Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access
  • Access by Xinjiang University

Solar neutrino measurements using the full data period of Super-Kamiokande-IV

K. Abe1,49, C. Bronner1, Y. Hayato1,49, K. Hiraide1,49, K. Hosokawa1, K. Ieki1,49, M. Ikeda1,49, S. Imaizumi1, K. Iyogi1 et al. (Super-Kamiokande Collaboration)

K. Iyogi1, J. Kameda1,49, Y. Kanemura1, R. Kaneshima1, Y. Kashiwagi1, Y. Kataoka1,49, Y. Kato1, Y. Kishimoto1,49,a, S. Miki1, S. Mine1,6, M. Miura1,49, T. Mochizuki1, S. Moriyama1,49, Y. Nagao1, M. Nakahata1,49, Y. Nakano1, S. Nakayama1,49, Y. Noguchi1, T. Okada1, K. Okamoto1, A. Orii1,b, K. Sato1, H. Sekiya1,49, H. Shiba1, K. Shimizu1, M. Shiozawa1,49, Y. Sonoda1, Y. Suzuki1, A. Takeda1,49, Y. Takemoto1,49, A. Takenaka1,c, H. Tanaka1,49, S. Watanabe1, T. Yano1, S. Han2, T. Kajita2,49,22, K. Okumura2,49, T. Tashiro2, T. Tomiya2, R. Wang2, X. Wang2, S. Yoshida2, D. Bravo-Berguño3, P. Fernandez3, L. Labarga3, N. Ospina3, B. Zaldivar3, B. W. Pointon4,53, F. d. M. Blaszczyk5,d, C. Kachulis5,49, E. Kearns5,49, J. L. Raaf5, J. L. Stone5, L. Wan5, T. Wester5, J. Bian6, N. J. Griskevich6, W. R. Kropp6,*, S. Locke6, M. B. Smy6, H. W. Sobel6,49, V. Takhistov6,24, P. Weatherly6, A. Yankelevich6, K. S. Ganezer7,*, J. Hill7, M. C. Jang8, J. Y. Kim8, S. Lee8, I. T. Lim8, D. H. Moon8, R. G. Park8, B. Bodur9, K. Scholberg9,49, C. W. Walter9,49, A. Beauchêne10, L. Bernard10, A. Coffani10, O. Drapier10, S. El Hedri10, A. Giampaolo10, J. Imber10, Th. A. Mueller10, P. Paganini10, R. Rogly10, B. Quilain10, A. Santos10, T. Nakamura11, J. S. Jang12, L. N. Machado13, J. G. Learned14, S. Matsuno14, N. Iovine15, K. Choi15, S. Cao16, L. H. V. Anthony17, R. P. Litchfield17,e, N. Prouse17, D. Marin17, M. Scott17, A. A. Sztuc17, Y. Uchida17, V. Berardi18, M. G. Catanesi18, R. A. Intonti18, E. Radicioni18, N. F. Calabria19, G. De Rosa19, A. Langella19, G. Collazuol20, F. Iacob20, M. Lamoureux20, M. Mattiazzi20, L. Ludovici21, M. Gonin22, L. Périssé22, G. Pronost22, C. Fujisawa23, Y. Maekawa23, Y. Nishimura23, R. Okazaki23, M. Friend24, T. Hasegawa24, T. Ishida24, M. Jakkapu24, T. Kobayashi24, T. Matsubara24, T. Nakadaira24, K. Nakamura24,49, Y. Oyama24, K. Sakashita24, T. Sekiguchi24, T. Tsukamoto24, T. Boschi25, N. Bhuiyan25, G. T. Burton25, J. Gao25, A. Goldsack25, T. Katori25, F. Di Lodovico25, J. Migenda25, S. Molina Sedgwick25,f, R. M. Ramsden25, M. Taani25, Z. Xie25, S. Zsoldos25,49, KE. Abe26, M. Hasegawa26, Y. Isobe26, Y. Kotsar26, H. Miyabe26, H. Ozaki26, T. Shiozawa26, T. Sugimoto26, A. T. Suzuki26, Y. Takagi26, Y. Takeuchi26,49, S. Yamamoto26, H. Zhong26, Y. Ashida27,g, J. Feng27, L. Feng27, T. Hayashino27, S. Hirota27, J. R. Hu27, Z. Hu27, M. Jiang27, M. Kawaue27, T. Kikawa27, M. Mori27,h, KE. Nakamura27, T. Nakaya27,49, R. A. Wendell27,49, K. Yasutome27, S. J. Jenkins28, N. McCauley28, P. Mehta28, A. Pritchard28, A. Tarrant28, M. J. Wilking29, Y. Fukuda30, Y. Itow31,32, H. Menjo31, M. Murase31, K. Ninomiya31, T. Niwa31, M. Tsukada31, Y. Yoshioka31, K. Frankiewicz33,i, J. Lagoda33, M. Mandal33, P. Mijakowski33, Y. S. Prabhu33, J. Zalipska33, J. Jiang34, M. Jia34, C. K. Jung34, J. L. Palomino34,j, G. Santucci34,k, W. Shi34,l, C. Vilela34,m, C. Yanagisawa34,n, D. Fukuda35, K. Hagiwara35, M. Harada35, Y. Hino35, T. Horai35, H. Ishino35, S. Ito35, H. Kitagawa35, Y. Koshio35,49, W. Ma35, F. Nakanishi35, N. Piplani35, S. Sakai35, M. Sakuda35, T. Tada35, T. Tano35, C. Xu35, R. Yamaguchi35, T. Ishizuka36, Y. Kuno37, G. Barr38, D. Barrow38, L. Cook38,49, S. Samani38,49, C. Simpson38,49, D. Wark38,44, A. M. Holin39, F. Nova39, S. Jung40, B. Yang40, J. Y. Yang40, J. Yoo40, J. E. P. Fannon41, L. Kneale41, M. Malek41, J. M. McElwee41, O. Stone41, M. D. Thiesse41, L. F. Thompson41, S. T. Wilson41, H. Okazawa42, S. M. Lakshmi43, Y. Choi45, S. B. Kim45, E. Kwon45, J. W. Seo45, I. Yu45, A. K. Ichikawa46, K. Nakamura46, S. Tairafune46, K. Nishijima47, A. Eguchi48, K. Iwamoto48, K. Nakagiri48, Y. Nakajima48,49, N. Ogawa48, S. Shima48, E. Watanabe48, M. Yokoyama48,49, R. G. Calland49, S. Fujita49, C. Jesús-Valls49, J. Xia49, T. K. Ming49, P. de Perio49, K. Martens49, M. Murdoch49, M. R. Vagins49,6, S. Izumiyama50, M. Kuze50, R. Matsumoto50, Y. Okajima50, M. Tanaka50, T. Yoshida50, M. Inomoto51, M. Ishitsuka51, H. Ito51, T. Kinoshita51, R. Matsumoto51, K. Ohta51, Y. Ommura51, M. Shinoki51, N. Shigeta51, T. Suganuma51, K. Yamauchi51, T. Yoshida51, J. F. Martin52, C. M. Nantais52, H. A. Tanaka52,m, T. Towstego52, R. Gaur53, V. Gousy-Leblanc53,o, M. Hartz53, A. Konaka53, X. Li53, S. Chen54, B. D. Xu54, B. Zhang54, S. Berkman55,d, M. Posiadala-Zezula56, S. B. Boyd57, R. Edwards57, D. Hadley57, M. Nicholson57, M. O’Flaherty57, B. Richards57, A. Ali58,53, B. Jamieson58, J. Walker58, S. Amanai59, Ll. Marti59, A. Minamino59, K. Okamoto59, G. Pintaudi59, S. Sano59, R. Sasaki59, S. Suzuki59, and K. Wada59 (Super-Kamiokande Collaboration)

  • 1Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
  • 2Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
  • 3Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain
  • 4Department of Physics, British Columbia Institute of Technology, Burnaby, British Columbia, V5G 3H2, Canada
  • 5Department of Physics, Boston University, Boston, Massachusetts 02215, USA
  • 6Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
  • 7Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
  • 8Institute for Universe and Elementary Particles, Chonnam National University, Gwangju 61186, Korea
  • 9Department of Physics, Duke University, Durham North Carolina 27708, USA
  • 10Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France
  • 11Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan
  • 12GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea
  • 13School of Physics and Astronomy, University of Glasgow, Glasgow, Scotland, G12 8QQ, United Kingdom
  • 14Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 15Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126, Korea
  • 16Institute For Interdisciplinary Research in Science and Education, ICISE, Quy Nhon, 55121, Vietnam
  • 17Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom
  • 18Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, I-70125, Bari, Italy
  • 19Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, I-80126, Napoli, Italy
  • 20Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, I-35131, Padova, Italy
  • 21INFN Sezione di Roma and Università di Roma “La Sapienza”, I-00185, Roma, Italy
  • 22ILANCE, CNRS - University of Tokyo International Research Laboratory, Kashiwa, Chiba 277-8582, Japan
  • 23Department of Physics, Keio University, Yokohama, Kanagawa, 223-8522, Japan
  • 24High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • 25Department of Physics, King’s College London, London, WC2R 2LS, United Kingdom
  • 26Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
  • 27Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
  • 28Department of Physics, University of Liverpool, Liverpool, L69 7ZE, United Kingdom
  • 29School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 30Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
  • 31Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 32Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 33National Centre For Nuclear Research, 02-093 Warsaw, Poland
  • 34Department of Physics and Astronomy, State University of New York at Stony Brook, New York 11794-3800, USA
  • 35Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
  • 36Media Communication Center, Osaka Electro-Communication University, Neyagawa, Osaka, 572-8530, Japan
  • 37Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
  • 38Department of Physics, Oxford University, Oxford, OX1 3PU, United Kingdom
  • 39Rutherford Appleton Laboratory, Harwell, Oxford, OX11 0QX, United Kingdom
  • 40Department of Physics, Seoul National University, Seoul 151-742, Korea
  • 41Department of Physics and Astronomy, University of Sheffield, S3 7RH, Sheffield, United Kingdom
  • 42Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka, 425-8611, Japan
  • 43August Chełkowski Institute of Physics, University of Silesia in Katowice, 75 Pułku Piechoty 1, 41-500 Chor zów, Poland
  • 44STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, OX11 0QX, United Kingdom
  • 45Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
  • 46Department of Physics, Faculty of Science, Tohoku University, Sendai, Miyagi, 980-8578, Japan
  • 47Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
  • 48Department of Physics, University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
  • 49Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
  • 50Department of Physics,Tokyo Institute of Technology, Meguro, Tokyo 152-8551, Japan
  • 51Department of Physics, Faculty of Science and Technology, Tokyo University of Science, Noda, Chiba 278-8510, Japan
  • 52Department of Physics, University of Toronto, Ontario, M5S 1A7, Canada
  • 53TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, V6T2A3, Canada
  • 54Department of Engineering Physics, Tsinghua University, Beijing, 100084, China
  • 55Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T1Z4, Canada
  • 56Faculty of Physics, University of Warsaw, Warsaw, 02-093, Poland
  • 57Department of Physics, University of Warwick, Coventry, CV4 7AL, United Kingdom
  • 58Department of Physics, University of Winnipeg, MB R3J 3L8, Canada
  • 59Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan

  • *Deceased.
  • aCurrently at Research Center for Neutrino Science, Tohoku University, Sendai 980-8578, Japan.
  • bCurrently at High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.
  • cCurrently at School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, China.
  • dCurrently at Fermi National Accelerator Laboratory, Batavia, IL 60510, USA.
  • eCurrently at School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom.
  • fCurrently at Department de Fisica Teorica, Universitat de Valencia, and Instituto de Fisica Corpuscular, CSIC, Universitat de Valencia, 46980 Paterna, Spain.
  • gCurrently at Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA.
  • hCurrently at Division of Science, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka-shi, Tokyo, Japan.
  • iCurrently at Department of Physics, Boston University, Boston, Massachusetts 02215, USA.
  • jCurrently at Department of Physics, Illinois Institute of Technology, Chicago, 60616, Illinois, USA.
  • kCurrently at Department of Physics and Astronomy, York University, Toronto, Ontario, Canada.
  • lCurrently at EP Department, CERN, 1211 Geneva 24, Switzerland.
  • mCurrently at SLAC National Accelerator Laboratory, 2575 Sand Hill Road, Menlo Park, CA 94025-7090, USA.
  • nAlso at BMCC/CUNY, Science Department, New York New York, 1007, USA.
  • oAlso at University of Victoria, Department of Physics and Astronomy, PO Box 1700 STN CSC, Victoria, BC V8W 2Y2, Canada.

Phys. Rev. D 109, 092001 – Published 3 May, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.092001

Abstract

An analysis of solar neutrino data from the fourth phase of Super-Kamiokande (SK-IV) from October 2008 to May 2018 is performed and the results are presented. The observation time of the dataset of SK-IV corresponds to 2970 days and the total live time for all four phases is 5805 days. For more precise solar neutrino measurements, several improvements are applied in this analysis: lowering the data acquisition threshold in May 2015, further reduction of the spallation background using neutron clustering events, precise energy reconstruction considering the time variation of the PMT gain. The observed number of solar neutrino events in 3.49–19.49 MeV electron kinetic energy region during SK-IV is 65,443388+390(stat.)±925(syst.) events. Corresponding B8 solar neutrino flux is (2.314±0.014(stat.)±0.040(syst.))×106cm2s1, assuming a pure electron-neutrino flavor component without neutrino oscillations. The flux combined with all SK phases up to SK-IV is (2.336±0.011(stat.)±0.043(syst.))×106cm2s1. Based on the neutrino oscillation analysis from all solar experiments, including the SK 5805 days dataset, the best-fit neutrino oscillation parameters are sin2θ12,solar=0.306±0.013 and Δm21,solar2=(6.100.81+0.95)×105eV2, with a deviation of about 1.5σ from the Δm212 parameter obtained by KamLAND. The best-fit neutrino oscillation parameters obtained from all solar experiments and KamLAND are sin2θ12,global=0.307±0.012 and Δm21,global2=(7.500.18+0.19)×105eV2.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (82)

  1. Z. Maki, M. Nakagawa, and S. Sakata, Remarks on the unified model of elementary particles, Prog. Theor. Phys. 28, 870 (1962).
  2. B. Pontecorvo, Neutrino experiments and the problem of conservation of leptonic charge, Sov. Phys. JETP 26, 984 (1968).
  3. R. Davis, Jr., D. S. Harmer, and K. C. Hoffman, Search for neutrinos from the sun, Phys. Rev. Lett. 20, 1205 (1968).
  4. K. S. Hirata, T. Kajita, T. Kifune, K. Kihara, M. Nakahata, K. Nakamura et al. (The Kamiokande-II Collaboration), Observation of B-8 solar neutrinos in the Kamiokande-II detector, Phys. Rev. Lett. 63, 16 (1989).
  5. A. I. Abazov, O. L. Anosov, E. L. Faizov, V. N. Gavrin, A. V. Kalikhov, T. V. Knodel et al., Search for neutrinos from sun using the reaction Ga-71 (electron-neutrino e-) Ge-71, Phys. Rev. Lett. 67, 3332 (1991).
  6. P. Anselmann et al. (The GALLEX Collaboration), Solar neutrinos observed by GALLEX at Gran Sasso, Phys. Lett. B 285, 376 (1992).
  7. M. Altmann et al. (The GNO Collaboration), GNO solar neutrino observations: Results for GNO I, Phys. Lett. B 490, 16 (2000).
  8. S. Fukuda et al. (The Super-Kamiokande Collaboration), Solar B-8 and hep neutrino measurements from 1258 days of Super-Kamiokande data, Phys. Rev. Lett. 86, 5651 (2001).
  9. Q. R. Ahmad et al. (The SNO Collaboration), Measurement of the rate of νe+dp+p+e interactions produced by B8 solar neutrinos at the Sudbury Neutrino Observatory, Phys. Rev. Lett. 87, 071301 (2001).
  10. Q. R. Ahmad et al. (The SNO Collaboration), Direct evidence for neutrino flavor transformation from neutral current interactions in the Sudbury Neutrino Observatory, Phys. Rev. Lett. 89, 011301 (2002).
  11. K. Eguchi et al. (The KamLAND Collaboration), First results from Kamland: Evidence for reactor antineutrino disappearance, Phys. Rev. Lett. 90, 021802 (2003).
  12. M. Agostini et al. (The Borexino Collaboration), First simultaneous precision spectroscopy of pp, Be7, and pep solar neutrinos with Borexino phase-II, Phys. Rev. D 100, 082004 (2019).
  13. M. Agostini et al. (The BOREXINO Collaboration), Comprehensive measurement of pp-chain solar neutrinos, Nature 562, 505 (2018).
  14. A. Gando et al. (The KamLAND Collaboration), Be7 solar neutrino measurement with KamLAND, Phys. Rev. C 92, 055808 (2015).
  15. M. Agostini et al. (The BOREXINO Collaboration), Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun, Nature (London) 587, 577 (2020).
  16. S. P. Mikheyev and A. Y. Smirnov, Resonance amplification of oscillations in matter and spectroscopy of solar neutrinos, Sov. J. Nucl. Phys. 42, 913 (1985).
  17. L. Wolfenstein, Neutrino oscillations in matter, Phys. Rev. D 17, 2369 (1978).
  18. A. J. Baltz and J. Weneser, Effect of transmission through the earth on neutrino oscillations, Phys. Rev. D 35, 528 (1987).
  19. J. Bouchez, M. Cribier, J. Rich, M. Spiro, D. Vignaud, and W. Hampel, Matter effects for solar neutrino oscillations, Z. Phys. C 32, 499 (1986).
  20. E. D. Carlson, Terrestrially enhanced neutrino oscillations, Phys. Rev. D 34, 1454 (1986).
  21. M. Cribier, W. Hampel, J. Rich, and D. Vignaud, MSW regeneration of solar νe in the earth, Phys. Lett. B 182, 89 (1986).
  22. S. T. Petcov, Diffractive—like (or parametric resonance—like?) enhancement of the earth (day—night) effect for solar neutrinos crossing the earth core, Phys. Lett. B 434, 321 (1998).
  23. P. Bakhti and A. Y. Smirnov, Oscillation tomography of the Earth with solar neutrinos and future experiments, Phys. Rev. D 101, 123031 (2020).
  24. A. Gando, Y. Gando, H. Hanakago, H. Ikeda, K. Inoue, K. Ishidoshiro et al. (The KamLAND Collaboration), Reactor on-off antineutrino measurement with KamLAND, Phys. Rev. D 88, 033001 (2013).
  25. K. Abe et al. (The Super-Kamiokande Collaboration), Solar neutrino measurements in Super-Kamiokande-IV, Phys. Rev. D 94, 052010 (2016).
  26. J. N. Bahcall, V. Barger, and D. Marfatia, How accurately can one test CPT conservation with reactor and solar neutrino experiments?, Phys. Lett. B 534, 120 (2002).
  27. Y. Fukuda et al. (The Super-Kamiokande Collaboration), The Super-Kamiokande detector, Nucl. Instrum. Methods Phys. Res., Sect. A 501, 418 (2003).
  28. K. Abe et al. (The Super-Kamiokande Collaboration), Calibration of the Super-Kamiokande detector, Nucl. Instrum. Methods Phys. Res., Sect. A 737, 253 (2014).
  29. K. Abe et al. (The Super-Kamiokande Collaboration), First gadolinium loading to Super-Kamiokande, Nucl. Instrum. Methods Phys. Res., Sect. A 1027, 166 (2022).
  30. J. P. Cravens et al. (The Super-Kamiokande Collaboration), Solar neutrino measurements in Super-Kamiokande-II, Phys. Rev. D 78, 032002 (2008).
  31. H. Nishino, K. Awai, Y. Hayato, S. Nakayama, K. Okumura, M. Shiozawa, A. Takeda, K. Ishikawa, A. Minegishi, and Y. Arai, High-speed charge-to-time converter ASIC for the Super-Kamiokande detector, Nucl. Instrum. Methods Phys. Res., Sect. A 610, 710 (2009).
  32. S. Yamada et al., Commissioning of the new electronics and online system for the Super-Kamiokande experiment, IEEE Trans. Nucl. Sci. 57, 428 (2010).
  33. Y. Nakano, T. Hokama, M. Matsubara, M. Miwa, M. Nakahata, T. Nakamura, H. Sekiya, Y. Takeuchi, S. Tasaka, and R. A. Wendell, Measurement of the radon concentration in purified water in the Super-Kamiokande IV detector, Nucl. Instrum. Methods Phys. Res., Sect. A 977, 164297 (2020).
  34. J. Hosaka et al. (The Super-Kamiokande Collaboration), Solar neutrino measurements in super-Kamiokande-I, Phys. Rev. D 73, 112001 (2006).
  35. Y. Nakano, H. Sekiya, S. Tasaka, Y. Takeuchi, R. A. Wendell, M. Matsubara, and M. Nakahata, Measurement of radon concentration in Super-Kamiokande’s buffer gas, Nucl. Instrum. Methods Phys. Res., Sect. A 867, 108 (2017).
  36. G. Pronost, M. Ikeda, T. Nakamura, H. Sekiya, and S. Tasaka, Development of new radon monitoring systems in the Kamioka mine, Prog. Theor. Exp. Phys. 2018, 093H01 (2018).
  37. K. Abe et al. (The Super-Kamiokande Collaboration), Radon background estimation by injecting radon enrich water at Super-Kamiokande IV detector (to be published).
  38. R. Brun, F. Bruyant, F. Carminati, S. Giani, M. Maire, A. McPherson, G. Patrick, and L. Urban, GEANT detector description and simulation tool, CERN-W5013, 10.17181/CERN.MUHF.DMJ1 (1994).
  39. W. T. Winter, S. J. Freedman, K. E. Rehm, and J. P. Schiffer, The B-8 neutrino spectrum, Phys. Rev. C 73, 025503 (2006).
  40. J. N. Bahcall, Hep energy spectrum, https://www.sns.ias.edu/~jnb/SNdata/sndata.html#hepspec (1998).
  41. J. N. Bahcall, M. Kamionkowski, and A. Sirlin, Solar neutrinos: Radiative corrections in neutrino—electron scattering experiments, Phys. Rev. D 51, 6146 (1995).
  42. B. Aharmim et al. (The SNO Collaboration), Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory, Phys. Rev. C 88, 025501 (2013).
  43. J. N. Bahcall and M. H. Pinsonneault, What do we (not) know theoretically about solar neutrino fluxes?, Phys. Rev. Lett. 92, 121301 (2004).
  44. M. Smy, Low energy event reconstruction and selection in Super-Kamiokande-III, in Proceedings of the 30th International Cosmic Ray Conference, Mérida, Yucatán, Mexico, 2007, edited by R. Caballero, J. C. D’Olivo, G. Medina-Tanco, L. Nellen, F. A. Sánchez, and J. F. Valdés-Galicia (Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008), pp. 1279–1282.
  45. M. Nakahata et al. (The Super-Kamiokande Collaboration), Calibration of Super-Kamiokande using an electron linac, Nucl. Instrum. Methods Phys. Res., Sect. A 421, 113 (1999).
  46. K. Abe et al. (The Super-Kamiokande Collaboration), Solar neutrino results in Super-Kamiokande-III, Phys. Rev. D 83, 052010 (2011).
  47. Y. Koshio, Study of solar neutrinos at Super Kamiokande, Ph.D. thesis, Tokyo U. (1998), https://www-sk.icrr.u-tokyo.ac.jp/sk/_pdf/articles/koshio-dthesis.pdf.
  48. S. Agostinelli et al. (GEANT4 Collaboration), GEANT4–a simulation toolkit, Nucl. Instrum. Methods Phys. Res., Sect. A 506, 250 (2003).
  49. J. Allison et al., Geant4 developments and applications, IEEE Trans. Nucl. Sci. 53, 270 (2006).
  50. J. Allison et al., Recent developments in Geant4, Nucl. Instrum. Methods Phys. Res., Sect. A 835, 186 (2016).
  51. E. Blaufuss et al. (The Super-Kamiokande Collaboration), N-16 as a calibration source for Super-Kamiokande, Nucl. Instrum. Methods Phys. Res., Sect. A 458, 638 (2001).
  52. D. E. Alburger, Beta Decay of N16, Phys. Rev. 111, 1586 (1958).
  53. Y. Nakano, B8 solar neutrino spectrum measurement using Super-Kamiokande IV, Ph.D. thesis, Tokyo U., 2016, https://www-sk.icrr.u-tokyo.ac.jp/sk/_pdf/articles/doc_thesis_naknao.pdf.
  54. S. W. Li and J. F. Beacom, First calculation of cosmic-ray muon spallation backgrounds for MeV astrophysical neutrino signals in Super-Kamiokande, Phys. Rev. C 89, 045801 (2014).
  55. S. W. Li and J. F. Beacom, Spallation backgrounds in Super-Kamiokande are made in muon-induced showers, Phys. Rev. D 91, 105005 (2015).
  56. S. W. Li and J. F. Beacom, Tagging spallation backgrounds with showers in water-Cherenkov detectors, Phys. Rev. D 92, 105033 (2015).
  57. S. Locke et al. (The Super-Kamiokande Collaboration), New methods and simulations for cosmogenic induced spallation removal in Super-Kamiokande-IV, arXiv:2112.00092.
  58. G. Carminati (The Super-Kamiokande Collaboration), The new wide-band solar neutrino trigger for Super-Kamiokande, Phys. Procedia 61, 666 (2015).
  59. M. Elnimr (The Super-Kamiokande Collaboration), Low energy B8 solar neutrinos with the wideband intelligent trigger at Super-Kamiokande, J. Phys. Conf. Ser. 888, 012189 (2017).
  60. B. Aharmim et al. (The SNO Collaboration), Electron energy spectra, fluxes, and day-night asymmetries of B-8 solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino Observatory, Phys. Rev. C 72, 055502 (2005).
  61. B. Aharmim et al. (The SNO Collaboration), Determination of the νe and total B8 solar neutrino fluxes with the Sudbury neutrino observatory phase I dataset, Phys. Rev. C 75, 045502 (2007).
  62. B. Aharmim et al. (The SNO Collaboration), An independent measurement of the total active B-8 solar neutrino flux using an array of He-3 proportional counters at the Sudbury Neutrino Observatory, Phys. Rev. Lett. 101, 111301 (2008).
  63. B. Aharmim et al. (The SNO Collaboration), Measurement of the νe and Total B8 solar neutrino fluxes with the Sudbury Neutrino observatory phase-III dataset, Phys. Rev. C 87, 015502 (2013).
  64. M. Agostini et al. (The Borexino Collaboration), Improved measurement of B8 solar neutrinos with 1.5kt·y of Borexino exposure, Phys. Rev. D 101, 062001 (2020).
  65. S. Abe et al. (The KamLAND Collaboration), Measurement of the B8 solar neutrino flux with the KamLAND liquid scintillator detector, Phys. Rev. C 84, 035804 (2011).
  66. M. Anderson et al. (The SNO+ Collaboration), Measurement of the B8 solar neutrino flux in SNO+ with very low backgrounds, Phys. Rev. D 99, 012012 (2019).
  67. Sunspot index and long-term solar observations, http://www.sidc.be/silso/datafiles (2021).
  68. A. Renshaw et al. (The Super-Kamiokande Collaboration), First indication of terrestrial matter effects on solar neutrino oscillation, Phys. Rev. Lett. 112, 091805 (2014).
  69. G. Bellini et al. (The Borexino Collaboration), Absence of day–night asymmetry of 862 keV Be7 solar neutrino rate in Borexino and MSW oscillation parameters, Phys. Lett. B 707, 22 (2012).
  70. J. N. Bahcall and P. I. Krastev, Do HEP neutrinos affect the solar neutrino energy spectrum?, Phys. Lett. B 436, 243 (1998).
  71. M. B. Smy et al. (The Super-Kamiokande Collaboration), Precise measurement of the solar neutrino day/night and seasonal variation in Super-Kamiokande-1, Phys. Rev. D 69, 011104 (2004).
  72. G. L. Fogli, E. Lisi, D. Montanino, and A. Palazzo, Quasivacuum solar neutrino oscillations, Phys. Rev. D 62, 113004 (2000).
  73. P. A. Zyla et al. (Particle Data Group), Review of particle physics, Prog. Theor. Exp. Phys. 2020, 083C01 (2020).
  74. B. Aharmim et al. (The SNO Collaboration), Search for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory, Phys. Rev. D 102, 062006 (2020).
  75. A. Gando et al. (The KamLAND Collaboration), Constraints on θ13 from a three-flavor oscillation analysis of reactor antineutrinos at KamLAND, Phys. Rev. D 83, 052002 (2011).
  76. K. Abe et al. (The Super-Kamiokande Collaboration), Solar neutrino measurements in Super-Kamiokande-IV, Phys. Rev. D 94, 052010 (2016).
  77. M. Agostini et al. (The BOREXINO Collaboration), Simultaneous precision spectroscopy of pp, Be7, and pep solar neutrinos with Borexino Phase-II, Phys. Rev. D 100, 082004 (2019).
  78. B. T. Cleveland, T. Daily, R. Davis, Jr., J. R. Distel, K. Lande, C. K. Lee, P. S. Wildenhain, and J. Ullman, Measurement of the solar electron neutrino flux with the Homestake chlorine detector, Astrophys. J. 496, 505 (1998).
  79. M. Altmann et al. (The GNO Collaboration), Complete results for five years of GNO solar neutrino observations, Phys. Lett. B 616, 174 (2005).
  80. J. N. Abdurashitov, V. N. Gavrin, V. V. Gorbachev, P. P. Gurkina, T. V. Ibragimova, A. V. Kalikhov et al. (The SAGE Collaboration), Measurement of the solar neutrino capture rate with gallium metal. III: Results for the 2002–2007 data-taking period, Phys. Rev. C 80, 015807 (2009).
  81. G. L. Fogli, E. Lisi, A. Marrone, D. Montanino, and A. Palazzo, Getting the most from the statistical analysis of solar neutrino oscillations, Phys. Rev. D 66, 053010 (2002).
  82. A. M. Dziewonski and D. L. Anderson, Preliminary reference earth model, Phys. Earth Planet. Interiors 25, 297 (1981).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation