Measuring the Neutrino Interaction Rates in SNO for Variable Fiducial Volumes

Details Measuring the Neutrino Interaction Rates in SNO for Variable Fiducial Volumes Measuring the Neutrino Interaction Rates in SNO for Variable Fiducial Volumes

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apr.x7004h&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

Neutrinos from ^8B decays in the Sun are detected in the Sudbury Neutrino Observatory (SNO) via the charged-current and neutral-current dissociation of deuterium as well as the elastic scattering off electrons. A spherical acrylic vessel filled with heavy water and surrounded by a light water shield is used in SNO as the target volume. Using the characteristic radial and solar angle distributions of the neutrino signal and its principal backgrounds we determine the interaction rates of solar neutrinos for variable fiducial volumes. This analysis demonstrates the stability of signal extraction in SNO independent of fiducial volume.

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