We report a measurement of the neutrino-electron elastic scattering rate from [superscript 8]B 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 [superscript 8]B neutrino spectrum, this corresponds to a spectrum integrated flux of 2.77 ± 0.26(stat) ± 0.32(syst) ×10[superscript 6] cm[superscript −2]s[superscript −1]. The analysis threshold is driven by [superscript 208]Tl present in the liquid scintillator, and the main source of systematic uncertainty is due to background from cosmogenic [superscript 11]Be. The measured rate is consistent...
A measurement of the 8B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with ...
We report on an improved measurement of the B8 solar neutrino interaction rate with the Borexino exp...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...
We report a measurement of the neutrino-electron elastic scattering rate from 8B solar neutrinos bas...
We report a measurement of the neutrino-electron elastic scattering rate from 8B solar neutrinos bas...
We report a measurement of the neutrino-electron elastic scattering rate from ^8B solar neutrinos ba...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV [superscript 7]B...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV Be7 solar neutri...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV Be7 solar neutri...
We report the measurement of electron neutrino elastic scattering from 8B solar neutrinos with 3 MeV...
6 pages, 4 figuresWe report the measurement of the 8B solar neutrinos interaction rate with the Bore...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
International audienceWe report on an improved measurement of the B8 solar neutrino interaction rate...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
A measurement of the 8B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with ...
We report on an improved measurement of the B8 solar neutrino interaction rate with the Borexino exp...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...
We report a measurement of the neutrino-electron elastic scattering rate from 8B solar neutrinos bas...
We report a measurement of the neutrino-electron elastic scattering rate from 8B solar neutrinos bas...
We report a measurement of the neutrino-electron elastic scattering rate from ^8B solar neutrinos ba...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV [superscript 7]B...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV Be7 solar neutri...
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV Be7 solar neutri...
We report the measurement of electron neutrino elastic scattering from 8B solar neutrinos with 3 MeV...
6 pages, 4 figuresWe report the measurement of the 8B solar neutrinos interaction rate with the Bore...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
International audienceWe report on an improved measurement of the B8 solar neutrino interaction rate...
The Sudbury Neutrino Observatory (SNO) is a water Cerenkov detector designed to study solar neutrino...
A measurement of the 8B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with ...
We report on an improved measurement of the B8 solar neutrino interaction rate with the Borexino exp...
The Sudbury Neutrino Observatory, through its measurements of the solar 8B neutrino flux via the cha...