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Physical Review Letters· 2012Q1

Indication of Reactor<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mover accent="true"><mml:mi>ν</mml:mi><mml:mo>¯</mml:mo></mml:mover><mml:mi>e</mml:mi></mml:msub></mml:math>Disappearance in the Double Chooz Experiment

Yoshihisa Abe, Christoph Aberle, T. Akiri, J. C. dos Anjos et al.

Short summary

The Double Chooz experiment observed a 5.6% deficit in reactor electron antineutrinos, indicating neutrino oscillations and providing the first evidence for a non-zero value of the neutrino mixing parameter sin²2θ₁₃.

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Key points

  • Observed 5.6% fewer reactor electron antineutrinos than predicted.
  • The observed-to-predicted event ratio was 0.944 ± 0.016 (stat) ± 0.040 (syst).
  • This deficit is consistent with neutrino oscillations.
  • Provides evidence for a non-zero neutrino mixing parameter sin²2θ₁₃, measured as 0.086 ± 0.041 (stat) ± 0.030 (syst).

AI-generated from the title and abstract; the full text is not read.

Abstract

The Double Chooz experiment presents an indication of reactor electron antineutrino disappearance consistent with neutrino oscillations. An observed-to-predicted ratio of events of $0.944\ifmmode\pm\else\textpm\fi{}0.016(\mathrm{stat})\ifmmode\pm\else\textpm\fi{}0.040(\mathrm{syst})$ was obtained in 101 days of running at the Chooz nuclear power plant in France, with two $4.25\text{ }\text{ }{\mathrm{GW}}_{\mathrm{th}}$ reactors. The results were obtained from a single $10\text{ }\text{ }{\mathrm{m}}^{3}$ fiducial volume detector located 1050 m from the two reactor cores. The reactor antineutrino flux prediction used the Bugey4 flux measurement after correction for differences in core composition. The deficit can be interpreted as an indication of a nonzero value of the still unmeasured neutrino mixing parameter ${sin}^{2}2{\ensuremath{\theta}}_{13}$. Analyzing both the rate of the prompt positrons and their energy spectrum, we find ${sin}^{2}2{\ensuremath{\theta}}_{13}=0.086\ifmmode\pm\else\textpm\fi{}0.041(\mathrm{stat})\ifmmode\pm\else\textpm\fi{}0.030(\mathrm{syst})$, or, at 90% C.L., $0.017&lt;{sin}^{2}2{\ensuremath{\theta}}_{13}&lt;0.16$.

The authors' abstract, as published at the source. Physical Review Letters, 2012 · DOI ↗

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Field: Nuclear and High Energy Physics

Nuclear and High Energy PhysicsPhysics and Astronomy