Atmospheric Neutrinos in SNO

Details Atmospheric Neutrinos in SNO Atmospheric Neutrinos in SNO

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..nws.j2004n&link_type=abstract

American Physical Society, Second Meeting of the Northwest Section 2000 May 19-20, 2000 University of Oregon Eugene, Oregon, abs

Physics

Scientific paper

The Sudbury Neutrino Observatory (SNO) was designed primarily to detect solar neutrinos. Its detection of atmospheric neutrinos, however, will be a nice bonus, providing an independent flux measurement in a geomagnetic environment very different from SuperKamiokande. This talk will provide a brief overview of atmospheric neutrino detection in SNO, including the advantages that come from being 2 km underground, as well as further detail on what we expect to see and some of what has been seen so far.

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