyJ. KamedaP. PrzewlockiM. J. WilkingJ. ZmudaL. L. KormosD. BrailsfordR. OhtaAndré RubbiaR. PoutissouS. TakahashiD. TerhorstLester D.r. ThompsonK. ZarembaF. SatoR. CastilloYuichi OyamaJ. KisielBerardiR. P. LitchfieldF. Di LodovicoC. HeartyA. IzmaylovJ. SteinmannAtsushi TakedaA. KilinskiC. W. WalterK. GiljeA. V. WaldronT. NagasakiAlexander FinchA. CliftonT. DealtryA. MissertA. RedijS. AssylbekovA. LonghinL. LudoviciJ. Caravaca RodríguezYu. G. KudenkoJ. MarteauP. A. RodriguesM. LaweR. J. SmithZ. WilliamsonA. KolacekeH.a. TanakaP. RojasK. NakayoshiL. MonfregolaKimihiro OkumuraP. HamiltonS. TobayamaFrédéric DufourT. OkusawaJoshua HignightYoshihiro SuzukiS. MurphyC. LicciardiM. IkedaA. C. KabothY. FukudaY. TotsukaI. LamontD. AutieroR. A. JohnsonM. MiuraL. MagalettiC. GigantiF. RetiereM. A.m. RaynerT. WachalaB. QuilainDennisT. WongjiradM. VaginsS. HorikawaT. AkiriS. BerkmanA. C. WeberRobert WilsonJ. M. PoutissouC. BronnerK. MavrokoridisJ. AdamJ. LagodaSy SuzukiF. D. M. BlaszczykM. MurdochHiroyuki SekiyaT. SzeglowskiS. YenC. BojechkoR. L. HelmerKendall MahnS. KumaratungaYusuke KoshioGalymovM. RavonelMarco LavederD. CherdackK. AbeR. SaccoC. McgrewY. KanazawaB. StillMasashi TanakaA. P. FurmanskiP. StamoulisA. GaudinL. KochT. SekiguchiA. HillairetY. PetrovKen SakashitaC. AndreopoulosA. ZalewskaK. NishikawaG. ChristodoulouD. NaplesT. HaraA. JacobS. ManlyAntonin VacheretW. R. KroppT. HasegawaS. MineC. K. JungW. TokiG. De RosaJ. HoleczekS. NakayamaK. E. DuffyIain Alexander BertramS. W. K. EmeryK. KosekiK. IyogiR. A. OwenD. KielczewskaM. BatkiewiczJ. F. MartinM. TzanovM. IevaJan T. SobczykC. J. MetelkoS. M. OserA. DabrowskaS. DytmanM. BarbiN. GrantJ. ImberS. MoriyamaS. ShortN. C. HastingsG. CollazuolE. D. ZimmermanJ.j. Gómez-cadenasE. MazzucatoH. KuboG. F. PearceY. SeiyaM. MacaireMasayuki NakahataA. KonakaF. BayM. PosiadalaY. UchidaM. B. SmyM. G. CatanesiP. PlonskiR. TacikJ. D. PerkinMark ScottOleg MineevJ. SchwehrO. PerevozchikovHajime TanakaM. GoninTakahiro HirakiC. PistilloL. EscuderoP. De PerioS. BordoniD. GoeldiS. Di LuiseL. CremonesiHadleyT. YuanPalladinoT. J. IrvineM. ZiembickiJ. ZalipskaJ. InslerK. LaihemY. SudaHenry W. SobelT. LindnerW. OryszczakD. SgalabernaC. DenshamM. SorelB. SmithO. DrapierM. NirkkoE. Reinherz-aronisMichal DziewieckiKazuhiro YamamotoR. A. WendellY. NishimuraTakaaki KajitaMatveevK. UenoA. K. IchikawaTomoko ArigaY. ShustrovS. HirotaB. E. BergerS. RothM. MezzettoA. CerveraFederico SanchezG. VasseurE. S. Pinzon GuerraTh. A. MuellerM. ZitoMatthew T. ReevesJ. MarzecPaoloneD. PayneH. KakunoI. KresloC. NielsenH. M. O'keeffeE. ScantamburloP. KitchingM. O. WasckoE. KearnsC. ListerR.p. KurjataS. W. BenthamAkitaka ArigaT. TsukamotoL. ZambelliB. A. PopovShigeki AokiT. MaruyamaL. PickardR. TerriS. GiffinWilsonKate ScholbergT. NakadairaJ. H. JoA. MurakamiM. HartzI. Z. DankoA. ThorleyA. KorzenevG.d. BarrA. MinaminoM. MalekRhiju DasB. JamiesonK. P. LeeI. KarpikovS. J. ColemanL. SouthwellJ. MyslikC. TouramanisAntonio EreditatoN. YershovT. GolanKevin Scott McfarlandT. KikawaTakashi KobayashiJ. DumarchezL. FloetottoScott DavisD. HansenS. J. IvesC. A. MillerT. TomuraE. L. MathieS. B. BoydT. IshiiM. M. KhabibullinK. SuzukiM. MccarthyY. TakeuchiT. IshidaD. RuterboriesHiroaki AiharaP. N. RatoffT. KutterKoji NakamuraA. N. KhotjantsevY. FujiiA. SuzukiMasashi YokoyamaE. PoplawskaTsuyoshi NakayaM. FriendA. BravarMasato ShiozawaM. TadaA. HaeslerP. JonssonS. BhadraP. SinclairArnaud RobertP. MijakowskiJy KimA. HimmelE. RadicioniR. G. CallandD. GudinM. LazosD. L. WarkA. D. MarinoA. BlondelN. J. BuchananK. IekiD. KarlenR. J. WilkesC. WilkinsonC. YanagisawaGareth J. BarkerM. HierholzerJ. P. ColemanYoshinari HayatoHaighT. DuboyskiT. Nakaisubject
General PhysicsParticle physicsSolar neutrinoPhysics MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomy7. Clean energy09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tau neutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillation01 Mathematical SciencesPhysicsScience & Technology02 Physical Scienceshep-exPhysicsHigh Energy Physics::PhenomenologyT2K experimentFísicaSolar neutrino problemNeutrino detectorT2K CollaborationPhysical SciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinodescription
The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3$\sigma$ when compared to 4.92 $\pm$ 0.55 expected background events. In the PMNS mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles $\theta_{12}$, $\theta_{23}$, $\theta_{13}$, a mass difference $\Delta m^2_{32}$ and a CP violating phase $\delta_{\mathrm{CP}}$. In this neutrino oscillation scenario, assuming $|\Delta m^2_{32}| = 2.4 \times 10^{-3}$ $\rm eV^2$, $\sin^2 \theta_{23} = 0.5$, and $\Delta m^2_{32} >0$ ($\Delta m^2_{32} <0$), a best-fit value of $\sin^2 2 \theta_{13}$ = $0.140^{+0.038}_{-0.032}$ ($0.170^{+0.045}_{-0.037}$) is obtained at $\delta_{\mathrm{CP}}=0$. When combining the result with the current best knowledge of oscillation parameters including the world average value of $\theta_{13}$ from reactor experiments, some values of $\delta_{\mathrm{CP}}$ are disfavored at the 90% CL.
year | journal | country | edition | language |
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2014-02-10 |