A search for astrophysical burst signals at the Sudbury Neutrino Observatory

作者：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; Ewan G T; Farine J; Fergani H; Fleurot F; Ford R J; Formaggio J A

来源：Astroparticle Physics, 2014, 55: 1-7.

DOI：10.1016/j.astropartphys.2013.12.004

• Neutrinos
• Gamma-ray burst
• Solar flares

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 bursts 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.

• 出版日期2014-3
• 单位Los Alamos; MIT