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    The Sudbury Neutrino Observatory (SNO) results have provided revolutionary insight into the properties of neutrinos and the core of the sun. The detector, shown in the artist's conception below, was built 6800 feet under ground, in INCO's Creighton mine near Sudbury, Ontario, Canada. SNO was a heavy-water Cherenkov detector designed to detect neutrinos produced by fusion reactions in the sun. It used 1000 tonnes of heavy water loaned from Atomic Energy of Canada Limited (AECL), and contained by a 12 meter diameter acrylic vessel. Neutrinos reacted with the heavy water (D2O) to produce flashes of light called Cherenkov radiation. This light was then detected by an array of 9600 photomultiplier tubes mounted on a geodesic support structure surrounding the heavy water vessel. The detector was immersed in light (normal) water within a 30 meter barrel-shaped cavity (the size of a 10 story building!) excavated from Norite rock. Located in the deepest part of the mine, the overburden of rock shielded the detector from cosmic rays. The detector laboratory, still functioning as part of the new SNOLAB facility, is extremely clean to reduce background signals from radioactive elements present in the mine dust which would otherwise hide the very weak signal from neutrinos. Plans are currently underway to upgrade the SNO detector for the new SNO+ experiment.

    The first co-spokesmen for the SNO collaboration when it was established in 1984 were Professor Herb Chen from U California, Irvine and Professor George Ewan, Queen¡¯s University. For interesting accounts of the early development work for the SNO experiment, please see:
    "Early Development of the Underground SNO Laboratory in Canada" and "The Funding Campaign for the Sudbury Neutrino Observatory", G.T. Ewan and W.F. Davidson, Physics in Canada, Vol. 61, No. 6 (2005), p. 339-346 and 347-350. (download in PDF format)
    For a review article summarizing the three phases of the SNO experiment, please see:
    "The Sudbury Neutrino Observatory", Nick Jelley, Arthur B. McDonald, and R.G. Hamish Robertson, Annu. Rev. Nucl. Part. Sci. 2009.59:431-465. (download in PDF format)
    Artist Concept of SNO

    Recent News

    In Memoriam: Andre Hamer 1968-2003

    Physics Documents

    SNO Web Pages on This Site

    SNO Web Sites at Participating Institutions

    Present Status

    Also see SNO Milestones for a history of SNO milestones

    The Sudbury Neutrino Observatory Institute (SNOI):

    SNO Project Director:

    Dr. A.B. McDonald (Queen's University)
    The Sudbury Neutrino Observatory Institute

    Department of Physics, Stirling Hall,
    Queen's University at Kingston,
    Kingston, Ontario, Canada
    K7L 3N6

    Tel: (613) 533-2702
    Fax: (613) 533-6813

    SNO Institute Director:

    Dr. Tony Noble (Queen's University)
    The Sudbury Neutrino Observatory Institute

    Department of Physics, Stirling Hall,
    Queen's University at Kingston,
    Kingston, Ontario, Canada
    K7L 3N6

    Tel: (613) 533-2679
    Fax: (613) 533-6813

    The SNO Site Project Office:

    SNO Operations Control Building


    INCO Creighton #9 Mine
    P.O. Box 159
    Lively, Ontario, Canada
    P3Y 1M3

    Tel: (705) 692-7000
    Fax: (705) 692-7001

    For general information email: xổ số khánh gia lai

    URL: http://www.sno.phy.queensu.ca/sno/ (Last revised Nov 9, 2015)
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