Sudbury Neutrino Observatory Institute Creighton Mine Lively, Ontario, Canada For further information: Prof. Art McDonald, Queen's University Director, Sudbury Neutrino Observatory Institute Creighton Mine, Lively Ontario (705) 692-7000 or (613) 541-1405 FAX (705) 692-7001 mcdonald@sno.phy.queensu.ca Dr. Doug Hallman Director of Communications, Sudbury Neutrino Observatory Laurentian University (705) 675-1151 Ext. 2231 FAX (705) 675-4868 edh@nu.phys.laurentian.ca Dr. Eugene Beier U.S. Co-spokesman, University of Pennsylvania Philadelphia, PA, USA (215) 898-5960 FAX (215) 898-8512 geneb@hep.upenn.edu Dr. David Wark U.K. Co-spokesman, RAL/University of Sussex Sussex, UK 01 235 445094 FAX 01 235 446733 d.wark1@physics.ox.ac.uk NEWS RELEASE: April 20th 2002, 1:20 pm Eastern Daylight Time Sensitive measurement by SNO observes solar neutrinos in a new way A team of scientists from Canada, the United States and the United Kingdom today announced the results of a unique new measurement of the total number of neutrinos of all known types reaching the Earth from the Sun. Using data entirely from the Sudbury Neutrino Observatory (SNO) in Canada they are also able to determine that the observed number of electron neutrinos (the type produced by the Sun) is only a fraction of the total number. This shows with great certainty that neutrinos from the Sun change from one type to another before reaching the Earth. Says SNO Project Director Art McDonald of Queen's University, "These new results show in a clear, simple and accurate way that solar neutrinos change their type. The total number of neutrinos we observe is also in excellent agreement with calculations of the nuclear reactions powering the Sun. The SNO team is really excited because these measurements enable neutrino properties such as mass to be specified with much greater certainty for fundamental theories of elementary particles." Neutrinos are particles with no electric charge and very little mass. They are known to exist in three types related to three different charged particles -- the electron and its lesser known relatives the muon and the tau. The Sun emits electron-neutrinos, which are created in the thermonuclear reactions in the solar core. Previous experiments have found fewer electron-neutrinos than suggested by calculations based on how the Sun burns -- the famous "solar neutrino problem". SNO uses the unique properties of heavy water -- where the hydrogen has an extra neutron in its nucleus -- to detect not only electron-neutrinos through one type of reaction, but also all three known neutrino types through a different reaction. The results presented today at the Joint American Physical Society/ American Astronomical Society meetings in Albuquerque, New Mexico, show that the number of electron-neutrinos observed is only about one third of the total number reaching the Earth. This shows unambiguously that electron-neutrinos emitted by the Sun have changed to muon- or tau-neutrinos before they reach Earth. Dr. Andre Hamer of Los Alamos National Laboratory told the meeting, "In order to make these measurements, we had to restrict the radioactivity in the detector to minute levels and determine the background effects very accurately to show clearly that we are observing neutrinos from the Sun. The care taken throughout this experiment to minimize radioactivity and the careful calibration and analysis of our data has enabled us to make these neutrino measurements with great accuracy." In June 2001, results from the detection of electron-neutrinos in SNO first indicated, with a certainty of 99.9%, that neutrinos change type on their way from the Sun, thus solving the long-standing problem. However, these conclusions were based on comparisons of results from SNO with those from a different experiment, the Super-Kamiokande detector in Japan. The new results, obtained entirely from the SNO, are so accurate that it is 99.999% probable that solar neutrinos change type before reaching Earth. The results, which have been submitted to Physical Review Letters, are of great importance because the way in which the neutrinos -- long thought to be massless particles -- change types is thought to be linked to neutrino mass and mass differences between various neutrino types. Says Professor Hamish Robertson of the University of Washington, "It was a dramatic and exciting moment for us when we first saw the neutrons being produced by this type of neutrino interaction and realized there were three times as many as you would get if only electron neutrinos were coming from the Sun. There's absolutely no question the neutrino type changes and now we know quite precisely the mass differences between these particles." Further background information: http://www.sno.phy.queensu.ca/sno/background_info/ Reference: Paul de la Riva, media relations officer Public Affairs Department Laurentian University Sudbury, ON, Canada (705) 673-6566 FAX (705) 675-4840 www.laurentian.ca pdelariva@nickel.laurentian.ca Nancy Marrello Public Affairs Queen's University Kingston, ON, Canada (613) 533-6000, ext. 74040 www.queensu.ca marrello@post.queensu.ca SNO Participating Institutions: Canada * University of British Columbia (BC, Canada) * Carleton University (Ontario, Canada) * University of Guelph (Ontario, Canada) * Laurentian University (Ontario, Canada) * Queen's University (Ontario, Canada) * Chalk River Laboratories (participated until 1996) * National Research Council of Canada (participated until 1991) United States * Brookhaven National Laboratory (New York, USA) * Lawrence Berkeley National Laboratory (California, USA) * Los Alamos National Laboratory (New Mexico, USA) * University of Pennsylvania (Pennsylvania, USA) * University of Washington (Washington, USA) * University of California at Irvine (participated until 1989) * Princeton University (participated until 1992) United Kingdom * Oxford University (Oxford, UK) Funding for SNO * Natural Sciences and Engineering Research Council Canada * U.S. Department of Energy * U.K. Science and Engineering Research Council * National Research Council Canada * Northern Ontario Heritage Fund Corporation * Industry Canada * INCO Limited SNO Sponsors * INCO Limited * Atomic Energy of Canada Limited * Northern Telecom * Ontario Hydro / Ontario Power Generation * Sun Microsystems * Agra-Monenco/Canatom Limited * CVD Manufacturing Inc. SNO Prime Contractors and Suppliers * Agra-Monenco/Canatom Limited (Project Management and design) * INCO Limited (Cavity excavation and support systems) * Dynatec International (Civil construction) * Reynolds Polymer Technology Incorporated (Acrylic vessel) * Lawrence Berkeley National Laboratory (Photomultiplier support structure) * Hamamatsu Photonics (Photomultipliers) * Schott Glass Incorporated (Photomultiplier glass bulbs) * CVD Manufacturing Inc. (CVD nickel for neutral current detectors) * Mirotech Limited (CVD nickel for neutral current detectors)
