Be7 solar neutrino measurement with KamLAND

Gando, A.; Gando, Y.; Hanakago, H.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Ishikawa, H.; Kishimoto, Y.; Koga, M.; Matsuda, R.; Matsuda, S.; Mitsui, T.; Motoki, D.; Nakajima, K.; Nakamura, K.; Obata, A.; Oki, A.; Oki, Y.; Otani, M.; Shimizu, I.; Shirai, J.; Suzuki, A.; Tamae, K.; Ueshima, K.; Watanabe, H.; Xu, B. D.; Yamada, S.; Yamauchi, Y.; Yoshida, H.; Kozlov, A.; Takemoto, Y.; Yoshida, S.; Grant, C.; Keefer, G.; McKee, D. W.; Piepke, A.; Banks, T. I.; Bloxham, T.; Freedman, S. J.; Fujikawa, B. K.; Han, K.; Hsu, L.; Ichimura, K.; Murayama, H.; O'Donnell, T.; Steiner, H. M.; Winslow, L. A.; Dwyer, D.; Mauger, C.; McKeown, R. D.; Zhang, C.; Berger, B. E.; Lane, C. E.; Maricic, J.; Miletic, T.; Learned, J. G.; Sakai, M.; Horton-Smith, G. A.; Tang, A.; Downum, K. E.; Tolich, K.; Efremenko, Y.; Kamyshkov, Y.; Perevozchikov, O.; Karwowski, H. J.; Markoff, D. M.; Tornow, W.; Detwiler, J. A.; Enomoto, S.; Heeger, K.; Decowski, M. P.

doi:10.1103/PhysRevC.92.055808

Title: ${}^{7}{Be}$ solar neutrino measurement with KamLAND

Journal Article · Mon Nov 30 00:00:00 EST 2015 · Physical Review C, Nuclear Physics

DOI:https://doi.org/10.1103/PhysRevC.92.055808· OSTI ID:1134245

Gando, A.; Gando, Y.; Hanakago, H.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Ishikawa, H.; Kishimoto, Y.; Koga, M.; Matsuda, R.; Matsuda, S.; Mitsui, T.; Motoki, D.; Nakajima, K.; Nakamura, K.; Obata, A.; Oki, A.; Oki, Y.; Otani, M.; Shimizu, I. more »

We report a measurement of the neutrino-electron elastic scattering rate of 862 keV ⁷Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)^₋1, which corresponds to an 862-keV ⁷Be solar neutrino flux of (3.26±0.52)×10⁹cm^₋2s^₋1, assuming a pure electron-flavor flux. Comparing this flux with the standard solar model prediction and further assuming three-flavor mixing, a ν_e survival probability of 0.66±0.15 is determined from the KamLAND data. Lastly, utilizing a global three-flavor oscillation analysis, we obtain a total ⁷Be solar neutrino flux of (5.82±1.02)×10⁹cm^₋2s^₋1, which is consistent with the standard solar model predictions.

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Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)

Sponsoring Organization:: USDOE; Japanese Ministry of Education, Culture, Sports, Science and Technology; the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan; Stichting FOM in the Netherlands

Contributing Organization:: KamLAND Collaboration

DOE Contract Number:: AC02-05CH11231; FG02-01ER41166; 16002002; 21000001

OSTI ID:: 1134245

Report Number(s):: LBNL-6653E; PRVCAN

Journal Information:: Physical Review C, Nuclear Physics, Vol. 92, Issue 5; ISSN 0556-2813

Publisher:: American Physical Society (APS)

Country of Publication:: United States

Language:: English

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Detection of sub-GeV dark matter and solar neutrinos via chemical-bond breaking Essig, Rouven; Mardon, Jeremy; Slone, Oren Physical Review D, Vol. 95, Issue 5 https://doi.org/10.1103/physrevd.95.056011	journal	March 2017
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Detection of sub-GeV Dark Matter and Solar Neutrinos via Chemical-Bond Breaking Essig, Rouven; Mardon, Jeremy; Slone, Oren arXiv https://doi.org/10.48550/arxiv.1608.02940	text	January 2016
Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment Akerib, D. S.; Akerlof, C. W.; Alsum, S. K. arXiv https://doi.org/10.48550/arxiv.1802.06039	text	January 2018
Constraining Sterile Neutrino Cosmology with Terrestrial Oscillation Experiments Berryman, Jeffrey M. arXiv https://doi.org/10.48550/arxiv.1905.03254	text	January 2019

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