Erratum: Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days [Phys. Rev. Lett. 81, 1158 (1998)]

Fukuda, Y.; Hayakawa, Tomokatsu; Ichihara, E.; Inoue, K.; Ishihara, K.; Ishino, H.; Itow, Y.; Kajita, T.; Kameda, J.; Kasuga, S.; Kobayashi, Kazuyoshi; Kobayashi, Yoshiyuki; Koshio, Y.; Martens, K.; Miura, Makoto; Nakahata, M.; Nakayama, S.; Okada, Atsushi; Oketa, M.; Okumura, K.; M, Ota; Sakurai, N.; Shiozawa, M.; Suzuki, Yoshihiro; Takeuchi, Y.; Totsuka, Y.; Yamada, Shoichi; Earl, M.; Habig, A.; Hong, J. T.; Kearns, E.; Kim, S. B.; Masuzawa, M.; Messier, M. D.; Scholberg, K.; Stone, James L.; Sulak, L.; Walter, C.W.; Goldhaber, M.; Barszczak, T.; Gajewski, W.; Halverson, P. G.; Hsu, Jonathan Y.; Kropp, W. R.; Price, L. R.; Reines, F.; Sobel, H. W.; Vagins, M. R.; Ganezer, K. S.; Keig, W. E.; Ellsworth, R. W.; Tasaka, S.; Flanagan, J.; Kibayashi, A.; Learned, J. G.; Matsuno, S.; Stenger, V. J.; Takemori, D.; Ishii, T.; Kanzaki, J.; Kobayashi, Tooru; Nakamura, K.; Nishikawa, K.; Oyama, Y.; Sakai, Akito; Sakuda, M.; Sasaki, O.; Echigo, S.; Kohama, M.; Haines, T. J.; Blaufuss, E.; Sanford, R.; Svoboda, R.; Chen, M. L.; Conner, Z.; Goodman, J. A.; Sullivan, G. W.; Mori, M.; Hill, J.; Jung, C. K.; Mauger, C.; McGrew, C.; Sharkey, E.; Viren, B.; Yanagisawa, C.; Doki, W.; Ishizuka, T.; Kitaguchi, Y.; Koga, Hisashi; Miyano, K.; Okazawa, H.; Saji, C.; Takahata, M.; Kusano, Akira; Nagashima, Yasuyuki; Takita, M.; Yamaguchi, Tomohiro; Yoshida, Masato; Etoh, M.; Fujita, K.; Hasegawa, T.; Hasegawa, T.; Hatakeyama, S.; Iwamoto, Toshiyuki; Kinebuchi, T.; Koga, M.; Maruyama, T.; Ogawa, Hiroshi; Suzuki, A.; Tsushima, F.; Koshiba, M.; Nemoto, Mariko; Nishijima, Kazuhiko; Futagami, T.; Hayato, Y.; Kanaya, Yoshio; Kaneyuki, K.; Watanabe, Y.; Kiełczewska, D.; Doyle, R. A.; George, Jimin; Stachyra, A.L; Wai, L.; Wilkes, J.; Young, K. K.

doi:10.1103/physrevlett.81.4279

Cited by 209 publications

(154 citation statements)

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“…The present Super-Kamiokande [2] and CHOOZ [11] data favor the approximate decoupling between solar and atmospheric neutrino oscillations, which are respectively attributed to ν e → ν µ and ν µ → ν τ transitions in the framework of three active neutrinos.Thus one may take ∆m …”

supporting

confidence: 50%

“…Recently a number of models of lepton mass matrices have been proposed at low energy scales [1], at which their consequences on the spectrum of neutrino masses and the mixing of lepton flavors can directly be confronted with the robust Super-Kamiokande data on atmospheric and solar neutrino oscillations [2]. From the theoretical point of view, however, a phenomenologically-favored scheme of lepton mass matrices might only serve as the lowscale approximation of a more fundamental theory responsible for the lepton mass generation and flavor mixing at superhigh energy scales.…”

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confidence: 99%

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Democratic neutrino mixing and radiative corrections

Zhang

2001

Phys. Rev. D

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The renormalization effect on a specific ansatz of lepton mass matrices, arising naturally from the breaking of flavor democracy for charged leptons and that of mass degeneracy for light neutrinos, is studied from a superhigh energy scale M 0 ∼ 10 13 GeV to the electroweak scale in the framework of the minimal supersymmetric standard model. We find that the democratic neutrino mixing pattern obtained from this ansatz may in general be instable against radiative corrections. With the help of similar flavor symmetries we prescribe a slightly different scheme of lepton mass matrices at the scale M 0 , from which the democratic mixing pattern of lepton flavors can be achieved, after radiative corrections, at the experimentally accessible scales. PACS number(s): 14.60. Pq, 12.15.Ff, 11.10.Hi Typeset using REVT E X 1

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supporting

confidence: 50%

mentioning

confidence: 99%

Democratic neutrino mixing and radiative corrections

Zhang

2001

Phys. Rev. D

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“…Although neutrinos were considered massless within the standard model, abundant evidence of lepton flavor violation by neutrinos strongly implies small but nonzero masses. A long-standing disparity between measurement and models of the solar ν e flux was corroborated by successive radiochemical [1][2][3] and waterCherenkov [4,5] experiments. Variation of the ratio of atmospheric ν μ to ν e provided initial evidence for distance-dependent neutrino disappearance [6].…”

Section: Introductionmentioning

confidence: 99%

Measurement of electron antineutrino oscillation based on 1230 days of operation of the Daya Bay experiment

An¹,

Balantekin²,

Band³

et al. 2017

Phys. Rev. D

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356

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A measurement of electron antineutrino oscillation by the Daya Bay Reactor Neutrino Experiment is described in detail. Six 2.9-GWth nuclear power reactors of the Daya Bay and Ling Ao nuclear power facilities served as intense sources of ν e 's. Comparison of theν e rate and energy spectrum measured by antineutrino detectors far from the nuclear reactors (∼1500-1950 m) relative to detectors near the reactors (∼350-600 m) allowed a precise measurement ofν e disappearance. More than 2.5 millionν e inverse beta-decay interactions were observed, based on the combination of 217 days of operation of six antineutrino detectors (December, 2011-July, 2012) with a subsequent 1013 days using the complete configuration of eight detectors (October, 2012-July, 2015. Theν e rate observed at the far detectors relative to the near detectors showed a significant deficit, R ¼ 0.949 AE 0.002ðstatÞAE 0.002ðsystÞ. The energy dependence ofν e disappearance showed the distinct variation predicted by neutrino oscillation. Analysis using an approximation for the three-flavor oscillation probability yielded the flavor-mixing angle sin 2 2θ 13 ¼ 0.0841 AE 0.0027ðstatÞ AE 0.0019ðsystÞ and the effective neutrino mass-squared difference of jΔm 2 ee j ¼ ð2.50 AE 0.06ðstatÞ AE 0.06ðsystÞÞ × 10 −3 eV 2 . Analysis using the exact three-flavor probability found Δm

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“…[2], Kamiokande and Super-Kamiokande [3] assigned mass to the neutrinos. Whereas in standard model (SM) neutrinos are massless.…”

Section: Confirmation Of Neutrino Oscillations By Different Neutrino mentioning

confidence: 99%

Extrinsic CPT Violation With Sterile Neutrino

.¹

2016

IJRET

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Erratum: Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days [Phys. Rev. Lett. 81, 1158 (1998)]

Abstract: Reference [15] should read as follows:[15] S. M. Bilenky and B.

Cited by 209 publications

References 3 publications

Democratic neutrino mixing and radiative corrections

Democratic neutrino mixing and radiative corrections

Measurement of electron antineutrino oscillation based on 1230 days of operation of the Daya Bay experiment

Extrinsic CPT Violation With Sterile Neutrino

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