Super-Kamiokande

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References

1 - Reviews
2 - Reviews - Conference Proceedings
3 - Atmospheric Neutrinos
4 - Atmospheric Neutrinos - Conference Proceedings
5 - Solar Neutrinos
6 - Solar Neutrinos - Conference Proceedings
7 - Supernova Neutrinos
8 - Astrophysical Neutrinos
9 - Physics
10 - Cosmic Rays
11 - Cosmic Rays - Conference Proceedings
12 - Detector
13 - Detector - Conference Proceedings
14 - Experimental Test
15 - Conference Proceedings
16 - Background

The references in each group are listed in approximate inverted chronological order.
Click on the reference label to search it in inSPIRE.

1 - Reviews

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

2 - Reviews - Conference Proceedings

[2-1]: Atmospheric Neutrinos in 2002, Kearns, Edward T., 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.).

3 - Atmospheric Neutrinos

[3-1]: 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.
[3-2]: 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.
[3-3]: 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.
[3-4]: 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.
[3-5]: Search for Matter-Dependent Atmospheric Neutrino Oscillations in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D77 (2008) 052001, arXiv:0801.0776.
[3-6]: 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 $138 +- 48 <b>(stat.)</b> {}^{+15}_{-32} \text{(sys.)}$ , disfavor the hypothesis of no tau neutrino appearance by 2.4 sigma.
[3-7]: 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.
[3-8]: 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.
[3-9]: 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 over neutrino energy was studied.
A dip in the distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation.
The observed 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.
[3-10]: Tau neutrinos favored over sterile neutrinos in atmospheric muon neutrino oscillations, Fukuda, S. et al. (Super-Kamiokande), Phys. Rev. Lett. 85 (2000) 3999-4003, arXiv:hep-ex/0009001.
[3-11]: Neutrino-induced upward stopping muons in Super-Kamiokande, Fukuda, Y. et al. (Super-Kamiokande), Phys. Lett. B467 (1999) 185-193, arXiv:hep-ex/9908049.
[3-12]: Observation of the east-west anisotropy of the atmospheric neutrino flux, Futagami, T. et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 5194-5197, arXiv:astro-ph/9901139.
[3-13]: Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2644-2648, arXiv:hep-ex/9812014.
[3-14]: Evidence for oscillation of atmospheric neutrinos, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1562-1567, arXiv:hep-ex/9807003.
[3-15]: Study of the atmospheric neutrino flux in the multi-GeV energy range, Fukuda, Y. et al. (Super-Kamiokande), Phys. Lett. B436 (1998) 33-41, arXiv:hep-ex/9805006.
[3-16]: Measurement of a small atmospheric $\nu_\mu$ / $\nu_e$ ratio, Fukuda, Y. et al. (Super-Kamiokande), Phys. Lett. B433 (1998) 9-18, arXiv:hep-ex/9803006.

4 - Atmospheric Neutrinos - Conference Proceedings

[4-1]: Results from Super-Kamiokande, Yasuo Takeuchi (Super-Kamiokande), arXiv:1112.3425, 2011. XXIV International Conference on Neutrino Physics and Astrophysics (Neutrino 2010).
[4-2]: 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.
[4-3]: SuperK recent results, Scholberg, K. (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.].
[4-4]: 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.
[4-5]: 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).
[4-6]: 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.
[4-7]: 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.
[4-8]: Atmospheric Neutrino Oscillations in Super-Kamiokande I, Ahabig, A. (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.
[4-9]: Recent results from atmospheric $\nu$ and K2K, Itow, Y., 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 $\nu_{\mu} -> \nu_e$ channel as compared with the CHOOZ limit and the Super-Kamiokande allowed region. [M.L.].
[4-10]: 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.
[4-11]: Atmospheric Neutrinos at Super-Kamiokande, Mauger, C. (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.
[4-12]: Experimental results on atmospheric neutrinos in Super-Kamiokande-I, Shiozawa, M. (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.
[4-13]: Super-Kamiokande atmospheric neutrino results, Toshito, Toshiyuki (Super-Kamiokande), arXiv:hep-ex/0105023, 2001.
[4-14]: Study of neutrino oscillations with the atmospheric neutrino data from Super-Kamiokande, Kajita, T. (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 100 (2001) 107-112.
[4-15]: Atmospheric neutrinos in Super-Kamiokande, Sobel, H. (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 91 (2001) 127-133.
[4-16]: Atmospheric neutrino results from Super-Kamiokande, Messier, M. D., Int. J. Mod. Phys. A16S1B (2001) 733-735.
[4-17]: Future atmospheric neutrino data from Super-Kamiokande, Kajita, T. (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 100 (2001) 139-141.
[4-18]: Atmospheric neutrinos at Super-Kamiokande, Scholberg, Kate (Super-Kamiokande), arXiv:hep-ex/9905016, 1999.
[4-19]: Evidence for neutrino oscillations in atmospheric neutrino observations, Shiozawa, M. (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.
[4-20]: Observation of east-west effect in atmospheric neutrinos by Super-Kamiokande, Kaneyuki, K. (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[4-21]: Multi-ring atmospheric neutrino events in Super- Kamiokande, Mauger, C. (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[4-22]: Upward coming muons in Super-Kamiokande and muon neutrino oscillations, Okada, A. (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[4-23]: Observation of atmospheric neutrinos in Super-Kamiokande and the neutrino oscillation parameters, Kaneyuki, K. (Super-Kamiokande), 1999. Prepared for 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[4-24]: Atmospheric neutrino results from Super-Kamiokande and Kamiokande: Evidence for $\nu_\mu$ oscillations, Kajita, Takaaki (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 77 (1999) 123-132, arXiv:hep-ex/9810001.
[4-25]: Atmospheric neutrino results from Super-Kamiokande, Kajita, T. (Super-Kamiokande), 1998. Given at International Workshop on JHF Science (JHF 98), Tsukuba, Japan, 4-7 Mar 1998.
[4-26]: Atmospheric neutrino flux studies with the Super-Kamiokande detector, Wai, L. (Super-Kamiokande), 1997. Prepared for Orbis Scientiae on Physics of Mass, Miami, Florida, 12-15 Dec 1997.

5 - Solar Neutrinos

[5-1]: Solar neutrino results in Super-Kamiokande-III, K. Abe et al. (Super-Kamiokande), Phys. Rev. D83 (2011) 052010, arXiv:1010.0118.
[5-2]: 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.
[5-3]: Solar neutrino measurements in Super-Kamiokande-I, Hosaka, J. et al. (Super-Kamkiokande), Phys. Rev. D73 (2006) 112001, arXiv:hep-ex/0508053.
[5-4]: 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.
[5-5]: 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.
[5-6]: 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.
[5-7]: 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.
[5-8]: Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data, Fukuda, S. et al. (Super-Kamiokande), Phys. Lett. B539 (2002) 179-187, arXiv:hep-ex/0205075.
[5-9]: Constraints on neutrino oscillations using 1258 days of Super-Kamiokande solar neutrino data, Fukuda, S. et al. (Super-Kamiokande), Phys. Rev. Lett. 86 (2001) 5656-5660, arXiv:hep-ex/0103033.
[5-10]: Solar B-8 and hep neutrino measurements from 1258 days of Super-Kamiokande data, Fukuda, S. et al. (Super-Kamiokande), Phys. Rev. Lett. 86 (2001) 5651-5655, arXiv:hep-ex/0103032.
[5-11]: Measurement of the solar neutrino energy spectrum using neutrino electron scattering, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2430-2434, arXiv:hep-ex/9812011.
[5-12]: Constraints on neutrino oscillation parameters from the measurement of day-night solar neutrino fluxes at Super-Kamiokande, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 1810-1814, arXiv:hep-ex/9812009.
[5-13]: Measurements of the solar neutrino flux from Super-Kamiokande's first 300 days, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1158-1162, arXiv:hep-ex/9805021.

6 - Solar Neutrinos - Conference Proceedings

[6-1]: Solar Neutrino Measurement at SK-III, B.S. Yang (Super-Kamiokande), arXiv:0909.5469, 2009. DPF-2009, Detroit, MI, July 2009.
[6-2]: 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.
[6-3]: 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.
[6-4]: 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.
[6-5]: 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.
[6-6]: Solar Neutrino Precision Measurements using all 1496 Days of Super-Kamiokande-I Data, Smy, M. B. (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.
[6-7]: Implications for solar neutrino oscillations from Super-Kamiokande and SNO data, Smy, M. B. (Super-Kamiokande), arXiv:hep-ex/0108053, 2001.
[6-8]: Solar neutrino results from super-Kamiokande, Smy, M. B. (Super-Kamiokande), arXiv:hep-ex/0106064, 2001.
[6-9]: Solar neutrino results (from radio-chemical and water Cherenkov detectors), Suzuki, Y., Nucl. Phys. Proc. Suppl. 100 (2001) 14-23.
[6-10]: Solar Neutrino Results from Super-Kamiokande, Suzuki, Y., Nucl. Phys. Proc. Suppl. 91 (2001) 29-35.
[6-11]: Recent Super-Kamiokande results on solar neutrinos, Koshio, Y. (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.
[6-12]: Solar neutrinos with Super-Kamiokande, Smy, M. B., arXiv:hep-ex/9903034, 1999.
[6-13]: Solar neutrinos at Super-Kamiokande, Inoue, K. (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 70 (1999) 273-283.
[6-14]: Solar neutrino results from Super-Kamiokande, Suzuki, Y. (Super-Kamiokande), Nucl. Phys. Proc. Suppl. 77 (1999) 35-42.
[6-15]: Solar neutrinos results and oscillation analysis from Super-Kamiokande, Koshio, Y. (Super-Kamiokande), 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[6-16]: Solar neutrino measurements from Super-Kamiokande, Vagins, M. R. (Super-Kamiokande), 1998. Prepared for 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, British Columbia, Canada, 23-29 Jul 1998.
[6-17]: Super-Kamiokande solar neutrino analysis: The first 201.6 days' results, Sanford, R. E. (Super-Kamiokande), 1997. Sixth Conference on the Intersections of Particle and Nuclear Physics (CIPANP 97), Big Sky, MT, 27 May - 2 June 1997.
[6-18]: Kamiokande-II results on solar neutrinos and the Super-Kamiokande experiment, Suzuki, Y., 1991. 11th Moriond Workshop on Tests of Fundamental Laws in Physics, Les Arcs, France, Jan 26 - Feb 2, 1991.

7 - Supernova Neutrinos

[7-1]: Search for Supernova Neutrino Bursts at Super-Kamiokande, Ikeda, M., Takeda, A., Fukuda, Y., Vagins, M. R., Sakuda, M. (Super-Kamiokande), Astrophys. J. 669 (2007) 519-524, arXiv:0706.2283.
[7-2]: Search for supernova relic neutrinos at Super-Kamiokande, Malek, M. et al. (Super-Kamiokande), Phys. Rev. Lett. 90 (2003) 061101, arXiv:hep-ex/0209028.

8 - Astrophysical Neutrinos

[8-1]: Search for Astrophysical Neutrino Point Sources at Super-Kamiokande, E. Thrane et al. (Super-Kamiokande), Astrophys. J. 704 (2009) 503-512, arXiv:0907.1594.
[8-2]: 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.
[8-3]: 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.
[8-4]: Search for diffuse astrophysical neutrino flux using ultra- high energy upward-going muons in Super-Kamiokande I, Swanson, M. E. C. (Super-Kamiokande), Astrophys. J. 652 (2006) 206-215, arXiv:astro-ph/0606126.
[8-5]: High-Energy Neutrino Astronomy with the Super-Kamiokande Detector, Habig, A. (Super-Kamiokande), arXiv:astro-ph/0507051, 2005. 29th ICRC, Pune, India.

9 - Physics

[9-1]: Search for Nucleon Decay into Charged Anti-lepton plus Meson in Super-Kamiokande I and II, H. Nishino et al., arXiv:1203.4030, 2012.
[9-2]: Search for GUT Monopoles at Super-Kamiokande, K. Ueno et al. (Super-Kamiokande), arXiv:1203.0940, 2012.
[9-3]: The search for n-nbar oscillation in Super-Kamiokande I, Super-Kamiokande collaboration et al. (Kamiokande), arXiv:1109.4227, 2011.
[9-4]: 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.
[9-5]: 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.
[9-6]: 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.
[9-7]: 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.
[9-8]: Search for proton decay through p -> anti-nu K+ in a large water Cherenkov detector, Hayato, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 83 (1999) 1529-1533, arXiv:hep-ex/9904020.
[9-9]: Search for proton decay via p -> e+ pi0 in a large water Cherenkov detector, Shiozawa, M. et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 3319-3323, arXiv:hep-ex/9806014.

10 - Cosmic Rays

[10-1]: 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.

11 - Cosmic Rays - Conference Proceedings

[11-1]: 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.

12 - Detector

[12-1]: 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.
[12-2]: The Super-Kamiokande detector, Fukuda, S. et al. (SuperKamiokade), Nucl. Instrum. Meth. A501 (2003) 418-462. http://www-sk.icrr.u-tokyo.ac.jp/doc/sk/pub/sknimpaper.pdf.
[12-3]: Measurement of radon concentrations at Super-Kamiokande, Takeuchi, Y. et al. (SuperKamiokade), Phys. Lett. B452 (1999) 418-424, arXiv:hep-ex/9903006.
[12-4]: Reconstruction algorithms in the Super-Kamiokande large water Cherenkov detector, Shiozawa, M. (Super-Kamiokande), Nucl. Instrum. Meth. A433 (1999) 240-246.
[12-5]: Calibration of Super-Kamiokande using an electron linac, Nakahata, M. et al. (Super-Kamiokande), Nucl. Instrum. Meth. A421 (1999) 113-129, arXiv:hep-ex/9807027.

13 - Detector - Conference Proceedings

[13-1]: Gadolinium study for a water Cherenkov detector, Atsuko Kibayashi (Super-Kamiokande), arXiv:0909.5528, 2009. DPF-2009, Detroit, MI, July 2009.

14 - Experimental Test

[14-1]: A Study on the e / mu identification capability of a water Cerenkov detector and the atmospheric neutrino problem, Kasuga, S. et al., Phys. Lett. B374 (1996) 238-242.

15 - Conference Proceedings

[15-1]: Low Energy Neutrino Astronomy in Super-Kamiokande, Michael Smy, arXiv:1110.0012, 2011. DPF 2011.
[15-2]: Recent Results from Super-Kamiokande, Sekiya, H. et al. (Super-Kamiokande), arXiv:0810.0595, 2008. ICHEP08, Philadelphia, USA, July 2008.
[15-3]: The Super-Kamiokande Experiment, C.W. Walter (Super-Kamiokande), arXiv:0802.1041, 2008. Neutrino Oscillations: Present Status and Future Plans.
[15-4]: 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.
[15-5]: Upward showering muons in Super-Kamiokande, A. Habig (Super-Kamiokande), 2004. HEAD 2004. http://neutrino.d.umn.edu/~habig/sk-showering.pdf.
[15-6]: Neutrino Physics: Experimental Status, Kajita, T., 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 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 C.L. allowed contour for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by Super-Kamiokande. [M.L.].
[15-7]: 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.
[15-8]: Atmospheric and long baseline neutrino, Nakaya, T. (Super-Kamiokande), eConf C020620 (2002) SAAT01, arXiv:hep-ex/0209036. 22nd Physics in Collision Conference (PIC 2002), Stanford, California, 20-22 June 2002.
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16 - Background

[16-1]: 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.

Useful Links

L/E analysis of the atmospheric neutrino data from Super-Kamiokande, Masaki Ishitsuka, PhD Thesis, University of Tokyo, Feb. 2004
Super-Kamiokande-I Solar Neutrino Data
U.S. Super-Kamiokande Collaboration Home Page
Evidence for Neutrino Mass from Observations of Atmospheric Neutrinos with Super-Kamiokande Ph.D. Thesis by Mark D. Messier
Atmospheric neutrino oscillation analysis using FLUKA 3D flux and Super-Kamiokande data, Atsuko Kibayashi, PhD Thesis, University of Hawaii, August 2002
Limits on $\nu_\mu \leftrightarrows \nu_{\mathrm{sterile}}$ Oscillations by the $\pi^0/\mu$ Measurement in the Water Cherenkov Detectors Shoei Nakayama, PhD Thesis, University of Tokyo, Mar. 2003

Neutrino Unbound

We Can Put an End to Word Attachments

Authors:
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it

Last Update: Tue 15 May 2012, day 136 of the year 2012, 09:42:20 UTC