PhysRevD.99.012012.pdf (301.51 kB)
Download fileMeasurement of the 8B solar neutrino flux in SNO+ with very low backgrounds
journal contribution
posted on 2023-06-12, 09:00 authored by M Anderson, S Andringa, S Asahi, M Askins, D J Auty, N Barros, D Bartlett, F Barão, Elisabeth FalkElisabeth Falk, Jeff HartnellJeff Hartnell, M Mlejnek, Martti Nirkko, Simon PeetersSimon Peeters, Michal RiganMichal Rigan, M I Stringer, SNO+ Collaboration, othersA measurement of the 8B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with the SNO+ detector during its water commissioning phase. At energies above 6 MeV the dataset is an extremely pure sample of solar neutrino elastic scattering events, owing primarily to the detector’s deep location, allowing an accurate measurement with relatively little exposure. In that energy region the best fit background rate is 0.25+0.09-0.07??events/kt-day, significantly lower than the measured solar neutrino event rate in that energy range, which is 1.03+0.13-0.12??events/kt-day. Also using data below this threshold, down to 5 MeV, fits of the solar neutrino event direction yielded an observed flux of 2.53+0.31-0.28(stat)+0.13-0.10(syst)×106??cm-2?s-1, assuming no neutrino oscillations. This rate is consistent with matter enhanced neutrino oscillations and measurements from other experiments.
History
Publication status
- Published
File Version
- Published version
Journal
Physical Review DISSN
2470-0010Publisher
American Physical SocietyExternal DOI
Issue
1Volume
99Page range
012012 1-7Department affiliated with
- Physics and Astronomy Publications
Research groups affiliated with
- Experimental Particle Physics Research Group Publications
Full text available
- Yes
Peer reviewed?
- Yes