English

Precision Measurement of Neutrino Oscillation Parameters with KamLAND

High Energy Physics - Experiment 2012-08-27 v3 Nuclear Experiment Geophysics

Abstract

The KamLAND experiment has determined a precise value for the neutrino oscillation parameter Δm212\Delta m^{2}_{21} and stringent constraints on θ12\theta_{12}. The exposure to nuclear reactor anti-neutrinos is increased almost fourfold over previous results to 2.44×1032\times10^{32} proton-yr due to longer livetime and an enlarged fiducial volume. An undistorted reactor νˉe\bar{\nu}_{e} energy spectrum is now rejected at >5σ\sigma. Extending the analysis down to the inverse beta decay energy threshold, and incorporating geo-neutrinos, gives a best-fit at Δm212\Delta m^{2}_{21}= 7.580.13+0.14(stat)0.15+0.15(syst)×1057.58^{+0.14}_{-0.13}(stat)^{+0.15}_{-0.15}(syst)\times10^{-5} eV2^{2} and tan2θ12\tan^2 \theta_{12}=0.560.07+0.10(stat)0.06+0.10(syst)0.56^{+0.10}_{0.07}(stat)^{+0.10}_{-0.06}(syst). Local Δχ2\Delta \chi^2-minima at higher and lower Δm212\Delta m^{2}_{21} are disfavored at >4σ\sigma. Combining with solar neutrino data, we obtain Δm212\Delta m^{2}_{21}= 7.590.21+0.21×1057.59^{+0.21}_{-0.21}\times10^{-5} eV2^{2} and tan2θ12\tan^2 \theta_{12}=0.470.05+0.060.47^{+0.06}_{-0.05}.

Keywords

Cite

@article{arxiv.0801.4589,
  title  = {Precision Measurement of Neutrino Oscillation Parameters with KamLAND},
  author = {The KamLAND Collaboration},
  journal= {arXiv preprint arXiv:0801.4589},
  year   = {2012}
}

Comments

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