Precision Measurement of Neutrino Oscillation Parameters with KamLAND

Abstract

The KamLAND experiment has determined a precise value for the neutrino oscillation parameter $\Delta m_{21}^2$ and stringent constraints on ${\theta }_{12}$. The exposure to nuclear reactor anti-neutrinos is increased almost fourfold over previous results to 2.44$\times 10^{32}$ proton-yr due to longer livetime and an enlarged fiducial volume. An undistorted reactor ${\bar{\nu }}_e$ energy spectrum is now rejected at >5$\sigma$. Extending the analysis down to the inverse beta decay energy threshold, and incorporating geo-neutrinos, gives a best-fit at $\Delta m_{21}^2$= $7.58_{-0.13}^{+0.14}(stat{)}_{-0.15}^{+0.15}(syst)\times 10^{-5}$ eV${}^2$ and ${\tan }^2{\theta }_{12}$=$0.56_{0.07}^{+0.10}(stat{)}_{-0.06}^{+0.10}(syst)$. Local $\Delta {\chi }^2$-minima at higher and lower $\Delta m_{21}^2$ are disfavored at >4$\sigma$. Combining with solar neutrino data, we obtain $\Delta m_{21}^2$= $7.59_{-0.21}^{+0.21}\times 10^{-5}$ eV${}^2$ and ${\tan }^2{\theta }_{12}$=$0.47_{-0.05}^{+0.06}$.

Version as published in PRL. Revised Fig. 2 (allowed contours) due to an error in the figure generating code (numbers or conclusions did not change). The full dChi2-map for this analysis is available at http://www.awa.tohoku.ac.jp/KamLAND/chi2map_3rdresult/chi2map.html . Fig. 3 (low E spectrum) was dropped due to space limitations

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• Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector
• Phases of Flavor Neutrino Masses and CP Violation
• Lepton flavor violation in SUSY left-right symmetric theories
• Neutrino flavor oscillations inside matter in conformal coupling models
• Neutrino spin-flavor oscillations in solar environment
• A Model of Neutrino Anomalies and IceCube data
• Relation between CPT Violation in Neutrino masses and mixings
• An infrared origin of leptonic mixing and its test at DeepCore
• New Signal of Atmospheric Tau Neutrino Appearance: Sub-GeV Neutral-Current Interactions in JUNO
• On the origin of the discrepancy between the expected and observed results at KamLAND
• Solar dynamo as host power pacemaker of the Earth global climate
• CP-violation reach of an electron capture neutrino beam
• Dark matter for Majorana neutrinos in a ${\mathbb{Z}}_4$ symmetry
• Mass Hierarchy Determination for ${\theta }_{13}=0$ and Atmospheric Neutrinos
• Neutrino Mass Matrix Related to Up-Quark Masses and Nearly Tribimaximal Mixing -- Based on a Yukawaon model --
• Phenomenology of neutrino mixing in vacuum and matter
• Current status of the T2K experiment
• Supernova neutrino signals by liquid Argon detector and neutrino magnetic moment
• How can CP violation in the neutrino sector be large in a $2\leftrightarrow 3$ symmetric model?
• Supernovae as laboratories for neutrino properties
• Solar neutrino results from Borexino and main future perspectives
• Combining Neutrino Oscillation Experiments with the Feldman-Cousins Method
• The replacement system of the JUNO liquid scintillator pilot experiment at Daya Bay
• A $\nu$ look at the Sun: Probing the conditions of the solar core using ${}^8$B neutrinos
• Laboratory Studies on the Removal of Radon-Born Lead from KamLAND's Organic Liquid Scintillator
• Running of Oscillation Parameters in Matter with Flavor-Diagonal Non-Standard Interactions of the Neutrino
• Enhancing the Sensitivity to Seesaw Predictions in Gauged $B-L$ Scenarios
• Liquid-organic time projection chamber for detecting low energy antineutrinos
• Constraining sterile neutrinos with a low energy beta-beam
• Universal Mass Matrix and Leptonic ${\theta }_{13}$ Angle
• Testing Geological Models with Terrestrial Antineutrino Flux Measurements
• A new scheme for short baseline electron antineutrino disappearance study
• The IsoDAR High Intensity H${}_2^{+}$ Transport and Injection Tests
• Advanced One-Parameter CKM Mixing Matrix and Universal Deviation from Exact Quark-Lepton Complementarity
• Uncertainties in the Anti-neutrino Production at Nuclear Reactors
• Simulated neutrino signals of low and intermediate energy neutrinos on Cd detectors
• Probing Extra Dimensions with Neutrino Oscillations
• KamLAND's search for correlated low-energy electron antineutrinos with astrophysical neutrinos from IceCube
• Electroweak right-handed neutrinos and new signals at the LHC
• Neutrino oscillation in the presence of background classical sources
• Review of Reactor Antineutrino Experiments
• Probing the equation of state of neutron stars using neutrino oscillations
• Status and Perspectives of Neutrino Physics
• Vetoing Cosmogenic Muons in A Large Liquid Scintillator
• Towards First Detection of the Solar MSW Transition With JUNO
• Radiative neutrino masses: A window to new physics
• Roads for Right-handed Neutrino Dark Matter: Fast Expansion, Standard Freeze-out, and Early Matter Domination
• Geometric gravitational origin of neutrino oscillations and mass-energy
• Search for Sterile Neutrinos with CUPID-0
• Symmetric teleparallel gravitational effects on solar neutrino oscillations
• Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Dark Matter Phenomenology: Sterile Neutrino Portal and Gravitational Portal in Extra-Dimensions
• Fine tuning in an A4-based Tri-Bimaximal neutrino-mixing model
• Lepton Flavor Violation of Z Gauge Boson Decays in Supersymmetric Type-III Seesaw Model
• Minimal structure for neutrino mass matrix
• Could Geoneutrinos Interact With the Geomagnetic Field?
• Lepton flavour violating stau decays versus seesaw parameters: correlations and expected number of events for both seesaw type-I and II
• The Sensitivity of SNO+ to $\Delta m_{12}^2$ Using Reactor Anti-neutrino Data
• Geo-Neutrinos
• Low-energy neutrinos
• Are Neutrino Oscillations a Non-stationary Phenomenon?
• The leptonic CP phase is determined by an equation involving the PMNS matrix elements
• Massive Majorana neutrinos in matter and a magnetic field
• Pion productions by proton and Helium-3 on Au197 target at beam energies of 2.8, 5, 10 and 16.587 GeV/nucleon