Journal
PHYSICAL REVIEW C
Volume 84, Issue 3, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.84.035804
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Funding
- Japanese Ministry of Education, Culture, Sports, Science and Technology [16002002]
- World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan
- US Department of Energy (DOE) [DE-FG03-00ER41138, DE-AC02-05CH11231, DE-FG02-01ER41166]
- DOE
- U.S. Department of Energy (DOE) [DE-FG02-01ER41166] Funding Source: U.S. Department of Energy (DOE)
- Division Of Physics
- Direct For Mathematical & Physical Scien [1002399] Funding Source: National Science Foundation
- Grants-in-Aid for Scientific Research [21000001, 21684008, 16002002, 10J02265, 23540289, 21244025] Funding Source: KAKEN
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We report a measurement of the neutrino-electron elastic scattering rate from B-8 solar neutrinos based on a 123 kton-day exposure of KamLAND. The background-subtracted electron recoil rate, above a 5.5-MeV analysis threshold is 1.49 +/- 0.14(stat) +/- 0.17(syst) events per kton-day. Interpreted as due to a pure electron flavor flux with a B-8 neutrino spectrum, this corresponds to a spectrum integrated flux of 2.77 +/- 0.26(stat) +/- 0.32(syst) x 10(6) cm(-2)s(-1). The analysis threshold is driven by Tl-208 present in the liquid scintillator, and the main source of systematic uncertainty is due to background from cosmogenic Be-11. The measured rate is consistent with existing measurements and with standard solar model predictions which include matter-enhanced neutrino oscillation.
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