Super-Kamiokande

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2015 Nobel Prize in Physics


Super-Kamiokande - Sudbury Neutrino Observatory

"for the discovery of neutrino oscillations, which shows that neutrinos have mass"

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References

1 - Reviews

[1-1]
Observation of atmospheric neutrinos, T. Kajita, Y. Totsuka, Rev. Mod. Phys. 73 (2001) 85-118.
[Kajita:2000mr]

2 - Reviews - Conference Proceedings

[2-1]
Atmospheric Neutrinos in 2002, Edward T. Kearns, Frascati Phys. Ser. 28 (2002) 413-426, arXiv:hep-ex/0210019. Heavy Quarks and Leptons 2002, Vietri sul Mare, Italy, May 27-June 1, 2002. http://hep.bu.edu/~kearns/pub/kearns-atmnu2002-hql.pdf.
From the article: ... recent developments in neutrino flux calculation is a key input to more detailed understanding of the data.... in neutrino oscillation studies the flux normalization is allowed to float as a free parameter.
Comment: In Ref.[Fukuda and others, Phys. Rev. Lett.81, 1562 (1998)] the overall normalization was estimated to have a 25% uncertainty but was fitted as a free parameter. An interesting question is whether now, after recent Monte Carlo calculations, the error on the total normalization could be reduced of a relevant factor and be used in the fit of neutrino oscillation studies.
Slide n.9 shows results of SK Fit using 3D Flux Calculations.
(M.L.).

[Kearns:2002jh]

3 - Atmospheric Neutrinos

[3-1]
Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation, E. Richard et al. (Super-Kamiokande), Phys. Rev. D94 (2016) 052001, arXiv:1510.08127.
[Richard:2015aua]
[3-2]
Test of Lorentz Invariance with Atmospheric Neutrinos, K. Abe et al. (Super-Kamiokande), Phys. Rev. D91 (2015) 052003, arXiv:1410.4267.
[Abe:2014wla]
[3-3]
Limits on Sterile Neutrino Mixing using Atmospheric Neutrinos in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D91 (2015) 052019, arXiv:1410.2008.
[Abe:2014gda]
[3-4]
A Measurement of the Appearance of Atmospheric Tau Neutrinos by Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 110 (2013) 181802, arXiv:1206.0328.
[Abe:2012jj]
[3-5]
Study of Non-Standard Neutrino Interactions with Atmospheric Neutrino Data in Super-Kamiokande I and II, G. Mitsuka et al. (Kamiokande), Phys. Rev. D84 (2011) 113008, arXiv:1109.1889.
[Mitsuka:2011ty]
[3-6]
Search for Differences in Oscillation Parameters for Atmospheric Neutrinos and Antineutrinos at Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 107 (2011) 241801, arXiv:1109.1621.
[Abe:2011ph]
[3-7]
Atmospheric neutrino oscillation analysis with sub-leading effects in Super-Kamiokande I, II, and III, R. Wendell et al. (Super-Kamiokande), Phys. Rev. D81 (2010) 092004, arXiv:1002.3471.
[Wendell:2010md]
[3-8]
Kinematic reconstruction of atmospheric neutrino events in a large water Cherenkov detector with proton identification, M. Fechner et al. (Super-Kamiokande), Phys. Rev. D79 (2009) 112010, arXiv:0901.1645.
[Fechner:2009aa]
[3-9]
Search for Matter-Dependent Atmospheric Neutrino Oscillations in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D77 (2008) 052001, arXiv:0801.0776.
[Abe:2008zza]
[3-10]
A Measurement of Atmospheric Neutrino Flux Consistent with Tau Neutrino Appearance, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 97 (2006) 171801, arXiv:hep-ex/0607059.
From the abstract: The Super-Kamiokande-I atmospheric neutrino data for 1489.2 days, which find a best fit tau neutrino appearance signal of $ 138 \pm 48 \text{(stat.)} {}^{+15}_{-32} \text{(sys.)} $, disfavor the hypothesis of no tau neutrino appearance by 2.4 sigma.
[Abe:2006fu]
[3-11]
Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande, J. Hosaka et al. (Super-Kamiokande), Phys. Rev. D74 (2006) 032002, arXiv:hep-ex/0604011.
[Hosaka:2006zd]
[3-12]
A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I, Y. Ashie et al. (Super-Kamiokande), Phys. Rev. D71 (2005) 112005, arXiv:hep-ex/0501064.
[Ashie:2005ik]
[3-13]
Evidence for an oscillatory signature in atmospheric neutrino oscillation, Y. Ashie et al. (Super-Kamiokande), Phys. Rev. Lett. 93 (2004) 101801, arXiv:hep-ex/0404034.
From the abstract: Muon neutrino disappearance probability as a function of neutrino flight length $L$ over neutrino energy $E$ was studied.
A dip in the $L/E$ distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation.
The observed $L/E$ distribution constrained $\nu_\mu \leftrightarrow \nu_\tau$ neutrino oscillation parameters; $1.9 \times 10^{-3} < \Delta m^2 < 3.0 \times 10^{-3} \, \mathrm{eV}^2$ and $\sin^22\theta > 0.90$ at 90% confidence level.

[Ashie:2004mr]
[3-14]
Tau neutrinos favored over sterile neutrinos in atmospheric muon neutrino oscillations, S. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 85 (2000) 3999-4003, arXiv:hep-ex/0009001.
[Fukuda:2000np]
[3-15]
Neutrino-induced upward stopping muons in Super-Kamiokande, Y. Fukuda et al. (Super-Kamiokande), Phys. Lett. B467 (1999) 185-193, arXiv:hep-ex/9908049.
[Fukuda:1999pp]
[3-16]
Observation of the east-west anisotropy of the atmospheric neutrino flux, T. Futagami et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 5194-5197, arXiv:astro-ph/9901139.
[Futagami:1999wz]
[3-17]
Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2644-2648, arXiv:hep-ex/9812014.
[Fukuda:1998ah]
[3-18]
Evidence for oscillation of atmospheric neutrinos, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1562-1567, arXiv:hep-ex/9807003.
[Fukuda:1998mi]
[3-19]
Study of the atmospheric neutrino flux in the multi-GeV energy range, Y. Fukuda et al. (Super-Kamiokande), Phys. Lett. B436 (1998) 33-41, arXiv:hep-ex/9805006.
[Fukuda:1998ub]
[3-20]
Measurement of a small atmospheric $\nu_\mu$ / $\nu_e$ ratio, Y. Fukuda et al. (Super-Kamiokande), Phys. Lett. B433 (1998) 9-18, arXiv:hep-ex/9803006.
[Fukuda:1998tw]

4 - Atmospheric Neutrinos - Conference Proceedings

[4-1]
Atmospheric Results from Super-Kamiokande, Roger Wendell (Super-Kamiokande), AIP Conf. Proc. 1666 (2015) 100001, arXiv:1412.5234. XXVI International Conference on Neutrino Physics and Astrophysics (Neutrino 2014).
[Wendell:2014dka]
[4-2]
Recent Atmospheric Neutrino Results from Super-Kamiokande, Alexander Himmel (Super-Kamiokande), AIP Conf.Proc. 1604 (2014) 345-352, arXiv:1310.6677. VII International Conference on Interconnections between Particle Physics and Cosmology (PPC2013).
[Himmel:2013jva]
[4-3]
Results from Super-Kamiokande, Yasuo Takeuchi (Super-Kamiokande), Nucl. Phys.B, Proc.Suppl.229-232 2012 (2012) 79-84, arXiv:1112.3425. XXIV International Conference on Neutrino Physics and Astrophysics (Neutrino 2010).
[Takeuchi:2011aa]
[4-4]
SuperK recent results, K. Scholberg (Super-Kamiokande), 2005. 20th International Workshop on Weak Interactions and Neutrinos (WIN'05), June 6-11, 2005, Delphi, Greece. http://conferences.phys.uoa.gr/win05/WIN05_WG3/scholberg.ppt.
Comment: Atmospheric neutrino results from a new (320 bins) analysis are presented. [M.L.].
[Scholberg:WIN2005]
[4-5]
Upward Showering Muons in Super-Kamiokande, S. Desai, A. Habig (Super-Kamiokande), 2005. 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, 3-11 Aug 2005. http://budoe.bu.edu/~shantanu/icrc05showering.sxi.pdf.
[DesaiHabig-ICRC05:]
[4-6]
Direct oscillatory evidence from the L/E analysis in Super-Kamiokande, M. Ishitsuka (Super-Kamiokande), 2004. NOON2004, The 5th Workshop on 'Neutrino Oscillations and their Origin', 11-15 February 2004, Tokyo, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2004/trape/10-ishitsuka.pdf.
Comment: First oscillation dip is observed in L/E data sample (see this figure).
[Ishitsuka-NOON2004]
[4-7]
SK atmospheric neutrino, C. Saji (Super-Kamiokande), 2004. NOON2004, The 5th Workshop on 'Neutrino Oscillations and their Origin', 11-15 February 2004, Tokyo, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2004/trape/09-Saji.pdf.
[Saji-NOON2004]
[4-8]
Atmospheric neutrino results from SuperKamiokande, E. Kearns (Super-Kamiokande), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/kearns.pdf.
[Kearns-Nu2004]
[4-9]
Upward Showering Muons in Super-Kamiokande, S. Desai (Super-Kamiokande), 2003. 28th International Cosmic Ray Conferences (ICRC 2003) 31 Jul - 7 Aug 2003, Tsukuba, Japan. http://budoe.bu.edu/~shantanu/icrc.pdf.
[Desai-ICRC2003]
[4-10]
Recent results from atmospheric $\nu$ and K2K, Y. Itow, 2003. 2nd International conference on Flavor Physics, ICFP 2003, 6-11 October 2003, Korea Institute for Advanced Study (KIAS). http://newton.kias.re.kr/~hepph/public_html/03icfp/talk/itow1.pdf.
Comment: The figure in slide n.34 shows the K2K excluded region for oscillations of accelerator neutrinos in the $\nu_{\mu} \to \nu_e$ channel as compared with the CHOOZ limit and the Super-Kamiokande allowed region. [M.L.].
[Itow:ICFP2003]
[4-11]
Atmospheric Neutrino Oscillations in Super-Kamiokande I, A. Ahabig (Super-Kamiokande), 2003. 28th International Cosmic Ray Conferences (ICRC 2003) 31 Jul - 7 Aug 2003, Tsukuba, Japan. http://neutrino.d.umn.edu/~habig/atmpd.pdf.
[Ahabig:ICRC2003]
[4-12]
New Results from Super-K and K2K, R. Jeffrey Wilkes (K2K), eConf C020805 (2002) TTH02, arXiv:hep-ex/0212035. Secrets of the B-Meson, Topical Conference, XXX SLAC Summer Institute, SLAC, August, 2002.
[Wilkes:2002mb]
[4-13]
Experimental results on atmospheric neutrinos in Super-Kamiokande-I, M. Shiozawa (Super-Kamiokande), 2002. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/shiozawa.
[Shiozawa-Nu2002]
[4-14]
Atmospheric Neutrinos at Super-Kamiokande, C. Mauger (Super-Kamiokande), 2002. 31st International Conference on High Energy Physics - ICHEP 02 - Amsterdam, Holland, 24-31 July 2002. http://www.ichep02.nl/Transparencies/NEU/NEU-1/NEU-1-4.Mauger.pdf.
[Mauger-ICHEP-2002]
[4-15]
Super-Kamiokande atmospheric neutrino results, Toshiyuki Toshito (Super-Kamiokande), arXiv:hep-ex/0105023, 2001.
[Toshito:2001dk]
[4-16]
Study of neutrino oscillations with the atmospheric neutrino data from Super-Kamiokande, T. Kajita (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 100 (2001) 107-112.
[Kajita:2001zv]
[4-17]
Atmospheric neutrinos in Super-Kamiokande, H. Sobel (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 91 (2001) 127-133.
[Sobel:2001tj]
[4-18]
Future atmospheric neutrino data from Super-Kamiokande, T. Kajita (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 100 (2001) 139-141.
[Kajita:2001ab]
[4-19]
Atmospheric neutrino results from Super-Kamiokande, M. D. Messier, Int. J. Mod. Phys. A16S1B (2001) 733-735.
[Messier:2001pk]
[4-20]
Atmospheric neutrinos at Super-Kamiokande, Kate Scholberg (Super-Kamiokande), arXiv:hep-ex/9905016, 1999.
[Scholberg:1999ar]
[4-21]
Upward coming muons in Super-Kamiokande and muon neutrino oscillations, A. Okada (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Okada:1999fb]
[4-22]
Observation of atmospheric neutrinos in Super-Kamiokande and the neutrino oscillation parameters, K. Kaneyuki (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Kaneyuki:1999fe]
[4-23]
Evidence for neutrino oscillations in atmospheric neutrino observations, M. Shiozawa (Super-Kamiokande and Kamiokande), Nucl. Instrum. Meth. A433 (1999) 307-313. 3rd International Workshop on Ring Imaging Cerenkov Detector (RICH 98), Ein Gedi, Dead Sea, Israel, 15-20 Nov 1998.
[Shiozawa:1999sp]
[4-24]
Multi-ring atmospheric neutrino events in Super- Kamiokande, C. Mauger (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Mauger:1999fa]
[4-25]
Observation of east-west effect in atmospheric neutrinos by Super-Kamiokande, K. Kaneyuki (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Kaneyuki:1999ez]
[4-26]
Atmospheric neutrino results from Super-Kamiokande and Kamiokande: Evidence for $\nu_\mu$ oscillations, Takaaki Kajita (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 77 (1999) 123-132, arXiv:hep-ex/9810001.
[Kajita:1998bw]
[4-27]
Atmospheric neutrino results from Super-Kamiokande, T. Kajita (Super-Kamiokande), 1998. Given at International Workshop on JHF Science (JHF 98), Tsukuba, Japan, 4-7 Mar 1998.
[Kajita:1998fr]
[4-28]
Atmospheric neutrino flux studies with the Super-Kamiokande detector, L. Wai (Super-Kamiokande), 1997. Prepared for Orbis Scientiae on Physics of Mass, Miami, Florida, 12-15 Dec 1997.
[Wai:1997cn]

5 - Solar Neutrinos

[5-1]
Solar Neutrino Measurements in Super-Kamiokande-IV, K. Abe et al. (Super-Kamiokande), Phys. Rev. D94 (2016) 052010, arXiv:1606.07538.
[Abe:2016nxk]
[5-2]
First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation, A. Renshaw et al. (Super-Kamiokande), Phys. Rev. Lett. 112 (2014) 091805, arXiv:1312.5176.
[Renshaw:2013dzu]
[5-3]
Solar neutrino results in Super-Kamiokande-III, K. Abe et al. (Super-Kamiokande), Phys. Rev. D83 (2011) 052010, arXiv:1010.0118.
[Abe:2010hy]
[5-4]
Solar neutrino measurements in Super-Kamiokande-II, J.P. Cravens et al. (Super-Kamiokande), Phys. Rev. D78 (2008) 032002, arXiv:0803.4312.
From the abstract: The results of the second phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first phase. The solar neutrino flux spectrum and time-variation as well as oscillation results are statistically consistent with the first phase and do not show spectral distortion. The time-dependent flux measurement of the combined first and second phases coincides with the full period of solar cycle 23 and shows no correlation with solar activity.
[Cravens:2008aa]
[5-5]
Solar neutrino measurements in Super-Kamiokande-I, J. Hosaka et al. (Super-Kamkiokande), Phys. Rev. D73 (2006) 112001, arXiv:hep-ex/0508053.
[Hosaka:2005um]
[5-6]
Limit On the Neutrino Magnetic Moment Using 1496 Days of Super-Kamiokande-I Solar Neutrino Data, D. W. Liu et al. (Super-Kamiokande), Phys. Rev. Lett. 93 (2004) 021802, arXiv:hep-ex/0402015.
[Liu:2004ny]
[5-7]
Precise Measurement of the Solar Neutrino Day/Night and Seasonal Variation in Super-Kamiokande-I, M.B. Smy et al. (Super-Kamiokande), Phys. Rev. D69 (2004) 011104, arXiv:hep-ex/0309011.
[Smy:2003jf]
[5-8]
A search for periodic modulations of the solar neutrino flux in Super-Kamiokande-I, J. Yoo et al. (Super-Kamiokande), Phys. Rev. D68 (2003) 092002, arXiv:hep-ex/0307070.
[Yoo:2003rc]
[5-9]
Search for anti-nu/e from the sun at Super-Kamiokande-I, Y. Gando et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 171302, arXiv:hep-ex/0212067.
From the article: For the ${}^8\mathrm{B}$ spectrum the upper limit to the solar $\bar{\nu}_e$ flux is $8 \times 10^{-3}$ of the SSM $\nu_e$ flux prediction for total energy = 8 Mev - 20 MeV.
[Gando:2002ub]
[5-10]
Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data, S. Fukuda et al. (Super-Kamiokande), Phys. Lett. B539 (2002) 179-187, arXiv:hep-ex/0205075.
[Fukuda:2002pe]
[5-11]
Constraints on neutrino oscillations using 1258 days of Super-Kamiokande solar neutrino data, S. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 86 (2001) 5656-5660, arXiv:hep-ex/0103033.
[Fukuda:2001nk]
[5-12]
Solar B-8 and hep neutrino measurements from 1258 days of Super-Kamiokande data, S. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 86 (2001) 5651-5655, arXiv:hep-ex/0103032.
[Fukuda:2001nj]
[5-13]
Measurement of the solar neutrino energy spectrum using neutrino electron scattering, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2430-2434, arXiv:hep-ex/9812011.
[Fukuda:1998ua]
[5-14]
Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super-Kamiokande, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 1810-1814, arXiv:hep-ex/9812009.
[Fukuda:1998rq]
[5-15]
Measurements of the solar neutrino flux from Super-Kamiokande's first 300 days, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1158-1162, arXiv:hep-ex/9805021.
[Fukuda:1998fd]

6 - Solar Neutrinos - Conference Proceedings

[6-1]
Solar Neutrino Results from Super-Kamiokande, Andrew Renshaw (Super-Kamiokande), Phys.Procedia 61 (2015) 345-354, arXiv:1403.4575.
[Renshaw:2014awa]
[6-2]
Solar neutrino analysis of Super-Kamiokande, Hiroyuki Sekiya (Super-Kamiokande), arXiv:1307.3686, 2013. 33rd International Cosmic Ray Conference, Rio De Janeiro 2013 (ICRC2013).
[Sekiya:2013hda]
[6-3]
Solar Neutrino Measurement at SK-III, B.S. Yang (Super-Kamiokande), arXiv:0909.5469, 2009. DPF-2009, Detroit, MI, July 2009.
[Yang:2009hp]
[6-4]
SuperKamiokande's solar neutrino results, M. Nakahata (Super-Kamiokande), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/nakahata.pdf.
[Nakahata-Nu2004]
[6-5]
The Solar Neutrino Day/Night Effect in Super-Kamiokande, M. B. Smy (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 138 (2005) 91, arXiv:hep-ex/0310064. TAUP 2003.
[Smy:2003sb]
[6-6]
A study of short-time periodic variation of the B8 solar neutrino flux at Super-Kamiokande, J. Yoo (Super-Kamiokande), eConf C030626 (2003) FRAP01, arXiv:hep-ex/0309048. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Yoo:2003ky]
[6-7]
The recent results of solar neutrino measurements in Super-Kamiokande, Y. Koshio (Super-Kamiokande), arXiv:hep-ex/0306002, 2003. XXXVIIIth Recontres de Moriond Electroweak Interactions and Unified Theories.
[Koshio:2003py]
[6-8]
Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data, M. B. Smy (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 118 (2003) 25, arXiv:hep-ex/0208004. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/smy.
[Smy:2002rz]
[6-9]
Implications for solar neutrino oscillations from Super-Kamiokande and SNO data, M. B. Smy (Super-Kamiokande), arXiv:hep-ex/0108053, 2001.
[Smy:2001yn]
[6-10]
Solar neutrino results from super-Kamiokande, M. B. Smy (Super-Kamiokande), arXiv:hep-ex/0106064, 2001.
[Smy:2001wf]
[6-11]
Solar neutrino results (from radio-chemical and water Cherenkov detectors), Y. Suzuki, Nucl. Phys. Proc. Suppl. 100 (2001) 14-23.
[Suzuki:2001kf]
[6-12]
Solar Neutrino Results from Super-Kamiokande, Y. Suzuki, Nucl. Phys. Proc. Suppl. 91 (2001) 29-35.
[Suzuki:2000xw]
[6-13]
Recent Super-Kamiokande results on solar neutrinos, Y. Koshio (Super-Kamiokande), 2000. 14th Rencontres de Physique de la Valle d'Aoste: Results and Perspectives in Particle Physics, La Thuile, Valle d'Aoste, Italy, 27 Feb - 4 Mar 2000.
[Koshio:2000an]
[6-14]
Solar neutrinos with Super-Kamiokande, M. B. Smy, arXiv:hep-ex/9903034, 1999.
[Smy:1999tt]
[6-15]
Solar neutrino results from Super-Kamiokande, Y. Suzuki (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 77 (1999) 35-42.
[Suzuki:1999cy]
[6-16]
Solar neutrinos at Super-Kamiokande, K. Inoue (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 70 (1999) 273-283.
[Inoue:1999ak]
[6-17]
Solar neutrinos results and oscillation analysis from Super-Kamiokande, Y. Koshio (Super-Kamiokande), 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Koshio:1999ff]
[6-18]
Solar neutrino measurements from Super-Kamiokande, M. R. Vagins (Super-Kamiokande), 1998. Prepared for 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, British Columbia, Canada, 23-29 Jul 1998.
[Vagins:1998kz]
[6-19]
Super-Kamiokande solar neutrino analysis: The first 201.6 days' results, R. E. Sanford (Super-Kamiokande), 1997. Sixth Conference on the Intersections of Particle and Nuclear Physics (CIPANP 97), Big Sky, MT, 27 May - 2 June 1997.
[Sanford:1997mm]
[6-20]
Kamiokande-II results on solar neutrinos and the Super-Kamiokande experiment, Y. Suzuki, 1991. 11th Moriond Workshop on Tests of Fundamental Laws in Physics, Les Arcs, France, Jan 26 - Feb 2, 1991.
[Suzuki:1991xy]

7 - Supernova Neutrinos

[7-1]
Real-Time Supernova Neutrino Burst Monitor at Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Astropart.Phys. 81 (2016) 39-48, arXiv:1601.04778.
[Abe:2016waf]
[7-2]
Supernova Relic Neutrino Search with Neutron Tagging at Super-Kamiokande-IV, H. Zhang et al. (Super-Kamiokande), Astropart.Phys. 60 (2015) 41, arXiv:1311.3738.
[Zhang:2013tua]
[7-3]
Search for Supernova Neutrino Bursts at Super-Kamiokande, M. Ikeda, A. Takeda, Y. Fukuda, M. R. Vagins, M. Sakuda (Super-Kamiokande), Astrophys. J. 669 (2007) 519-524, arXiv:0706.2283.
[Ikeda:2007sa]
[7-4]
Search for supernova relic neutrinos at Super-Kamiokande, M. Malek et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 061101, arXiv:hep-ex/0209028.
[Malek:2002ns]

8 - Astrophysical Neutrinos

[8-1]
Search for an excess of events in the Super-Kamiokande detector in the directions of the astrophysical neutrinos reported by the IceCube Collaboration, K. Abe et al. (Super-Kamiokande), arXiv:1707.08604, 2017.
[1707.08604]
[8-2]
Search for Neutrinos in Super-Kamiokande associated with Gravitational Wave Events GW150914 and GW151226, K. Abe et al. (Super-Kamiokande), arXiv:1608.08745, 2016.
[1608.08745]
[8-3]
Search for Astrophysical Neutrino Point Sources at Super-Kamiokande, E. Thrane et al. (Super-Kamiokande), Astrophys. J. 704 (2009) 503-512, arXiv:0907.1594.
[Thrane:2009tw]
[8-4]
Study of TeV Neutrinos with Upward Showering Muons in Super-Kamiokande, S. Desai et al. (Super-Kamiokande), Astropart. Phys. 29 (2008) 42-54, arXiv:0711.0053.
[Desai:2007ra]
[8-5]
High energy neutrino astronomy using upward-going muons in Super-Kamiokande-I, K. Abe et al. (Super-Kamiokande), Astrophys. J. 652 (2006) 198, arXiv:astro-ph/0606413.
[Abe:2006at]
[8-6]
Search for diffuse astrophysical neutrino flux using ultra- high energy upward-going muons in Super-Kamiokande I, M. E. C. Swanson (Super-Kamiokande), Astrophys. J. 652 (2006) 206-215, arXiv:astro-ph/0606126.
[Swanson:2006gm]
[8-7]
High-Energy Neutrino Astronomy with the Super-Kamiokande Detector, A. Habig (Super-Kamiokande), arXiv:astro-ph/0507051, 2005. 29th ICRC, Pune, India.
[Habig:2005fc]

9 - Dark Matter

[9-1]
Search for neutrinos from annihilation of captured low-mass dark matter particles in the Sun by Super-Kamiokande, K. Choi et al. (Super-Kamiokande), Phys. Rev. Lett. 114 (2015) 141301, arXiv:1503.04858.
[Choi:2015ara]
[9-2]
An Indirect Search for WIMPs in the Sun using 3109.6 days of upward-going muons in Super-Kamiokande, T. Tanaka et al. (Kamiokande), Astrophys. J. 742 (2011) 78, arXiv:1108.3384.
[Tanaka:2011uf]
[9-3]
Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande, S. Desai et al. (Super-Kamiokande), Phys. Rev. D70 (2004) 083523, arXiv:hep-ex/0404025.
[Desai:2004pq]

10 - Dark Matter - Conference Proceedings

[10-1]
Searching for Dark Matter Annihilation into Neutrinos with Super-Kamiokande, Katarzyna Frankiewicz (Super-Kamiokande), arXiv:1510.07999, 2015. DPF 2015 Meeting of the American Physical Society Division of Particles and Fields, Ann Arbor, Michigan, August 4-8, 2015.
[Frankiewicz:2015zma]

11 - Nucleon Decay

[11-1]
Search for Proton Decay via $p \to e^+\pi^0$ and $p \to \mu^+\pi^0$ in 0.31 megaton$\cdot$years exposure of the Super-Kamiokande Water Cherenkov Detector, K. Abe et al. (Super-Kamiokande), Phys. Rev. D95 (2017) 012004, arXiv:1610.03597.
[Miura:2016krn]
[11-2]
Search for Nucleon and Di-nucleon Decays with an Invisible Particle and a Charged Lepton in the Final State at the Super-Kamiokande Experiment, V. Takhistov et al. (Super-Kamiokande), Phys. Rev. Lett. 115 (2015) 121803, arXiv:1508.05530.
[Takhistov:2015fao]
[11-3]
Search for dinucleon decay into pions at Super-Kamiokande, J. Gustafson et al. (Super-Kamiokande), Phys. Rev.D (2015), arXiv:1504.01041.
[Gustafson:2015qyo]
[11-4]
A Search for Nucleon Decay via $n \rightarrow \bar\nu pi^{0}$ and $p \rightarrow \bar\nu pi^{+}$ in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 113 (2014) 121802, arXiv:1305.4391.
[Abe:2013lua]
[11-5]
Search for Proton Decay into Muon plus Neutral Kaon in Super-Kamiokande I, II, and III, C.Regis et al. (Super-Kamiokande), Phys. Rev. D86 (2012) 012006, arXiv:1205.6538.
[Regis:2012sn]
[11-6]
Search for Nucleon Decay into Charged Anti-lepton plus Meson in Super-Kamiokande I and II, H. Nishino et al. (Super-Kamiokande), Phys. Rev. D85 (2012) 112001, arXiv:1203.4030.
[Nishino:2012ipa]
[11-7]
Search for nucleon decay via modes favored by supersymmetric grand unification models in Super-Kamiokande-I, K. Kobayashi et al. (Super-Kamiokande), Phys. Rev. D72 (2005) 052007, arXiv:hep-ex/0502026.
[Kobayashi:2005pe]
[11-8]
Search for proton decay through p - > anti-nu K+ in a large water Cherenkov detector, Y. Hayato et al. (Super-Kamiokande), Phys. Rev. Lett. 83 (1999) 1529-1533, arXiv:hep-ex/9904020.
[Hayato:1999az]
[11-9]
Search for proton decay via p - > e+ pi0 in a large water Cherenkov detector, M. Shiozawa et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 3319-3323, arXiv:hep-ex/9806014.
[Shiozawa:1998si]

12 - Nucleon Decay - Conference Proceedings

[12-1]
Review of Nucleon Decay Searches at Super-Kamiokande, Volodymyr Takhistov (Super-Kamiokande), arXiv:1605.03235, 2016. 51st Rencontres de Moriond: Electroweak Interactions and Unified Theories (La Thuile, Italy, March 12-19, 2016).
[Takhistov:2016eqm]

13 - Physics

[13-1]
Search for GUT Monopoles at Super-Kamiokande, K. Ueno et al. (Super-Kamiokande), Astropart. Phys. 36 (2012) 131-136, arXiv:1203.0940.
[Ueno:2012md]
[13-2]
The search for n-nbar oscillation in Super-Kamiokande I, Super-Kamiokande collaboration et al. (Super-Kamiokande), Phys. Rev. D91 (2015) 072006, arXiv:1109.4227.
[Abe:2011ky]
[13-3]
Search for Neutral Q-balls in Super-Kamiokande II, Y. Takenaga et al. (Super-Kamiokande), Phys. Lett. B647 (2007) 18-22, arXiv:hep-ex/0608057.
[Takenaga:2006nr]

14 - Cosmic Rays

[14-1]
First measurement of radioactive isotope production through cosmic-ray muon spallation in Super-Kamiokande IV, Y. Zhang et al. (Super-Kamiokande), Phys. Rev. D93 (2016) 012004, arXiv:1509.08168.
[Super-Kamiokande:2015xra]
[14-2]
Observation of the Anisotropy of 10 TeV Primary Cosmic Ray Nuclei Flux with the Super-Kamiokande-I Detector, Gene Guillian et al. (Super-Kamiokande), Phys. Rev. D75 (2007) 062003, arXiv:astro-ph/0508468.
[Guillian:2005wp]

15 - Cosmic Rays - Conference Proceedings

[15-1]
Anisotropy of the primary cosmic-ray flux in Super-Kamiokande, Yuichi Oyama (Super-Kamiokande), arXiv:astro-ph/0605020, 2006. 'Les Rencontres de Physique de la Vallee d'Aosta (La Thuile 2006)', La Thuile, Aosta Valley, Italy, March 5-11, 2006.
[Oyama:2006mm]

16 - Detector

[16-1]
Calibration of the Super-Kamiokande Detector, K. Abe et al. (Super-Kamiokande), Nucl.Instrum.Meth. A737 (2014) 253-272, arXiv:1307.0162.
[Abe:2013gga]
[16-2]
First Study of Neutron Tagging with a Water Cherenkov Detector, H. Watanabe, H. Zhang (Super-Kamiokande), Astropart. Phys. 31 (2009) 320-328, arXiv:0811.0735.
[Watanabe:2008ru]
[16-3]
The Super-Kamiokande detector, S. Fukuda et al. (SuperKamiokade), Nucl. Instrum. Meth. A501 (2003) 418-462. http://www-sk.icrr.u-tokyo.ac.jp/doc/sk/pub/sknimpaper.pdf.
[Fukuda:2002uc]
[16-4]
Measurement of radon concentrations at Super-Kamiokande, Y. Takeuchi et al. (SuperKamiokade), Phys. Lett. B452 (1999) 418-424, arXiv:hep-ex/9903006.
[Takeuchi:1999zq]
[16-5]
Reconstruction algorithms in the Super-Kamiokande large water Cherenkov detector, M. Shiozawa (Super-Kamiokande), Nucl. Instrum. Meth. A433 (1999) 240-246.
[Shiozawa:1999sd]
[16-6]
Calibration of Super-Kamiokande using an electron linac, M. Nakahata et al. (Super-Kamiokande), Nucl. Instrum. Meth. A421 (1999) 113-129, arXiv:hep-ex/9807027.
[Nakahata:1998pz]

17 - Detector - Conference Proceedings

[17-1]
Gadolinium study for a water Cherenkov detector, Atsuko Kibayashi (Super-Kamiokande), arXiv:0909.5528, 2009. DPF-2009, Detroit, MI, July 2009.
[Kibayashi:2009ih]

18 - Experimental Test

[18-1]
A Study on the e / mu identification capability of a water Cerenkov detector and the atmospheric neutrino problem, S. Kasuga et al., Phys. Lett. B374 (1996) 238-242.
[Kasuga:1996dm]

19 - Background

[19-1]
Muon Simulations for Super-Kamiokande, KamLAND and CHOOZ, Alfred Tang, Glenn Horton-Smith, Vitaly A. Kudryavtsev, Alessandra Tonazzo, Phys. Rev. D74 (2006) 053007, arXiv:hep-ph/0604078.
[Tang:2006uu]

20 - Conference Proceedings

[20-1]
Low Energy Neutrino Astronomy in Super-Kamiokande, Michael Smy, arXiv:1110.0012, 2011. DPF 2011.
[Smy:2011tm]
[20-2]
Recent Results from Super-Kamiokande, H. Sekiya et al. (Super-Kamiokande), arXiv:0810.0595, 2008. ICHEP08, Philadelphia, USA, July 2008.
[Sekiya:2008nb]
[20-3]
The Super-Kamiokande Experiment, C.W. Walter (Super-Kamiokande), arXiv:0802.1041, 2008. Neutrino Oscillations: Present Status and Future Plans.
[Walter:2008ys]
[20-4]
Super Kamiokande results: atmospheric and solar neutrinos, M.Ishitsuka (Super-Kamiokande), arXiv:hep-ex/0406076, 2004. XXXIX Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, March 21-28-2004. http://moriond.in2p3.fr/EW/2004/transparencies/3_Wednesday/3_2_afternoon/3_2_3_Ishitsuka/Ishitsuka.pdf.
[Ishitsuka:2004un]
[20-5]
Upward showering muons in Super-Kamiokande, A. Habig (Super-Kamiokande), 2004. HEAD 2004. http://neutrino.d.umn.edu/~habig/sk-showering.pdf.
[Habig-HEAD2004]
[20-6]
Neutrino Physics: Experimental Status, T. Kajita, 2003. 19th International Workshop on Weak Interactions and Neutrinos, WIN2003, October 6-11, Lake Geneva, Wisconsin, USA. http://conferences.fnal.gov/win03/Talks/Takaaki%20Kajita.pdf.
Comment: The slide n. 19 shows the $ 90 \% $ C.L. allowed contours for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by different atmospheric neutrino experiments. The figure in slide n.24 shows the $ 90 \% $ C.L. allowed contour for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by Super-Kamiokande. [M.L.].
[Kajita:WIN2003]
[20-7]
Status of the Super-Kamiokande, the K2K-2 experiment and JHF nu project, Y. Hayato, 2003. EPS2003. http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07Hayato.ppt.
[Hayato:EPS2003]
[20-8]
Atmospheric and long baseline neutrino, T. Nakaya (Super-Kamiokande), eConf C020620 (2002) SAAT01, arXiv:hep-ex/0209036. 22nd Physics in Collision Conference (PIC 2002), Stanford, California, 20-22 June 2002.
[Nakaya:2002ki]
[20-9]
Five Years of Neutrino Physics with Super-Kamiokande, M. B. Smy (Super-Kamiokande), arXiv:hep-ex/0206016, 2002. XXXVII Rencontres de Moriond Electroweak Interactions and Unified Theories Les Arcs, March 9-16-2002. http://moriond.in2p3.fr/EW/2002/transparencies/3_Tuesday/morning/M_Smy/M_Smy.pdf.
[Smy:2002hr]
[20-10]
Results in Neutrino Oscillation from Super-Kamiokande I, Y. Itow, 2002. 2nd International Workshop on Nuclear and Particle Physics at 50-GeV PS, Kyoto University, Kyoto, Japan, September 27-29, 2002. http://jnusrv01.kek.jp/jnu/NP02/Sep27/itow.pdf.
[Itow-Kyoto2002]
[20-11]
The JHF-Kamioka Neutrino Project and Status of Super-Kamiokande, T. Kajita (Super-Kamiokande), 2002. Conference on Physics beyond the Standard Model - BEYOND THE DESERT 02 - Oulu, Finland, 2-7 June 2002. http://cupp.oulu.fi/trans/Kajita.pdf.
[Kajita-Oulu2002]
[20-12]
Recent results from the Super-Kamiokande experiment, Yuichi Oyama (Super-Kamiokande), arXiv:hep-ex/0104015, 2001.
[Oyama:2001bq]
[20-13]
Results from Super-Kamiokande, C. Yanagisawa, Nucl. Phys. Proc. Suppl. 95 (2001) 93-99.
[Yanagisawa:2001xy]
[20-14]
Recent results in Super-Kamiokande and K2K, Y. Itow (Super-Kamiokande and K2K), Phys. Scripta T93 (2001) 53-58.
[Itow:2001vr]
[20-15]
Neutrino mass and mixing measurements at Super-Kamiokande, R. Svoboda (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 98 (2001) 165-174.
[Svoboda:2001jj]
[20-16]
Results from Super-Kamiokande, Y. Totsuka, Nucl. Phys. A663 (2000) 218-230.
[Totsuka:2000qy]
[20-17]
Latest results from Super-Kamiokande, T. Kajita (Super-Kamiokande), AIP Conf. Proc. 539 (2000) 31-40.
[Kajita:2000pk]
[20-18]
Experimental results on neutrino oscillations using atmospheric, solar and accelerator beams, D. Kielczewska (Super-Kamiokande and K2K), Acta Phys. Polon. B31 (2000) 1181-1207.
[Kielczewska:2000ru]
[20-19]
Evidence for neutrino oscillation observed in Super- Kamiokande, Y. Totsuka, Phys. Scripta T85 (2000) 82-90. Nobel Symposium, Stockholm, August 20-25, 1998. http://www-sk.icrr.u-tokyo.ac.jp/doc/sk/pub/text.ps.gz.
[Totsuka:2000vt]
[20-20]
Results from Super-Kamiokande, T. Kajita (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 85 (2000) 44-51.
[Kajita:2000yb]
[20-21]
Search for dark matter WIMPs using upward-going muons in Super-Kamiokande, S. Desai (Super-Kamiokande), 2000. 4th International Symposium on Sources and Detection of Dark Matter in the Universe (DM 2000), Marina del Rey, California, 23-25 Feb 2000.
[Desai:2000mi]
[20-22]
Super-Kamiokande, M. Nakahata (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 87 (2000) 125-134.
[Nakahata:2000dt]
[20-23]
Neutrino oscillations at Super-Kamiokande, D. Kielczewska (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 81 (2000) 133-142.
[Kielczewska:2000mh]
[20-24]
Neutrino-induced upward going muons in Super-Kamiokande, A. Habig (Super-Kamiokande), arXiv:hep-ex/9903047, 1999.
[Habig:1999cq]
[20-25]
Current status of nucleon decay searches with Super- Kamiokande, Brett Viren (Super-Kamiokande), arXiv:hep-ex/9903029, 1999.
[Viren:1999pk]
[20-26]
The search for proton decay at Super-Kamiokande, K. S. Ganezer (Super-Kamiokande), 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Ganezer:1999fx]
[20-27]
News on solar neutrinos from Super-Kamiokande, K. Inoue, 1999. In 'Venice 1999, Neutrino telescopes, vol. 1' 53-62.
[Inoue:1999mr]
[20-28]
Solar and atmospheric neutrino oscillations: Super- Kamiokande results, Y. Suzuki (Super-Kamiokande), 1999. In 'Cape Town 1999, Weak interactions and neutrinos' 277- 290.
[Suzuki:1999xp]
[20-29]
Recent results from Super-Kamiokande, T. Kajita, Phys. Atom. Nucl. 62 (1999) 1963-1970.
[Kajita:1999dd]
[20-30]
Atmospheric neutrino oscillations at Super-Kamiokande, Y. Itow (Super-Kamiokande and K2K), 1999. In 'La Thuile 1999, Results and perspectives in particle physics' 3-20.
[Itow:1999ar]
[20-31]
Present status of solar and atmospheric neutrinos, M. Nakahata (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 76 (1999) 425-434.
[Nakahata:1999vd]
[20-32]
Recent results from Super-Kamiokande, M. Takita (Super-Kamiokande), 1998. 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, British Columbia, Canada, 23-29 Jul 1998.
[Takita:1998jv]
[20-33]
Search for p - > K+ anti-nu with Super-Kamiokande, Y. Hayato (Super-Kamiokande), 1998. Prepared for 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, British Columbia, Canada, 23-29 Jul 1998.
[Hayato:1998ra]
[20-34]
Results on neutrino oscillations from 400 days of Super-Kamiokande data, Y. Itow (Super-Kamiokande), 1997. Given at 25th SLAC Summer Institute on Particle Physics: Physics of Leptons (SSI 97), Stanford, CA, 4-15 Aug 1997.
[Itow:1997df]
[20-35]
Results from Super-Kamiokande, T. Kajita (Super-Kamiokande), 1997. Given at 17th International Conference on Physics in Collision (PIC 97), Bristol, England, 25-27 June 1997.
[Kajita:1997uv]
[20-36]
Results from Super-Kamiokande, K. Martens (Super-Kamiokande), 1997. International Europhysics Conference on High-Energy Physics (HEP 97), Jerusalem, Israel, 19-26 Aug 1997.
[Martens:1997dh]
[20-37]
Nucleon instability search with Super-Kamiokande, J. Stone, 1996. International Workshop on Future Prospects of Baryon Instability Search in p decay and n --> anti-n Oscillation Experiments, Oak Ridge, TN, 28-30 Mar 1996.
[Stone:1996ip]

21 - Slides

[21-1]
Results from Super-Kamiokande, Michael Smy (Super-Kamiokande), 2012. Neutrino 2012, XXV International Conference on Neutrino Physics and Astrophysics, 3-9 June 2012, Kyoto, Japan. http://kds.kek.jp/getFile.py/access?contribId=3&sessionId=2&resId=0&materialId=slides&confId=9151.
[Smy-NU2012]

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Last Update: Mon 21 Aug 2017, 09:42:44 UTC