Periodicity studies of solar neutrino signals at the Sudbury Neutrino Observatory

Details Periodicity studies of solar neutrino signals at the Sudbury Neutrino Observatory Periodicity studies of solar neutrino signals at the Sudbury Neutrino Observatory

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..apr.h9002a&link_type=abstract

American Physical Society, APS April Meeting, April 22-26, 2006, abstract #H9.002

Physics

Scientific paper

The Sudbury Neutrino Observatory collaboration has performed a search for sinusoidal periodicity in the ^8B solar neutrino flux, and has found no evidence of variations for periods between 1 day and 10 years. I describe here an effort to use the Rayleigh Power Test to probe periodicities in the SNO data in a higher frequency range than has been previously sampled (> 1 day-1). This has the advantage of sensitivity to neutrino flux variations that might arise due to solar oscillatory activity, particularly gravitational mode oscillations (``g-mode'' oscillations), which are confined to the interior of the sun.

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