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This book is based on the author's work in the T2K long-baseline neutrino oscillation experiment, in which neutrinos are generated by a proton beam and are detected by near and far neutrino detectors. In order to achieve the precise measurement of the neutrino oscillation, an accurate understanding of the neutrino beam and the neutrino interaction is essential. Thus, the author measured the neutrino beam properties and the neutrino interaction cross sections using a near neutrino detector called INGRID and promoted a better understanding of them. Then, the author performed a neutrino oscillation analysis using the neutrino beam and neutrino interaction models verified by the INGRID measurements. As a result, some values of the neutrino CP phase are disfavored at the 90% confidence level. If the measurement precision is further improved, we may be able to discover the finite CP phase which involves the CP violation. Thus, this result is an important step towards the discovery of CP violation in the lepton sector, which may be the key to understanding the origin of the matter–antimatter asymmetry in the universe.
This dissertation describes a measurement of the neutrino oscillation parameters $Delta m2̂_{21}$, $theta_{12}$ and constraints on $theta_{13}$ based on a study of reactor antineutrinos at a baseline of $sim 180,$km with the KamLAND detector. The data presented here was collected between April 2002 and November 2009, and amounts to a total exposure of $2.64 \pm 0.07 times 10{̂32}$ proton-years. For this exposure we expect $2140 \pm 74 (syst)$ antineutrino candidates from reactors, assuming standard model neutrino behavior, and $350 pm 88 (syst)$ candidates from background. The number observed is 1614. The ratio of background-subtracted candidates observed to expected is $$frac{N_{Obs}-N_{Bkg}}{N_{Exp}} = 0.59 \pm 0.02 (stat)\pm 0.045 (syst)nonumber$$ which confirms reactor neutrino disappearance at greater than 5$sigma$ significance. Interpreting this deficit as being due to neutrino oscillation, the best-fit oscillation parameters from a three-flavor analysis are $Delta m{̂2}_{21} = 7.60 {̂+0.20}_{-0.19} times 10{̂-5} rm{eV2̂}$, mbox{$theta_{12} = 32.5 \pm 2.9$ degrees} and $sin{̂2}theta_{13} = 0.025 {̂+0.035}_{-0.035}$, the 95% confidence-level upper limit on $sin{̂2}theta_{13}$ is mbox{$sin{̂2}theta_{13}
The aim of this workshop was to put together the efforts from various fields necessary for understanding neutrino oscillations in detail, from both experimental and theoretical points of view. One of the main experimental issues was to understand the absolute flux of both the atmospheric and the solar neutrinos in order to obtain detailed parameter information on neutrino oscillations.The proceedings contain many discussions on phenomenology and theories about neutrino mass and oscillations. The topics include: solar neutrino oscillations; neutrino mixing and the neutrino mass matrices; the origin of the neutrino masses; long baseline neutrino oscillation experiments; KamLAND and low energy neutrino measurements. Related subjects such as μ-eγ experiments and proton decay are also discussed.
This dissertation describes a measurement of the neutrino oscillation parameters m2 21, [theta]12 and constraints on [theta]13 based on a study of reactor antineutrinos at a baseline of ~ 180 km with the KamLAND detector. The data presented here was collected between April 2002 and November 2009, and amounts to a total exposure of 2.64 ± 0.07 × 1032 proton-years. For this exposure we expect 2140 ± 74(syst) antineutrino candidates from reactors, assuming standard model neutrino behavior, and 350±88(syst) candidates from background. The number observed is 1614. The ratio of background-subtracted candidates observed to expected is (NObs - NBkg)/ (NExp) = 0.59 ± 0.02(stat) ± 0.045(syst) which confirms reactor neutrino disappearance at greater than 5[sigma] significance. Interpreting this deficit as being due to neutrino oscillation, the best-fit oscillation parameters from a three-flavor analysis are m2 21= 7.60+0.20 -0.19×10-5eV2, [theta]12 = 32.5 ± 2.9 degrees and sin2 [theta]13 = 0.025+0.035 -0.035, the 95% confidence-level upper limit on sin2 [theta]13 is sin2 [theta]13
Between Apr. 2002 and May 2006 KamLAND measured the electron antineutrino flux at the Kamioka mine (2700 m.w.e.) in Japan. The nue sources were 19 Japanese nuclear reactor facilities at distances of 87 km to 830 km. Antineutrinos were detected by inverse beta decay, nue + p → e+ + n; detection of a positron and neutron pair constituted a neutrino signal. 1 kton of liquid scintillator served as both target and detector; the total exposure was 4.14 x 1034 proton days. In 1179.3 days of detector livetime, 550 antineutrino interactions were detected above a 3.4 MeV threshold, with an estimated 55 +/- 18 from backgrounds. The number, spectrum, and time of the nu e signals support neutrino flavor oscillation with Dm212 = (7.72 +/- 0.24) x 105 eV 2 and tan2theta12 = 0.48 +/- 0.12, in the Large Mixing Angle region. Assuming CPT invariance, KamLAND and solar neutrino results combined give Dm212 = (7.71 +/- 0.25) x 105 eV 2 and tan2theta12 = 0.49 +/- 0.05.
This thesis reports the calculation of neutrino production for the T2K experiment; the most precise a priori estimate of neutrino production that has been achieved for any accelerator-based neutrino oscillation experiment to date. The production of intense neutrino beams at accelerator facilities requires exceptional understanding of chains of particle interactions initiated within extended targets. In this thesis, the calculation of neutrino production for T2K has been improved by using measurements of particle production from a T2K replica target, taken by the NA61/SHINE experiment. This enabled the reduction of the neutrino production uncertainty to the level of 5%, which will have a significant impact on neutrino oscillation and interaction measurements by T2K in the coming years. In addition to presenting the revised flux calculation methodology in an accessible format, this thesis also reports a joint T2K measurement of muon neutrino and antineutrino disappearance, and the accompanying electron neutrino and antineutrino appearance, with the updated beam constraint.