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Measurement of the [superscript 8]B solar neutrino flux with the KamLAND liquid scintillator detector

Author(s)
Winslow, Lindley
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Alternative title
Measurement of the 8B solar neutrino flux with the KamLAND liquid scintillator detector
Terms of use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
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Abstract
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 with existing measurements and with standard solar model predictions which include matter-enhanced neutrino oscillation.
Date issued
2011-09
URI
http://hdl.handle.net/1721.1/69835
Department
Massachusetts Institute of Technology. Department of Physics
Journal
Physical Review C
Publisher
American Physical Society (APS)
Citation
Abe, S. et al. “Measurement of the ^{8}B Solar Neutrino Flux with the KamLAND Liquid Scintillator Detector.” Physical Review C 84.3 (2011): n. pag. Web. 22 Mar. 2012. © 2011 American Physical Society
Version: Final published version
ISSN
0556-2813
1089-490X

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