6533b7d3fe1ef96bd1260964

RESEARCH PRODUCT

Journal of High Energy Physics

G. MentionR. SvobodaT. KawasakiP. NovellaJ. DhoogheN. VassilopoulosAmanda PortaD. KrynZelimir DjurcicN. WalshJ. ReichenbacherJ. M. López-castañoH. De KerretH. H. Trinh ThiR. MilincicR. MilincicYuri KamyshkovMuriel FallotJ. MartinoA. CucoanesS. ShimojimaA.c. SchilithzP.-j. ChangA. OnillonL. B. BezrukovI. BekmanJ.v. DawsonG. A. Horton-smithM. FrankeAnatael CabreraR. CarrA. StükenS. M. FernandesK. CrumFlorian KaetherE. BlucherJ. I. Crespo-anadónY. NikitenkoT. SumiyoshiS. PerassoA. MinottiAlain LetourneauJ. FeldeJ. FeldeD. FrancoMarcos CerradaM. ElnimrV. V. SinevEric BaussanMarcos DracosDavid LhuillierErnesto KempL. CamilleriE. DamonR. SharankovaV. FischerJ. MaricicJ. MaricicManfred LindnerJ. C. Dos AnjosAntoine CollinD. ShresthaM. ObolenskyR. SantorelliLuis GonzálezCécile JolletB. ReinholdE. ConoverM. BergevinYoshio AbeL. N. KalousisT.j.c. BezerraS. LuchtS. RothJ. M. LoseccoAnselmo MeregagliaJ. SpitzLothar OberauerDaniel M. KaplanC. PalomaresA. StahlY. SakamotoI. Gil-botellaV. ZimmerC. GrantC. VeyssiereTobias LachenmaierV. SibilleS. V. SukhotinE. SmithH. P. LimaA. OsbornM. KuzeN. HaagChristian BuckB. RyboltR. RoncinJ. C. BarriereJ. BusenitzYing SunYing SunC. MarianiA. HourlierLydie GiotM. RöhlingJosef JochumJunpei MaedaJunpei MaedaL. GoodenoughF. Von FeilitzschD. DietrichMichael HofmannStefan WagnerMatthew L StraitJanet ConradT. HaraA. TonazzoM. Göger-neffKazuhiro TeraoChristopher WiebuschYasushi NagasakaG. A. ValdiviessoS. SchönertM. C. GoodmanT. MileticF. YermiaI. M. PepeP. ChimentiG. PronostP. PfahlerC. E. LaneT. MatsubaraE. ChauveauM. H. ShaevitzE. CadenMasaki IshitsukaLindley WinslowStefan SchoppmannJ. HaserM. VivierM. D. SkorokhvatovMichael WurmMichael WurmH. WatanabeG. YangG. YangBayarto LubsandorzhievThierry LasserreThierry LasserreF. SuekaneL.f.f. StokesA.v. EtenkoI. StancuH. Furuta

subject

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics - Instrumentation and DetectorsNeutrino Detectors and TelescopeFOS: Physical sciencesCHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)ExperimentDistortion0103 physical sciencesEnergy spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsMixing (physics)PhysicsNeutrino Detectors and Telescopes010308 nuclear & particles physicsOscillationPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorFunction (mathematics)Instrumentation and Detectors (physics.ins-det)OscillationNeutrinoInstrumentation and Detectors

description

The Double Chooz experiment presents improved measurements of the neutrino mixing angle $\theta_{13}$ using the data collected in 467.90 live days from a detector positioned at an average distance of 1050 m from two reactor cores at the Chooz nuclear power plant. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties with respect to previous publications, whereas the efficiency of the $\bar\nu_{e}$ signal has increased. The value of $\theta_{13}$ is measured to be $\sin^{2}2\theta_{13} = 0.090 ^{+0.032}_{-0.029}$ from a fit to the observed energy spectrum. Deviations from the reactor $\bar\nu_{e}$ prediction observed above a prompt signal energy of 4 MeV and possible explanations are also reported. A consistent value of $\theta_{13}$ is obtained from a fit to the observed rate as a function of the reactor power independently of the spectrum shape and background estimation, demonstrating the robustness of the $\theta_{13}$ measurement despite the observed distortion.

10.1007/jhep10(2014)086https://hdl.handle.net/11858/00-001M-0000-0025-049D-611858/00-001M-0000-0025-049F-2