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dc.contributor.authorWinslow, Lindley
dc.date.accessioned2018-07-20T17:29:51Z
dc.date.available2018-07-20T17:29:51Z
dc.date.issued2015-11
dc.date.submitted2015-07
dc.identifier.issn0556-2813
dc.identifier.issn1089-490X
dc.identifier.urihttp://hdl.handle.net/1721.1/117030
dc.description.abstractWe report a measurement of the neutrino-electron elastic scattering rate of 862 keV [superscript 7]Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)[superscript -1], which corresponds to an 862-keV [superscript 7]Be solar neutrino flux of (3.26±0.52)×109cm[superscript -2]s[superscript -1], assuming a pure electron-flavor flux. Comparing this flux with the standard solar model prediction and further assuming three-flavor mixing, a ν[superscript e] survival probability of 0.66±0.15 is determined from the KamLAND data. Utilizing a global three-flavor oscillation analysis, we obtain a total Be7 solar neutrino flux of (5.82±1.02)×109cm[superscript -]2s[superscript -1], which is consistent with the standard solar model predictions.en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-AC02-05CH11231)en_US
dc.description.sponsorshipUnited States. Department of Energy (Grant DE-FG02-01ER41166)en_US
dc.publisherAmerican Physical Society (APS)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PHYSREVC.92.055808en_US
dc.rightsArticle 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.en_US
dc.sourceAPSen_US
dc.title[superscript 7]Be solar neutrino measurement with KamLANDen_US
dc.typeArticleen_US
dc.identifier.citationGando, A., et al. “Be 7 Solar Neutrino Measurement with KamLAND.” Physical Review C, vol. 92, no. 5, Nov. 2015. © 2015 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorWinslow, Lindley
dc.relation.journalPhysical Review Cen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-05-08T16:33:18Z
dspace.orderedauthorsGando, 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.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-9970-108X
mit.licensePUBLISHER_POLICYen_US


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