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First Data from Daya Bay: Closing in on a Neutrino Mystery

Berkeley Lab researchers are leaders in an international effort to close in on neutrino mass

August 15, 2011
Paul Preuss 510-486-6249  paul_preuss@lbl.gov
News Release
The Daya Bay Reactor Neutrino Experiment captures faint flashes of light that indicate antineutrino interactions in detectors filled with scintillator fluids. Each detectors is lined with photomultiplier tubes. Two detectors have begun collecting data, two more have been completed, and four are under construction. (Photo by Roy Kaltschmidt, Berkeley Lab Public Affairs)

The Daya Bay Reactor Neutrino Experiment captures faint flashes of light that indicate antineutrino interactions in detectors filled with scintillator fluids. Each detector is lined with photomultiplier tubes. Two detectors have begun collecting data, two more have been completed, and four are under construction. (Photo by Roy Kaltschmidt, Berkeley Lab Public Affairs)

Some of the most intriguing questions in basic physics focus on neutrinos. How much do the different kinds weigh and which is the heaviest? The answers lie in how the three “flavors” of neutrinos – electron, muon, and tau neutrinos – oscillate or mix, changing from one to another as they race virtually without interruption through unbounded reaches of matter and space.

Three mathematical terms known as “mixing angles” described the process, and the Daya Bay Reactor Neutrino Experiment has just begun taking data to establish the last, least-known mixing angle to unprecedented precision. China and the United States lead the international Daya Bay Collaboration, including participants from Russia, the Czech Republic, Hong Kong, and Taiwan. U.S. participation is led by the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab).

The last elusive mixing angle is dubbed θ13 (theta one-three) and holds clues to how electrons and their cousins, muons and tau particles, were born in the moments after the big bang. Knowing θ13 could explain why there is more matter than antimatter in the universe – and indeed why there is any matter at all.

“The first data from Daya Bay set us on a path to precision that’s an order of magnitude better than present measurements and much more precise than other experiments now in progress,” says Daya Bay co-spokesperson Kam-Biu Luk of Berkeley Lab’s Physics Division, a professor of physics at the University of California at Berkeley. “We’ll measure the amplitude of the oscillation due to the least-known mixing angle to within one percent. The results will be a major contribution to understanding the role of neutrinos in the evolution of basic kinds of matter in the earliest moments after the big bang.”

Data for the Daya Bay Experiment will be collected by eight large detectors buried deep underground in the mountains adjacent to the six powerful nuclear reactors of the China Guangdong Nuclear Power Group in southern China, not far from Hong Kong. Nuclear reactors produce enormous quantities of antineutrinos (which in most vital respects are identical to neutrinos), and the reactors at Daya Bay yield millions of quadrillions of them every second.

Three experimental halls house the detectors, which will measure mixing angle θ13 by comparing the flux and energy distribution of interactions in the pairs of detectors in Halls 1 and 2, each about half a kilometer from the nearest reactors, with the four detectors in Hall 3, which is about two kilometers from the reactors. The very first data are now being recorded in Hall 1.

The first detectors now taking data are housed in the experimental hall nearest the two Daya Bay reactors, shown here as the water pool in which the detectors are submerged had been completely filled and before the pool was covered with a sliding roof, instrumented to identify incoming energetic cosmic rays.  (Photo by Joseph Y.K. Hor)

The detectors now taking data are housed in the experimental hall nearest the two Daya Bay reactors, shown as the water pool in which they are submerged had been completely filled and before the pool was covered with a sliding roof, instrumented to identify incoming cosmic rays. (Photo by Joseph Y.K. Hor)

The detectors are filled with liquid scintillator, lined with photomultiplier tubes, and shielded from cosmic rays and other background noise. They pinpoint antineutrino interactions by their faint flashes of blue light inside the vessels. Such interactions are exceedingly rare. Somewhat over a thousand a day will be caught by the near detectors, and only a few hundred a day by the far detectors.

“To achieve our one-percent goal, the differences in sensitivity among all eight detectors must be almost imperceptible, to within four-tenths of a percent of one another,” says William Edwards of Berkeley Lab’s Physics Division, Daya Bay’s U.S. Project and Operations Manager. “Although all data will contribute to the measurement, initial data-taking will be aimed at understanding the systematics of the antineutrino detectors in Hall 1 – basically to find out how identical they are.”

Hall 2, the other near hall, is expected to begin taking data this fall. As more data flows in, the upper limit on the value of the θ13 measurement will continue to trend lower.

“When the Far Hall comes on line next summer,” says Edwards, “the limit will drop like a rock. We’ll achieve a sensitivity on the measurement that is not possible with any other detector now planned or under construction.”

From two to three years of data collection with all eight detectors will be needed to meet the goal of measuring the oscillation amplitude of θ13 to within one percent. It’s a sensitivity not expected to be surpassed for a long time to come.

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At its inception the Daya Bay Experiment broke new ground as the first equal partnership between the U.S. and China on a major high-energy physics project, leveraging monetary support, technical expertise, and intellectual contributions from over 40 institutions in collaborating countries around the world. Initial U.S. participation was guided by James Siegrist, Associate Laboratory Director for General Sciences at Berkeley Lab and Director of the Physics Division.

Other current and former Berkeley Lab members of the Daya Bay Collaboration include Kam-Biu Luk, Bill Edwards, Mike Barry, Ken Chow, Matt Hoff, Jason Lee, Nanyang Li, Cheng-Ju Lin, Sa Liu, John Joseph, Yasuhiro Nakajima, Pedro Ochoa, Simon Patton, Patrick Tsang, Herb Steiner, Mary Stuart, Craig E. Tull, Steve Virostek, Mike Wingert, and Weili Zhong.

For more on the first neutrino data collected at Daya Bay, see the Daya Bay Collaboration news release on the Interactions.org site, at http://www.interactions.org/cms/?pid=1030972. More about Daya Bay is at http://newscenter.lbl.gov/feature-stories/2011/07/27/daya-bay-brink/.

U.S. participation in the Daya Bay Reactor Neutrino Experiment is supported by the U.S. Department of Energy’s Office of Science. The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, and is working to address some of the most pressing challenges of our time. For more information, please visit http://science.energy.gov.

Lawrence Berkeley National Laboratory addresses the world’s most urgent scientific challenges by advancing sustainable energy, protecting human health, creating new materials, and revealing the origin and fate of the universe. Founded in 1931, Berkeley Lab’s scientific expertise has been recognized with 12 Nobel prizes. The University of California manages Berkeley Lab for the U.S. Department of Energy’s Office of Science. For more, visit www.lbl.gov.


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