Daya Bay and RENO: how reactor experiments pinned down the last neutrino mixing angle

For more than a decade, the smallest neutrino mixing angle θ₁₃ was the most-wanted number in oscillation physics. In 2012, two reactor experiments — one in southern China, one in South Korea — independently nailed it within weeks of each other.

Conceptual rendering of a reactor antineutrino detector hall

By 2010, neutrino physicists knew almost everything they could know about the PMNS mixing matrix from the existing oscillation data — except one parameter. The mixing angle θ₁₃, which governs the strength of mixing between the first and third neutrino mass eigenstates, was experimentally consistent with zero. Several experiments had set upper limits on it, but no one had ever measured a non-zero value.

This mattered. θ₁₃ is the gateway parameter to CP violation in the neutrino sector. If θ₁₃ turns out to be zero, then CP-violation effects in neutrino oscillation are unobservable in practice — no asymmetry between the rates at which muon neutrinos turn into electron neutrinos versus the corresponding antineutrino conversions. If θ₁₃ is non-zero but small, the asymmetry is hard but doable. If θ₁₃ is non-zero and not too small, CP violation becomes accessible.

Two experiments — Daya Bay in southern China and RENO in South Korea — were both built specifically to measure θ₁₃ using reactor antineutrinos. Within four weeks of each other in early 2012, they announced their results. The answer was clear: θ₁₃ is comfortably non-zero, and the path to measuring CP violation was open.

Why reactors

A nuclear reactor produces an enormous flux of electron antineutrinos as a byproduct of the fission of uranium and plutonium isotopes. A typical commercial reactor emits roughly 6 × 10²⁰ antineutrinos per second, with energies of a few MeV. These antineutrinos pour through the detectors and the surrounding rock at all times the reactor is operating.

Reactor experiments measure neutrino disappearance: how many antineutrinos that should arrive at the detector actually do? If antineutrinos oscillate into other flavors during their trip, the count is reduced. By measuring the deficit, the experiment infers the oscillation parameters.

For measuring θ₁₃ specifically, the trick is to optimize the baseline length. Different oscillation effects dominate at different distances. θ₁₃-driven oscillation produces a clear deficit at a baseline of about 1.5 to 2 kilometers for typical reactor neutrino energies. Place a detector at that distance and compare its rate to one closer to the reactor — close enough that no oscillation has had time to develop — and the difference reveals θ₁₃.

The Daya Bay design

The Daya Bay complex sits about 60 kilometers from Hong Kong, hosting six commercial reactors at the Daya Bay and Ling Ao nuclear power plants. The experiment installed eight identical antineutrino detectors in three underground halls dug into the granite hills around the plants.

Two detectors were placed at the near halls, close (about 360-470 meters) to the reactors. Four detectors were placed at the far hall, about 1.6 kilometers away — exactly the optimal distance for θ₁₃ sensitivity. (Initially the experiment ran with fewer detectors and added the rest over the first year of operation.)

Each detector is a stack of three concentric volumes: an inner target of gadolinium-loaded liquid scintillator (20 tons), a buffer of pure scintillator, and an outer veto of mineral oil. The gadolinium-loading is the technical key: when an antineutrino undergoes inverse beta decay in the scintillator, the resulting neutron is captured by gadolinium within tens of microseconds, releasing a characteristic 8-MeV gamma signal that flags the event cleanly.

By having the same kind of detector both near and far from the reactors, Daya Bay could compare rates without needing to know the absolute reactor antineutrino flux to high precision. The flux uncertainty cancels in the ratio. Only the oscillation effect remains.

The March 2012 announcement

Daya Bay began full data-taking in late December 2011. By early March 2012, after just 55 days of running, the team had enough statistics to claim discovery.

The result, announced at a seminar on March 8, 2012 at the Institute of High Energy Physics in Beijing, was a 5.2σ detection of θ₁₃. The measured value was sin²(2θ₁₃) ≈ 0.092 — large enough that the deficit between the near and far detectors was unambiguous.

This was significantly above the upper limits set by previous experiments and meant that CP violation measurements would be experimentally feasible with the next generation of long-baseline experiments.

RENO’s independent confirmation

About four weeks later, on April 3, 2012, the RENO collaboration in South Korea announced a confirming measurement. RENO is built on similar principles — multiple identical detectors at near and far distances from the Yonggwang nuclear power complex on the country’s western coast. The far detector sits about 1.4 kilometers from the reactor cores.

RENO’s result, sin²(2θ₁₃) ≈ 0.113, agreed with Daya Bay within errors. The independent confirmation, from an entirely separate detector designed by an entirely separate team, gave the field high confidence that θ₁₃ was real and not an artifact.

A third experiment — Double Chooz in France — had also seen hints of non-zero θ₁₃ but with less statistical power. Its eventual result was consistent with Daya Bay and RENO.

What it enabled

The non-zero value of θ₁₃ at the magnitude Daya Bay and RENO measured is the reason the current generation of CP-violation experiments — T2K and NOvA — exists, and the reason the next generation — DUNE and Hyper-Kamiokande — is being built.

Each of these experiments works by sending a beam of muon neutrinos through hundreds of kilometers of Earth and looking for the resulting electron-neutrino appearance at the far end. The probability of that appearance depends on θ₁₃ (which sets the size of the effect), the mass ordering, and the CP-violating phase δ_CP (which makes neutrinos and antineutrinos behave slightly differently). With θ₁₃ measured to high precision, the long-baseline experiments can focus on extracting the remaining unknowns.

In a real sense, Daya Bay and RENO opened the door to the era of precision CP-violation measurement in the neutrino sector. Without them, the strategy for the next generation of experiments would be very different.

A reactor antineutrino mystery

In the years since the θ₁₃ discovery, reactor antineutrino experiments have also turned up an unexpected puzzle: the reactor antineutrino anomaly. The total measured rate of antineutrinos from reactors, when compared against updated calculations of the expected flux, is consistently lower by a few percent — particularly in the 5 MeV energy region, where there is also an unexplained shape distortion (“the 5 MeV bump”).

The anomaly has multiple possible explanations. One is the existence of a sterile neutrino with mass around 1 eV, into which the reactor antineutrinos partially oscillate at short baselines. Another is that the predicted antineutrino spectrum from reactor fuel was miscalculated. Experiments — including very-short-baseline reactor experiments like PROSPECT in the US and STEREO in France — are still working to resolve which explanation is correct.

What the reactor program looks like next

Daya Bay completed its data-taking in December 2020 and is publishing legacy results. Its final θ₁₃ measurement is among the most precise oscillation parameters known.

The future of reactor neutrino physics now centers on JUNO, the 20,000-ton liquid scintillator detector currently being commissioned in southern China. JUNO sits 53 kilometers from a cluster of reactor cores — exactly the right baseline to measure the mass ordering through the fine structure of the oscillation pattern. Together with DUNE and Hyper-K, JUNO will close out the remaining unknowns in the PMNS matrix during the next decade.

The smallest number that mattered

Daya Bay and RENO’s measurement of θ₁₃ was, in some sense, a quiet result. There was no immediate Nobel Prize. There was no public splash. But within the field, it was understood immediately to be the kind of breakthrough that opens whole new experimental programs.

θ₁₃ being non-zero is the reason DUNE and Hyper-K can hope to measure CP violation. It is the reason the next decade of neutrino physics has a clear roadmap. And it is the kind of result — clean, multiply confirmed, executed with modest detectors in two countries within weeks of each other — that exemplifies what experimental particle physics looks like when it works.


For the parameter that θ₁₃ opens the door to, see CP violation in the neutrino sector. For the experiments now using θ₁₃ to search for CP violation, see T2K, NOvA, DUNE, and Hyper-Kamiokande. For the reactor anomaly story, see Sterile neutrinos.

Further reading

Primary sources

Background and context

Frequently asked

What is θ₁₃ and why does it matter?

θ₁₃ is one of three mixing angles that describe how neutrino flavors mix with mass eigenstates in the PMNS matrix. For decades it was the smallest and least-known of the three. Its non-zero value is what enables CP violation to be detectable in neutrino oscillations — making it the gateway to measuring the CP-violating phase δ_CP.

How does a reactor neutrino experiment work?

Nuclear reactors produce intense fluxes of electron antineutrinos as byproducts of fission. Detectors placed at various distances from the reactor measure how many antineutrinos arrive. By comparing rates between near and far detectors, the experiments isolate the small oscillation deficit caused by θ₁₃, free from systematic uncertainties about the absolute neutrino flux.

Why were Daya Bay and RENO competing?

Both experiments were designed specifically to measure θ₁₃ and were under construction at the same time. They ended up announcing results within weeks of each other in March-April 2012. The independent confirmations strengthened the result enormously — neither could be dismissed as an artifact of one experiment's systematics.

What did Daya Bay actually find?

Daya Bay announced in March 2012 that the mixing angle θ₁₃ is non-zero at the 5.2σ level, with sin²(2θ₁₃) ≈ 0.092. This was the first definitive measurement of the smallest neutrino mixing angle. RENO's confirmation followed shortly after, and the result has since been refined to sin²(2θ₁₃) ≈ 0.085.

What enables CP violation studies because of θ₁₃?

CP violation in neutrino oscillations appears as a difference between the rates at which muon neutrinos turn into electron neutrinos versus the rates for the corresponding antineutrino transitions. That rate difference is proportional to sin(θ₁₃), so a non-zero θ₁₃ is required for the effect to be observable. Daya Bay and RENO showed θ₁₃ is large enough that CP-violation measurements are feasible.

Cite this article 5 formats

APA

Neutrino Times Editorial Team. (2025, October 7). Daya Bay and RENO: how reactor experiments pinned down the last neutrino mixing angle. Neutrino Times. https://neutrino-times.com/articles/daya-bay-reno-measuring-theta-13/

Chicago

Neutrino Times Editorial Team. "Daya Bay and RENO: how reactor experiments pinned down the last neutrino mixing angle." Neutrino Times, October 7, 2025. https://neutrino-times.com/articles/daya-bay-reno-measuring-theta-13/.

MLA

Neutrino Times Editorial Team. "Daya Bay and RENO: how reactor experiments pinned down the last neutrino mixing angle." Neutrino Times, 7 Oct. 2025, https://neutrino-times.com/articles/daya-bay-reno-measuring-theta-13/.

BibTeX

@misc{neutrino-times-daya-bay-reno-measuring-theta-13,
  author       = {Neutrino Times Editorial Team},
  title        = {Daya Bay and RENO: how reactor experiments pinned down the last neutrino mixing angle},
  howpublished = {Neutrino Times},
  year         = {2025},
  month        = {oct},
  url          = {https://neutrino-times.com/articles/daya-bay-reno-measuring-theta-13/},
  note         = {Accessed: 2025-10-07}
}

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