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Aharmim, B.; Ahmed, S. N.; Anthony, A. E.; Barros, N.; Beier, E. W.; Bellerive, A.; Beltran, B.; Bergevin, M.; Biller, S. D.; Boudjemline, K.; Boulay, M. G.; Cai, B.; Chan, Y. D.; Chauhan, D.; Chen, M.; Cleveland, B. T.; Cox, G. A.; Dai, X.; Deng, H.; Detwiler, J. A.; DiMarco, M.; Diamond, M. D.; Doe, P. J.; Doucas, G.; Drouin, P. -L.; Duncan, F. A.; Dunford, M.; Earle, E. D.; Elliott, S. R.; Evans, H. C. ... view all 127 authors View less authors (2013)
Publisher: Elsevier
Languages: English
Types: Article
Subjects: Astrophysics - Solar and Stellar Astrophysics, QC, Nuclear Experiment

Classified by OpenAIRE into

arxiv: High Energy Physics::Experiment, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Physics::Instrumentation and Detectors, Astrophysics::Solar and Stellar Astrophysics
The Sudbury Neutrino Observatory (SNO) has confirmed the standard solar model and neutrino oscillations through the observation of neutrinos from the solar core. In this paper we present a search for neutrinos associated with sources other than the solar core, such as gamma-ray bursters and solar flares. We present a new method for looking for temporal coincidences between neutrino events and astrophysical bursts of widely varying intensity. No correlations were found between neutrinos detected in SNO and such astrophysical sources.
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