For more information, contact:
Pete Genzer, 631 344-3174, or
Mona S. Rowe, 631 344-5056
June 18, 2001

First Results from the Sudbury Neutrino Observatory Explain Missing Solar Neutrinos and Reveal New Neutrino Properties

UPTON, NY - Physicists from Canada, the U.K., and the U.S. are today announcing that their first results provide a solution to a 30-year old mystery - the puzzle of the missing solar neutrinos. The Sudbury Neutrino Observatory (SNO) finds that the solution lies not with the Sun, but with the neutrinos, which change as they travel from the core of the Sun to the Earth. 

Neutrinos are elementary particles of matter with no electric charge and very little mass. There are three types: the electron-neutrino, the muon-neutrino and the tau-neutrino. Electron-neutrinos, which are associated with the familiar electron, are emitted in vast numbers by the nuclear reactions that fuel the Sun. Since the early 1970s, several experiments have detected neutrinos arriving on Earth, but they have found only a fraction of the number expected from detailed theories of energy production in the Sun. This meant there was something wrong with either the theories of the Sun, or the understanding of neutrinos.

"We now have high confidence that the discrepancy is not caused by problems with the models of the Sun but by changes in the neutrinos themselves as they travel from the core of the Sun to the earth," says Dr. Art McDonald, SNO Project Director and Professor of Physics at Queen's University in Kingston, Ontario. "Earlier measurements had been unable to provide definitive results showing that this transformation from solar electron neutrinos to other types occurs. The new results from SNO, combined with previous work, now reveal this transformation clearly, and show that the total number of electron neutrinos produced in the Sun are just as predicted by detailed solar models."

The SNO scientists present their first results today in a paper submitted to Physical Review Letters and in presentations at the Canadian Association of Physicists Annual Conference at Victoria, B.C. and at SNO Institutions in the U.S. and the U.K. 

"It is exciting that the first fruits of our labors have turned out to be scientifically significant, after several years of intensive effort by more than 150 scientists to build this neutrino detector and get it operating," said Richard Hahn, head of the Solar Neutrino Group at Brookhaven National Laboratory, one of the collaborating institutions. "There is much more that we can do and plan to do in SNO over the next few years to continue to unravel the mysteries of the neutrino." Brookhaven's current role is in ensuring that the SNO's heavy water, a critical part of the neutrino detector, remains ultra-pure and is not affected by environmental factors.

Brookhaven's history of neutrino research dates to the 1950s, and in 1968, scientist Ray Davis's pioneering work in a South Dakota gold mine sent the neutrino world into an uproar by first documenting the missing electron neutrinos (more information).

"The determination that the electron neutrinos from the Sun transform into neutrinos of another type is very important for a full understanding of the Universe at the most microscopic level," said U.K. co-spokesman Prof. David Wark of the Rutherford/Appleton Laboratory and the University of Sussex. "This transformation of neutrino types is not allowed in the Standard Model of elementary particles. Theoreticians will be seeking the best way to incorporate this new information about neutrinos into more comprehensive theories. "

The direct evidence for solar neutrino transformation also indicates that neutrinos have mass. By combining this with information from previous measurements, it is possible to set an upper limit on the sum of the known neutrino masses. "Even though there is an enormous number of neutrinos in the universe, the mass limits show that neutrinos make up only a small fraction of the total mass and energy content of the universe," says Dr. Hamish Robertson, U.S. co-spokesman and Professor of Physics at the University of Washington in Seattle.

The SNO detector, which is located 2,000 meters below ground in INCO's Creighton nickel mine near Sudbury, Ontario, uses 1,000 tons of heavy water to intercept about 10 neutrinos per day. The results being reported today are the first in a series of sensitive measurements that SNO is performing. From this initial phase, the SNO scientists report on an accurate and specific measurement of the number of solar electron neutrinos reaching their detector by studying a reaction unique to heavy water where a neutron is changed into a proton. They combined these first SNO results with measurements by the SuperKamiokande detector in Japan of the scattering of solar neutrinos from electrons in ordinary water (offering a small sensitivity to other neutrino types), to provide the direct evidence that neutrinos oscillate, or change types, as they travel from the Sun. 

At the beginning of June, the SNO scientists began the next phase of their measurements by adding salt to the heavy water to study another neutrino reaction with deuterium that provides a large sensitivity to all neutrino types. Their further measurements can address the transformation of neutrino type with even greater sensitivity, and help scientists study other properties of neutrinos, the Sun and supernovae. 

Background Information On The Sudbury Neutrino Observatory 

The Sudbury Neutrino Observatory is a unique neutrino telescope, the size of a ten-story building, 2 kilometers underground in INCO's Creighton Mine near Sudbury, Ontario, which was planned, constructed, and operated by a 100-member team of scientists from Canada, the United States, and the United Kingdom. Through its use of heavy water, the SNO detector provides new ways to detect neutrinos from the Sun and other astrophysical objects and measure their properties. For many years, the number of solar neutrinos measured by other underground detectors has been found to be smaller than expected from theories of energy generation in the Sun. This has led scientists to infer that either the understanding of the Sun is incomplete, or that the neutrinos are changing from one type to another in transit from the core of the Sun. 

The SNO detector has the capability to determine whether solar neutrinos are changing their type en-route to Earth, thus providing answers to questions about neutrino properties and solar-energy generation. The SNO detector consists of 1,000 tons of ultra-pure heavy water enclosed in a 12-meter-diameter acrylic plastic vessel, which in turn is surrounded by ultra-pure ordinary water in a giant 22-meter-diameter by 34-meter-high cavity. Outside the acrylic vessel is a 17-meter-diameter geodesic sphere containing 9,456 light sensors or photomultiplier tubes, which detect tiny flashes of light emitted as neutrinos are stopped or scattered in the heavy water. The flashes are recorded and analyzed to extract information about the neutrinos causing them. At a detection rate on the order of 10 per day, many days of operation are required to provide sufficient data for a complete analysis. The laboratory includes electronics and computer facilities, a control room, and water purification systems for both heavy and regular water. 

The construction of the SNO Laboratory began in 1990 and was completed in 1998 at a cost of $73 million Canadian dollars with support from the Natural Sciences and Engineering Research Council of Canada, the National Research Council of Canada, the Northern Ontario Heritage Foundation, Industry, Science and Technology Canada, INCO Limited, the United States Department of Energy, and the Particle Physics and Astronomy Research Council of the UK. The heavy water is on loan from Canada's federal agency AECL with the cooperation of Ontario Power Generation, and the unique underground location is provided through the cooperation and support of INCO Limited. 

Measurements at the SNO Laboratory began in 1999, and the detector has been in almost continuous operation since November, 1999 when, after a period of calibration and testing, its operating parameters were set in their final configuration.

The URL for the SNO web site is

Solar neutrino research group at Brookhaven.

SNO Participating Institutions


Queen's University, Carleton University, Laurentian University,
University of Guelph, University of British Columbia, Chalk River
Laboratories (to 1996)

United States

Brookhaven National Laboratory, Lawrence Berkeley National
Laboratory, Los Alamos National Laboratory, University of
Pennsylvania, University of Washington, Princeton University (to 1992), University of California at Irvine (to 1989)

United Kingdom

Oxford University

For further information:

Prof. Art McDonald, Director
Sudbury Neutrino Observatory Institute
Queen's University
Kingston, Ontario
(613) 533 2702, Cell: (613) 541 1405
FAX (613) 533 6813; or
Sudbury Neutrino Observatory
Creighton Mine, Lively Ontario
(705) 692-7000
FAX (705) 692-7001

Prof. Doug Hallman
Director of Communications
Sudbury Neutrino Observatory
Laurentian University
Sudbury, Ontario
(705) 675-1151 Ext. 2231
FAX (705) 675-4868

Dr. Eugene Beier, U.S. Co-spokesman
University of Pennsylvania
Philadelphia, PA, USA (215) 898-5960
FAX (215) 898-8512

Dr. David Wark, U.K. Co-spokesman
RAL/University of Sussex
Sussex, UK
011 44 1 235 445094
FAX 011 44 1 235 446733


Paul de la Riva, media relations officer
Department of Public Affairs
Laurentian University
Sudbury, ON, Canada
(705) 673-6566
FAX (705) 675-4840

Anne Kershaw, Manager Public Affairs
Queen's University
Kingston, Ontario, Canada
(613) 533 6000 ext 74038
FAX (613) 533 6652

The U.S. Department of Energy's Brookhaven National Laboratory conducts research in the physical, biomedical, and environmental sciences, as well as in energy technologies. Brookhaven also builds and operates major facilities available to university, industrial, and government scientists. The Laboratory is operated by Brookhaven Science Associates, a partnership led by Stony Brook University and Battelle, a nonprofit applied science and technology organization.