Measurement of the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity.
By S. N. Ahmed, A. Anthony, E. Beier, A. Bellerive, S. Biller, J. Boger, M. Boulay, M. Bowler, T. Bowles, S. Brice and 121 more. Physical Review Letters, 2004
602 citations recorded by the source corpus.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/9a4bbf62f9a5db188bca35041030182b5a77e91c
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In Nuclear and High Energy Physics
Citations in the corpus
- FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION (2008, neutral): “…solar neutrinos (Davis et al. 1968; Cleveland et al. 1998; Hampel et al. 1999; Abdurashitov et al. 1999; Fukuda et al. 2001b,a; Ahmad et al. 2002; Ahmed et al. 2004), reactor neutrinos (Eguchi et al. 2003; Araki et al. 2005), and accelerator beam neutrinos (Ahn et al. 2003; Michael et al. 2006).”
- New Solar Opacities, Abundances, Helioseismology, and Neutrino Fluxes (2004, background): “Using OP opacity, the ratio of the 8B neutrino flux calculated with the older (larger) heavy element abundances (or with the newer (lower) heavy element abundances) to the total 8B neutrino flux measured by the Sudbury Neutrino Observatory (Ahmed et al. 2004) is (see Table 2) SolarModel 8B ν flux Me”
- Dark energy from mass varying neutrinos (2003, neutral): “1.1 Coincidences and Damn Coincidences 2”
- An improved limit on the axion–photon coupling from the CAST experiment (2007, background): “Even though details of our understanding of the Sun may change in the future, the solar neutrino measurement of all active flavours [61] has provided a direct verification of the Sun’s inner properties so that it is hard to imagine that adopting a standard solar model for the axion flux calculation ”