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Objective
Measure the neutrino mixing angle θ₁₃ through short-baseline reactor antineutrino disappearance, using functionally identical near and far detectors to cancel flux and detection systematics.
Method
Six 20-ton gadolinium-loaded liquid-scintillator detectors deployed in three underground experimental halls (two near halls at ~400–500 m, one far hall at ~1,600 m) near six reactor cores with combined thermal power of 17.4 GW. Inverse beta decay events tagged by delayed neutron capture on gadolinium produce a sharp 8 MeV gamma cascade.
Key results
- 2012: definitive first measurement of θ₁₃ with sin²2θ₁₃ = 0.092 ± 0.017 at 5.2σ — the last major PMNS mixing angle to be established as non-zero.
- Final precision result: sin²2θ₁₃ ≈ 0.0856 ± 0.0029 (2022), the most precise measurement of this angle.
- Precise Δm²₃₁ measurement from reactor channel, complementing long-baseline accelerator determinations.
- Upper limits on eV-scale sterile neutrino mixing in the relevant parameter space.
Significance
Daya Bay's 2012 result established the last of the three mixing angles as non-zero, enabling CP-violation searches in long-baseline neutrino experiments. The near/far identical-detector design became the template for subsequent reactor-oscillation measurements including the short-baseline sterile searches and the planned long-baseline JUNO.
Site and configuration
The Daya Bay complex comprises six reactor cores at three sites in coastal Guangdong province, with combined thermal power of 17.4 GW — among the largest reactor neutrino sources in the world. The experimental halls were excavated into granite hillsides, with three underground halls placed at carefully optimized baselines:
- EH1: 362 m from two Daya Bay cores
- EH2: 500 m from the two Ling Ao cores
- EH3 (far): 1,579 m from the Daya Bay and 1,912 m from Ling Ao cores
Six antineutrino detectors were distributed among the halls, with two detectors per hall at EH1 and EH2 and four at the far hall. The near-hall placement samples the essentially-unoscillated reactor flux and is used as a reference against the far-hall deficit.
Detector design
Each antineutrino detector is a three-zone concentric structure:
- Inner 20-ton target: 0.1% gadolinium-loaded linear-alkylbenzene scintillator
- Middle gamma catcher: unloaded scintillator
- Outer buffer: mineral oil
192 8-inch photomultipliers view the inner volumes. A muon system of water Cherenkov and RPC layers vetoes cosmic-ray events.
Gadolinium loading gives the delayed-coincidence signal a sharper time and energy profile: neutron capture on Gd releases ~8 MeV of gamma energy within ~30 μs of the prompt positron signal, well above the natural radioactive background.
The six detectors were built to be identical within tight tolerances (mass, fiducialization, photomultiplier response) so that near-to-far ratios cancel systematic uncertainties in reactor flux modeling, detection efficiency, and cross-section.
Results
The first result (2012) measured at 5.2σ significance from 55 days of data.
Subsequent data releases refined the measurement with additional exposure and systematic improvements. The final 2022 result is corresponding to . This is the best-measured of the three neutrino mixing angles.
Daya Bay also published a precision reactor antineutrino spectrum, confirming the well-known “5 MeV bump” in the energy distribution and constraining reactor-flux evolution models.
Shutdown and legacy
Daya Bay ceased operations in December 2020 after nine years of running. The infrastructure remains in place; some detector components have been repurposed for the PROSPECT-II short-baseline experiment at Oak Ridge.
The reactor- measurement — along with RENO (Korea) and Double Chooz (France) — anchors the global PMNS determination. Long-baseline accelerator experiments (T2K, NOvA) use Daya Bay’s value as an external input when extracting , effectively breaking what would otherwise be a degeneracy.
Significance
Daya Bay demonstrated that reactor neutrinos, with their clean flavor content and well-characterized spectrum, can compete with accelerator experiments for high-precision oscillation measurements. JUNO inherits this tradition at a longer baseline and larger detector mass for the mass-ordering determination.