Document Type
Article
Publication Date
1-1-2010
Abstract
We have performed three searches for high-frequency signals in the solar neutrino flux measured by the Sudbury Neutrino Observatory, motivated by the possibility that solar g-mode oscillations could affect the production or propagation of solar 8B neutrinos. The first search looked for any significant peak in the frequency range 1-144day-1, with a sensitivity to sinusoidal signals with amplitudes of 12% or greater. The second search focused on regions in which g-mode signals have been claimed by experiments aboard the Solar and Heliospheric Observatory satellite, and was sensitive to signals with amplitudes of 10% or greater. The third search looked for extra power across the entire frequency band. No statistically significant signal was detected in any of the three searches. © 2010. The American Astronomical Society.
Publication Source (Journal or Book title)
Astrophysical Journal
First Page
540
Last Page
548
Recommended Citation
Aharmim, B., Ahmed, S., Anthony, A., Barros, N., Beier, E., Bellerive, A., Beltran, B., Bergevin, M., Biller, S., Boudjemline, K., Boulay, M., Burritt, T., Cai, B., Chan, Y., Chauhan, D., Chen, M., Cleveland, B., Cox, G., Dai, X., Deng, H., Detwiler, J., Dimarco, M., Doe, P., Doucas, G., Drouin, P., Duba, C., Duncan, F., & Dunford, M. (2010). Searches for high-frequency variations in the 8B solar neutrino flux at the sudbury neutrino observatory. Astrophysical Journal, 710 (1), 540-548. https://doi.org/10.1088/0004-637X/710/1/540