Atmospheric Neutrinos

Useful Links

References

MINOS

Measurement of Neutrino Oscillations with the MINOS Detectors in the NuMI Beam

(13 June 2008)

MINOS

A Study of Muon Neutrino Disappearance Using the Fermilab Main Injector Neutrino Beam

(5 November 2007)

K2K

An improved search for oscillation in a long-baseline accelerator experiment

(2 March 2006)

First Observations of Separated Atmospheric and Events in the MINOS Detector

(15 December 2005)

107 observed events

expected events without oscillations

probability of a statistical fluctuation (no oscillations)

probability of a statistical fluctuation (no oscillations) of rate

probability of a statistical fluctuation (no oscillations) of spectrum

best-fit:

108 observed events

expected events without oscillations

probability of a statistical fluctuation about

the observed spectrum reveals the type of distortion expected from oscillations

T. Kajita, WIN2003

(October 2003)

Best fit value of mixing parameters: , [Y. Hayato, EPS2003].
(July 2003)

The combined analysis of Super-Kamiokande atmospheric neutrino data in terms of two-neutrino mixing indicate that the oscillation channel is favored [M. Shiozawa, Neutrino 2002].
(June 2002)

Useful Links

Atmospheric Neutrino Experiments.

Review of Particle Physics: Cosmic Rays

The FLUKA 3-D Atmospheric Neutrino Flux, tables of calculated fluxes (see hep-ph/9907408)

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

APS Neutrino Study: Solar and Atmospheric Neutrino Experiments Working Group

Nuance Neutrino Generator

L/E analysis of the atmospheric neutrino data from Super-Kamiokande, Masaki Ishitsuka, PhD Thesis, University of Tokyo, Feb. 2004

Atmosphere

Physics of Atmospheres and Oceans

References

[1-1]

Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. http://www.oup.com/uk/catalogue/?ci=9780198508717.

[1-2]

Physics and Astrophysics Of Neutrinos, Fukugita, M., (ed.), Suzuki, A., (ed.), Springer, 1994.

[1-3]

Cosmic Rays and Particle Physics, Gaisser, T. K., Cambridge University Press, 1990.

[2-1]

Discovery of neutrino oscillations, Kajita, T., Rept. Prog. Phys. 69 (2006) 1607-1635.

[2-2]

Atmospheric neutrinos, Kajita, T., New J. Phys. 6 (2004) 194. http://www.iop.org/EJ/abstract/1367-2630/6/1/194.

[2-3]

Astrophysical Neutrino Telescopes, A. B. McDonald et al., Rev. Sci. Instrum. 75 (2004) 293, arXiv:astro-ph/0311343.
Comment: The figure n. 19 shows the 90 % C.L. allowed contours for oscillations obtained by different atmospheric neutrino experiments. [M.L.].

[2-4]

Oscillations of atmospheric neutrinos, Jung, C. K., McGrew, C., Kajita, T., Mann, T., Ann. Rev. Nucl. Part. Sci. 51 (2001) 451-488.
From the article: The observation made by the Super-Kamiokande experiment of muon flavor disappearance in the atmospheric neutrino flux provides compelling evidence for neutrino flavor oscillations and, by implication, for nonzero neutrino rest mass. In the Standard Model neutrinos are assumed to be massless. However, the quantum-mechanical phenomenon of neutrino oscillations requires neutrinos to have a nonzero rest mass. Consequently, the Super-Kamiokande observations alter our view of these fundamental leptons and have profound implications for elementary particle physics, cosmology and astrophysics. Ultimately, the Standard Model must be modified to accomodate this result.

[2-5]

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

[2-6]

The atmospheric neutrino anomaly: Muon neutrino disappearance, Learned, J. G. (SuperKamioKande), arXiv:hep-ex/0007056, 2000.

[2-7]

Neutrino astronomy, Totsuka, Yoji, Rept. Prog. Phys. 55 (1992) 377-430.

[2-8]

Observational neutrino astrophysics, Koshiba, M., Phys. Rep. 220 (1992) 229-381.

[3-1]

Atmospheric neutrino and Long Baseline neutrino experiments, Giorgio Giacomelli, AIP Conf. Proc. 972 (2008) 412-420, arXiv:0712.2126. Carpatian Summer School of Physics 2007, Sinaia, Romania, August 2007.

[3-2]

Atmospheric neutrino oscillations, Giacomelli, G., Giorgini, M. (the MACRO), arXiv:hep-ex/0504002, 2005. 7th School on Non-Accelerator Astroparticle Physics, Trieste, Italy, 2004.

[3-3]

Evidence for Neutrino Mass: A Decade of Discovery, K.M. Heeger, arXiv:hep-ex/0412032, 2004. SEESAW25: International Conference on the Seesaw Mechanism and Neutrino Mass, Paris, France, 10-11 June 2004.

[3-4]

Recent Results of non-accelarator-based neutrino experiments, Yifang Wang, Int. J. Mod. Phys. A20 (2005) 5244, arXiv:hep-ex/0411028. "32nd International Conference on High Energy Physics", Aug. 16-22, 2004, Beijing, P.R. China.

[3-5]

Neutrinos underground, Sobel,H., 2004. AAAS meeting 2004, 17-21 Feb. 2004, Washington, DC, US. http://harv11.fnal.gov/~smaria/aaas04/hank_aaas04.pdf.

[3-6]

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 oscillations obtained by different atmospheric neutrino experiments. The figure in slide n.24 shows the C.L. allowed contour for oscillations obtained by Super-Kamiokande. [M.L.].

[3-7]

Results and status of current accelerator neutrino experiments, Nishikawa, K., 2003. XXI International Symposium on Lepton Photon 2003, 11-16 August 2003, Fermi National Accelerator Laboratory, Batavia, Illinois, USA. http://conferences.fnal.gov/lp2003/program/S10/nishikawa_s10.pdf.
Comment: The slide n.40 shows the expected sensitivity on of different projects. [M.L.].

[3-8]

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.).

[3-9]

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.

[3-10]

Atmospheric Neutrinos and K2K, Nishikawa, K., 2002. Topical Seminar on Frontier of Particle Physics 2002: Neutrinos and Cosmology, 20-25 August 2002, Beijing, China. http://bes.ihep.ac.cn/particle/2002/presentation/K.Nishikawa/TALK_2.ZIP.

[3-11]

Status and prospects of neutrino oscillations: Atmospheric, Kajita, T., 2002. Fourth NuFact '02 Workshop on Neutrino Factories based on Muon Storage Rings, Imperial College, London, 1-6 July 2002. http://www.hep.ph.ic.ac.uk/NuFact02/Scientific-programme/files/Monday/plenary/A03_kajita.ppt.

[3-12]

Experimental measurements of atmospheric neutrinos, Kearns, Edward, Nucl. Phys. Proc. Suppl. 70 (1999) 315-323, arXiv:hep-ex/9803007.

[4-1]

Phenomenology with Massive Neutrinos, Gonzalez-Garcia, M. C., Maltoni, Michele, Phys. Rept. 460 (2008) 1-129, arXiv:0704.1800.

[4-2]

Global analysis of three-flavor neutrino masses and mixings, Fogli, G. L., Lisi, E., Marrone, A., Palazzo, A., Prog. Part. Nucl. Phys. 57 (2006) 742-795, arXiv:hep-ph/0506083.

[4-3]

Atmospheric neutrinos and neutrino oscillations, Takaaki Kajita, Paolo Lipari, Comptes Rendus Physique 6 (2005) 739-748.

[4-4]

Report of the Solar and Atmospheric Neutrino Experiments Working Group of the APS Multidivisional Neutrino Study, H. Back et al., arXiv:hep-ex/0412016, 2004.

[4-5]

Neutrino Masses and Oscillations: Triumphs and Challenges, R.D. McKeown, P. Vogel, Phys. Rep. 394 (2004) 315, arXiv:hep-ph/0402025.

[4-6]

Cosmic rays, Gaisser, T. K., Stanev, T., Phys. Lett. B592 (2004) 228-234. The Review of Particle Properties 2004. http://pdg.lbl.gov/2004/reviews/cosmicrayrpp.pdf.

[4-7]

Neutrino Mixing, Carlo Giunti, Marco Laveder, arXiv:hep-ph/0310238, 2003. In "Developments in Quantum Physics - 2004", p. 197-254, edited by F. Columbus and V. Krasnoholovets, Nova Science, Hauppauge, NY. http://novapublishers.com/catalog/product_info.php?products_id=1633.

[4-8]

Flux of Atmospheric Neutrinos, Gaisser, T. K., Honda, M., Ann. Rev. Nucl. Part. Sci. 52 (2002) 153, arXiv:hep-ph/0203272.
From the article: An offset in normalization of the neutrino flux does not affect the conclusions about oscillations, which are robust. Nevertheless, it is interesting and informative to compare the measured neutrino flux as directly as possible in an absolute fashion with the calculations. Fig. 25 at page 58 compares the neutrino fluxes measured at Super-K with the two calculations [,15-40] that have been used extensively as input to the detector simulation. The comparisons are made as a function of visible energy by the Super-K group. The magnitudes are consistent with what is expected for oscillations in this energy range that involve and but not ; namely, there is a deficit of , whereas the measured flux of electron neutrinos is consistent with the calculation.

[4-9]

Neutrino Masses and Mixing: Evidence and Implications, M.C. Gonzalez-Garcia, Y. Nir, Rev. Mod. Phys. 75 (2003) 345-402, arXiv:hep-ph/0202058.

[4-10]

Finally neutrino has mass?, Bilenky, S. M., Giunti, C., Kim, C. W., Int. J. Mod. Phys. A15 (2000) 625-650, arXiv:hep-ph/9902462.

[4-11]

Phenomenology of neutrino oscillations, S. M. Bilenky, C. Giunti, W. Grimus, Prog. Part. Nucl. Phys. 43 (1999) 1, arXiv:hep-ph/9812360.

[4-12]

Cosmic ray showers, Greisen, K., Ann. Rev. Nucl. Part. Sci. 10 (1960) 63-108.

[5-1]

Muons and Neutrinos 2007, Thomas K. Gaisser, arXiv:0801.4542, 2008. 30th International Cosmic Ray Conference, Merida, Yucatan, July, 2007.

[5-2]

Atmospheric Neutrinos, Thomas K. Gaisser, AIP Conf. Proc. 944 (2007) 140-142, arXiv:astro-ph/0612274. Neutrino 2006.

[5-3]

Global fits to neutrino oscillation data, Thomas Schwetz, Phys. Scripta T127 (2006) 1-5, arXiv:hep-ph/0606060. SNOW2006 workshop, Stockholm, 2-6 May 2006.

[5-4]

Neutrino oscillations: Current status and prospects, Thomas Schwetz, Acta Phys. Polon. B36 (2005) 3203, arXiv:hep-ph/0510331. XXIX International Conference of Theoretical Physics, "Matter To The Deepest: Recent Developments In Physics of Fundamental Interactions", 8-14 September 2005, Ustron, Poland.

[5-5]

Neutrino mass and mixing parameters: A short review, G.L. Fogli et al., arXiv:hep-ph/0506307, 2005. 40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005.

[5-6]

Atmospheric neutrino challenges, Todor Stanev, Nucl. Phys. Proc. Suppl. 145 (2005) 69, arXiv:astro-ph/0412395. NOW 2004.

[5-7]

Three-flavour effects and CP- and T-violation in neutrino oscillations, Evgeny Akhmedov, Phys. Scripta T121 (2005) 65, arXiv:hep-ph/0412029. Nobel Symposium 129 - Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.

[5-8]

Physics of Massive Neutrinos, J. W. F. Valle, Nucl. Phys. Proc. Suppl. 149 (2005) 3, arXiv:hep-ph/0410103. Sixth International Conf. on Neutrino Factories and SuperBeams (NuFact04) Osaka, Japan, July 26-August 1, 2004.

[5-9]

Neutrino 2004: Concluding Talk, Guido Altarelli, Nucl. Phys. Proc. Suppl. 143 (2005) 470, arXiv:hep-ph/0410101. Neutrino 2004, Paris, 14-19 June 2004.

[5-10]

Global Analysis of Neutrino Data, M. C. Gonzalez-Garcia, Phys. Scripta T121 (2005) 72, arXiv:hep-ph/0410030. Nobel Symposium on Neutrino Physics, Haga Slott, Enkoping, Sweden.

[5-11]

Global analysis of neutrino oscillation, S. Goswami, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/goswami.pdf.

[5-12]

Neutrino physics, recent results, Lisi, E., 2004. IFAE-2004, 14-16 April 2004, Torino, Italy. http://agenda.cern.ch/askArchive.php?base=agenda&categ=a041654&id=a041654s3t6/transparencies, http://www.ph.unito.it/ifae/Proceedings/Sessioni/Neutrinos.pdf.

[5-13]

Neutrino masses twenty-five years later, Valle, J W F, Aip Conf. Proc. 687 (2003) 16, arXiv:hep-ph/0307192. MRST'03 (Joe-Fest), Syracuse, NY, May 2003.

[5-14]

Neutrino oscillations in the framework of the tree-neutrino mixing, Bilenky, S. M., arXiv:hep-ph/0307186, 2003. Ist Yamada Symposium Om neutrinos and Dark Matter in Nuclear Physics, June 9-14, 2003, Nara, Japan.

[5-15]

Neutrino Physics after KamLAND, Smirnov, Alexei Yu., arXiv:hep-ph/0306075, 2003. 4th Workshop on "Neutrino Oscillations and their Origin" (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Smirnov.pdf.

[5-16]

Status of Neutrino Fits, C. Giunti, arXiv:hep-ph/0305139, 2003. XXXVIIIth Rencontres de Moriond, ElectroWeak Interactions and Unified Theories, 15-22 March 2003, Les Arcs, France. http://moriond.in2p3.fr/EW/2003/Transparencies/1_Sunday/1_2_afternoon/1_2_6_Giunti/C.Giunti.pdf.

[5-17]

Neutrino Masses and Mixing: Where We Stand and Where We are Going, M. C. Gonzalez-Garcia, arXiv:hep-ph/0211054, 2002. 10th International Conference on Supersymmetry and Unification of Fundamental Interactions, SUSY02 (June 17-23, 2002, DESY, Hamburg).

[5-18]

Theory of Neutrino Masses and Mixing, M.C. Gonzalez-Garcia, Nucl. Phys. Proc. Suppl. 117 (2003) 186, arXiv:hep-ph/0210359. 31st international conference on high energy physics (ICHEP 2002), Amsterdam, 24-31 July 2002.

[5-19]

Current Status of Neutrino Masses and Mixings, Giunti, C., arXiv:hep-ph/0209103, 2002. 31st International Conference on High Energy Physics "ICHEP02", 24-31 July 2002, Amsterdam. http://www.ichep02.nl/Transparencies/NEU/NEU-2/NEU-2-1.giunti.ps.

[6-1]

First Evidence For Atmospheric Neutrino-Induced Cascades with the IceCube Detector, Michelangelo D'Agostino, arXiv:0910.2555, 2009.

[7-1]

Atmospheric neutrino oscillation analysis with sub-leading effects in Super-Kamiokande I, II, and III, R. Wendell et al. (Super-Kamiokande), arXiv:1002.3471, 2010.

[7-2]

Measurement of the Cosmic Ray and Neutrino-Induced Muon Flux at the Sudbury Neutrino Observatory, Collaboration, SNO (SNO), Phys. Rev. D80 (2009) 012001, arXiv:0902.2776.

[7-3]

Determination of the Atmospheric Neutrino Flux and Searches for New Physics with AMANDA-II, Collaboration, The IceCube (IceCube), Phys. Rev. D79 (2009) 102005, arXiv:0902.0675.

[7-4]

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.

[7-5]

Search for Matter-Dependent Atmospheric Neutrino Oscillations in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D77 (2008) 052001, arXiv:0801.0776.

[7-6]

Experimental study of the atmospheric neutrino backgrounds for proton decay to positron and neutral pion searches in water Cherenkov detectors, S. Mine et al. (K2K), Phys. Rev. D77 (2008) 032003, arXiv:0801.0182.

[7-7]

Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector, A. Achterberg et al. (IceCube), Phys. Rev. D76 (2007) 027101, arXiv:0705.1781.

[7-8]

Charge-Separated Atmospheric Neutrino-Induced Muons in the MINOS Far Detector, P. Adamson et al. (MINOS), Phys. Rev. D75 (2007) 092003, arXiv:hep-ex/0701045.

[7-9]

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 , disfavor the hypothesis of no tau neutrino appearance by 2.4 sigma.

[7-10]

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.

[7-11]

First Observations of Separated Atmospheric Muon Neutrino and Muon Anti-Neutrino Events in the MINOS Detector, P. Adamson et al. (MINOS), Phys. Rev. D73 (2006) 072002, arXiv:hep-ex/0512036.
From the abstract: The ratio of upward to downward-going events in the data is compared to the Monte Carlo expectation in the absence of neutrino oscillations giving: ... The ratio of to events in the data is compared to the Monte Carlo expectation assuming neutrinos and anti-neutrinos oscillate in same manner giving: ... Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for and .

[7-12]

Neutrino Oscillation Effects in Soudan-2 Upward-stopping muons, Allison, W. W. M. et al. (Soudan-2), Phys. Rev. D72 (2005) 052005, arXiv:hep-ex/0507068.

[7-13]

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.

[7-14]

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 neutrino oscillation parameters; and at 90% confidence level.

[7-15]

Observation of Atmospheric Neutrino Oscillations in Soudan 2, M. Sanchez et al. (Soudan 2), Phys. Rev. D68 (2003) 113004, arXiv:hep-ex/0307069.

[7-16]

Atmospheric neutrino oscillations from upward throughgoing muon multiple scattering in MACRO, M. Ambrosio et al. (MACRO), Phys. Lett. B566 (2003) 35, arXiv:hep-ex/0304037.

[7-17]

Matter effects in upward-going muons and sterile neutrino oscillations, Ambrosio, M. et al. (MACRO), Phys. Lett. B517 (2001) 59-66, arXiv:hep-ex/0106049.

[7-18]

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.

[7-19]

Low energy atmospheric muon neutrinos in MACRO, Ambrosio, M. et al. (MACRO), Phys. Lett. B478 (2000) 5-13.

[7-20]

The atmospheric neutrino flavor ratio from a 3.9 fiducial kiloton-year exposure of Soudan 2, Allison, W. W. M. et al. (Soudan-2), Phys. Lett. B449 (1999) 137-144, arXiv:hep-ex/9901024.

[7-21]

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.

[7-22]

Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO, Ambrosio, M. et al. (MACRO), Phys. Lett. B434 (1998) 451-457, arXiv:hep-ex/9807005.

[7-23]

Evidence for oscillation of atmospheric neutrinos, Fukuda, Y. et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1562-1567, arXiv:hep-ex/9807003.

[7-24]

Measurement of the flux and zenith angle distribution of upward through-going muons in Kamiokande II + III, Hatakeyama, S. et al. (Kamiokande), Phys. Rev. Lett. 81 (1998) 2016-2019, arXiv:hep-ex/9806038.

[7-25]

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.

[7-26]

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.

[7-27]

The Baksan underground scintillation telescope, Alekseev, E. N. et al., Phys. Part. Nucl. 29 (1998) 254-256.

[7-28]

Atmospheric muon-neutrino fraction above 1-GeV, Clark, R. et al. (IMB), Phys. Rev. Lett. 79 (1997) 345-348.

[7-29]

Study of neutron background in the atmospheric neutrino sample in Kamiokande, Fukuda, Y. et al. (Kamiokande), Phys. Lett. B388 (1996) 397-401.

[7-30]

Determination of the atmospheric neutrino spectra with the Frejus detector, Daum, K. (Frejus.), Z. Phys. C66 (1995) 417-428.

[7-31]

Atmospheric muon-neutrino / electron-neutrino ratio in the multiGeV energy range, Fukuda, Y. et al. (Kamiokande), Phys. Lett. B335 (1994) 237-245.

[7-32]

IMB-3: A Large water Cerenkov detector for nucleon decay and neutrino interactions, Becker-Szendy, R. et al. (IMB), Nucl. Instrum. Meth. A324 (1993) 363-382.

[22-202]

Survey of atmospheric neutrino data and implications for neutrino mass and mixing, Beier, E. W. et al., Phys. Lett. B283 (1992) 446-453.

[7-34]

Observation of a small atmospheric ratio in Kamiokande, Hirata, K. S. et al. (Kamiokande), Phys. Lett. B280 (1992) 146-152.

[7-35]

A Search for muon-neutrino oscillations with the IMB detector, Becker-Szendy, R. et al. (IMB), Phys. Rev. Lett. 69 (1992) 1010-1013.

[7-36]

The electron-neutrino and muon-neutrino content of the atmospheric flux, Becker-Szendy, R. et al. (IMB), Phys. Rev. D46 (1992) 3720-3724.

[7-37]

Measurement of atmospheric neutrino composition with IMB-3, Casper, D. et al. (IMB), Phys. Rev. Lett. 66 (1991) 2561-2564.

[7-38]

Flux and angular distribution of muons created by cosmic ray neutrinos, Boliev, M. M. et al., Bull. Russ. Acad. Sci. Phys. 55 (1991) NO.4126.

[7-39]

Experimental study of upward stopping muons in NUSEX, Aglietta, M. et al., Europhys. Lett. 15 (1991) 559-564.

[7-40]

A Study of atmospheric neutrino oscillations in the Frejus experiment, Berger, Christoph et al. (Frejus), Phys. Lett. B245 (1990) 305-310.

[7-41]

Experimental study of upward going muons in Kamiokande, Oyama, Y. et al. (Kamiokande), Phys. Rev. D39 (1989) 1481.

[7-42]

Study of atmospheric neutrino interactions with the Frejus detector, Berger, Christoph et al. (Frejus), Phys. Lett. B227 (1989) 489.

[7-43]

Experimental study of atmospheric neutrino flux in the NUSEX experiment, Aglietta, M. et al. (The NUSEX), Europhys. Lett. 8 (1989) 611-614.

[7-44]

Experimental study of the atmospheric neutrino flux, Hirata, K. S. et al. (Kamiokande), Phys. Lett. B205 (1988) 416.

[7-45]

Contained neutrino interactions in an underground water detector, Bionta, R. M. et al. (IMB), Phys. Rev. D38 (1988) 768-775.

[7-46]

Atmospheric neutrino background and pion nuclear effect for Kamioka nucleon decay experiment, Nakahata, Masayuki et al. (Kamiokande), J. Phys. Soc. Jap. 55 (1986) 3786.

[7-47]

Calculation of atmospheric neutrino induced backgrounds in a nucleon decay search, Haines, T. J. et al. (IMB), Phys. Rev. Lett. 57 (1986) 1986-1989.

[7-48]

Status of the Frejus experiment and preliminary results on contained events, Bareyre, P. et al. (AACHEN-ORSAY-PALAISEAU-SACLAY-WUPPERTAL), Nuovo Cim. C9 (1986) 159-166.

[7-49]

Test of neutrino oscillations using atmospheric neutrinos, LoSecco, J. M. et al. (IMB), Phys. Rev. Lett. 54 (1985) 2299.

[7-50]

Nucleon stability, magnetic monopoles and atmospheric neutrinos in the Mont Blanc experiment, Battistoni, G. et al., Phys. Lett. B133 (1983) 454.

[7-51]

Fully contained events in the Mont Blanc nucleon decay detector, Battistoni, G. et al., Phys. Lett. B118 (1982) 461.

[7-52]

Neutrino backgrounds in the Kolar Gold Field nucleon decay experiment, Krishnaswamy, M. r. et al., Pramana 19 (1982) 525-554.

[7-53]

Limitations on parameters of neutrino oscillations according to data of the baksan underground telescope, Boliev, M. M. et al., Yad. Fiz. 34 (1981) 1418-1421. In Russian.

[7-54]

Cosmic ray muon fluxes deep underground: intensity versus depth, and the neutrino induced component, Crouch, M. F. et al., Phys. Rev. D18 (1978) 2239-2252.

[7-55]

Evidence for the production of a new particle in neutrino interactions, Krishnaswamy, M. R. et al., Phys. Lett. B57 (1975) 105.

[7-56]

Neutrino-induced muons deep underground, Bergeson, H. E., Cassiday, G. L., Hendricks, M. B., Phys. Rev. Lett. 31 (1973) 66-70.

[7-57]

Krishnaswamy, M. R. et al., Proc. R. Soc. London A323 (1971) 489.

[22-210]

Muons produced by atmospheric neutrinos: Analysis, Chen, H. H., Kropp, W. R., Sobel, H. W., Reines, F., Phys. Rev. D4 (1971) 99-121.

[7-59]

Muons produced by atmospheric neutrinos: Experiment, Reines, F. et al., Phys. Rev. D4 (1971) 80-98.

[7-60]

Observation of a non-elastic cosmic ray neutrino interaction, C. V. Achar et al., Phys. Lett. 19 (1965) 78-80.

[7-61]

Detection of muons produced by cosmic ray neutrinos deep underground, C. V. Achar et al., Phys. Lett. 18 (1965) 196-199.

[7-62]

Evidence for high-energy cosmic ray neutrino interactions, F. Reines et al., Phys. Rev. Lett. 15 (1965) 429-433.

[8-1]

IceCube3-a new window on the Universe, Thomas K. Gaisser, Denis Robertson (IceCube), AIP Conf. Proc. 1123 (2009) 177-189, arXiv:0901.4294. 3rd Latin American School on Cosmic Rays, Arequipa, Peru, September, 2008.

[8-2]

Neutrino Oscillation Measurements with IceCube, Carsten Rott (IceCube), arXiv:0810.3698, 2008. ICHEP08.

[8-3]

Recent Results from Super-Kamiokande, Sekiya, H. et al. (Super-Kamiokande), arXiv:0810.0595, 2008. ICHEP08, Philadelphia, USA, July 2008.

[8-4]

The Super-Kamiokande Experiment, C.W. Walter, arXiv:0802.1041, 2008. Neutrino Oscillations: Present Status and Future Plans.

[8-5]

The MACRO Experiment at Gran Sasso, G. Giacomelli, A. Margiotta, arXiv:0707.1691, 2007. Charles Peck - Fest, Caltech, 2005.

[8-6]

First Results from AMANDA using the TWR System, Andrea Silvestri et al. (IceCube), arXiv:astro-ph/0701319, 2007. International School of Cosmic Ray Astrophysics, 15th Course: 'Astrophysics at Ultra-high Energies', Erice, Italy, 20-27 June 2006.

[8-7]

Neutrino-induced muons observed with MINOS, Habig, Alec T. (MINOS), arXiv:hep-ex/0507010, 2005. 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, 3-11 Aug 2005.

[8-8]

MACRO results on atmospheric neutrinos, G. Giacomelli, A. Margiotta (MACRO), Nucl. Phys. Proc. Suppl. 145 (2005) 116, arXiv:hep-ex/0504029. NOW 2004 Workshop, Conca Specchiulla, Otranto, Italy, September 2004.

[8-9]

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.

[8-10]

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.].

[8-11]

New MACRO results on atmospheric neutrino oscillations, G. Giacomelli, A. Margiotta (MACRO), Phys. Atom. Nucl. 67 (2004) 1139, arXiv:hep-ex/0407023. NANP03 Int. Conf., Dubna, 2003.

[8-13]

Super Kamiokande results: atmospheric and solar neutrinos, M.Ishitsuka, Super-Kamiokande Collaboration (Super-Kamiokande), arXiv:hep-ex/0406076, 2004. XXXIXth Rencontres de Moriond on Electroweak Interactions (2004).

[8-13]

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.

[8-14]

MACRO results on atmospheric neutrino oscillations, G. Giacomelli, A. Margiotta (MACRO), Eur. Phys. J. C33 (2004) S826, arXiv:hep-ex/0406037. HEP EPS Conf., Aachen, Germany, July 2003.

[8-15]

Other (past, present and future) atmospheric neutrino experiments, H. Gallagher, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/gallagher.ppt.

[8-16]

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.

[8-17]

Searching for atmospheric neutrino oscillations at MINOS, Blake, A. (MINOS), 2004. UK Institute of Physics: Particle Physics 2004, 5-7 April 2004, Birmingham, UK. http://agenda.cern.ch/askArchive.php?base=agenda&categ=a04837&id=a04837s9t2%2Ftransparencies%2Fblake.pdf.

[8-18]

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).

[8-19]

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.

[8-20]

Results from the BAIKAL neutrino telescope, R. Wischnewski (The BAIKAL), arXiv:astro-ph/0305302, 2003. 28th International Cosmic Ray Conference, Tsukuda, Japan, July 31 - August 7, 2003.

[8-21]

Atmospheric Neutrino Oscillations in Super-Kamiokande I, Ahabig, A. (Super-Kamiokande), 2003. Talk given at the 28th International Cosmic Ray Conferences (ICRC 2003) 31 Jul - 7 Aug 2003, Tsukuba, Japan. http://neutrino.d.umn.edu/~habig/atmpd.pdf.

[8-22]

Recent results from atmospheric 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 channel as compared with the CHOOZ limit and the Super-Kamiokande allowed region. [M.L.].

[8-23]

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.

[8-24]

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.

[8-25]

Other Atmospheric Neutrino Experiments, Goodman, Maury, Nucl. Phys. Proc. Suppl. 118 (2003) 99, arXiv:hep-ex/0210055. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/goodman.

[8-26]

Atmospheric neutrino oscillations with the MACRO detector, M. Giorgini (MACRO), arXiv:hep-ex/0210008, 2002. Beyond the Desert 02, Conference on Physics beyond the Standard Model, Oulu, Finland, 2-7 June 2002.

[8-27]

Neutrino Physics and Astrophysics with the MACRO Experiment at the Gran Sasso Lab, G. Giacomelli (MACRO), Braz. J. Phys. 33 (2003) 211, arXiv:hep-ex/0210006. 25th Meeting of the Nuclear Division of the Brasilian Physical Society, S. Pedro, Brasil, 1-4 September 2002.

[8-28]

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.

[8-29]

Atmospheric neutrino oscillations, G. Giacomelli, M. Giorgini, M. Spurio, arXiv:hep-ex/0201032, 2002.

[8-30]

Results from Soudan-2 on Atmospheric Neutrinos and Limits on Matter Instability, Mann, T. (Soudan-2), 2002. Conference on Neutrinos and Implications for Physics Beyond the Standard Model, Stony Brook, Oct. 11-13, 2002. http://insti.physics.sunysb.edu/itp/conf/neutrino/talks/mann.pdf.

[8-31]

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.

[8-32]

Experimental results on atmospheric neutrinos in Super-Kamiokande-I, Shiozawa, M. (Super-Kamiokande), 2002. XX^th International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/shiozawa.

[8-33]

Atmospheric Neutrinos: Status and Prospects with approved Experiments, Shiozawa, M. (Super-Kamiokande), 2002. Workshop on Large Detectors for proton decay, supernovae, and atmospheric neutrinos, and low energy neutrinos from high intensity beams, NNN02, CERN, 16-18 January 2002. http://muonstoragerings.cern.ch/NuWorkshop02/presentations/shiozawa1.ppt.

[8-34]

Atmospheric Neutrinos, Totsuka, Y., 2001. TAUP2001 - Topics in Astroparticle and Underground Physics, LNGS, Italy (September 8-12, 2001). http://taup2001.lngs.infn.it/f1/f1.pdf.
From the article: Is there a problem in the atmospheric neutrino data of Super-Kamiokande-I when compared with the 3D calculations of G.Battistoni and others [15-28]?.

[8-35]

Experiments with Solar and Atmospheric Neutrinos: Evidence for Neutrino Masses and Lepton Mixing. Experimental status and Future Projects, Schoenert, S., 2001. Astroparticle Physics Workshop, DESY - Zeuten, 19-21 June 2001. http://www.desy.de/desy-hs/zeuthen2001/presentations/main/schoenert.pdf.

[8-36]

Atmospheric neutrino results from Super-Kamiokande, Messier, M. D., Int. J. Mod. Phys. A16S1B (2001) 733-735.

[8-37]

Atmospheric neutrinos at Super-Kamiokande, Scholberg, Kate (Super-Kamiokande), arXiv:hep-ex/9905016, 1999.

[9-1]

Measurement of Neutrino Oscillations with the MINOS Detectors in the NuMI Beam, P. Adamson et al. (MINOS), Phys. Rev. Lett. 101 (2008) 131802, arXiv:0806.2237.

[9-2]

A Study of Muon Neutrino Disappearance Using the Fermilab Main Injector Neutrino Beam, Adamson, P. et al. (MINOS), Phys. Rev. D77 (2008) 072002, arXiv:0711.0769.
From the abstract: We report the results of a search for disappearance by the Main Injector Neutrino Oscillation Search []. The experiment uses two detectors separated by 734 km to observe a beam of neutrinos created by the Neutrinos at the Main Injector facility at Fermi National Accelerator Laboratory.... Based on measurements in the Near Detector, in the absence of neutrino oscillations we expected charged-current interactions at the Far Detector but observed 215. This deficit of events corresponds to a significanc e of 5.2 standard deviations. The deficit is energy dependent and is consistent with two-flavor neutrino oscillations according to and at 68% confidence level.

[9-3]

Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam, D.G. Michael et al. (MINOS), Phys. Rev. Lett. 97 (2006) 191801, arXiv:hep-ex/0607088.
From the abstract: The data are consistent with muon neutrino disappearance via oscillation with and (68% C.L.).

[9-4]

Measurement of neutrino oscillation by the K2K experiment, Ahn, M. H. et al. (K2K), Phys. Rev. D74 (2006) 072003, arXiv:hep-ex/0606032.

[9-5]

An improved search for oscillation in a long-baseline accelerator experiment, S. Yamamoto et al. (K2K), Phys. Rev. Lett. 96 (2006) 181801, arXiv:hep-ex/0603004.
From the abstract: At , the best fit value of the K2K disappearance analysis, we set an upper limit of at 90% confidence level.

[9-6]

Evidence for muon neutrino oscillation in an accelerator-based experiment, E. Aliu et al. (K2K), Phys. Rev. Lett. 94 (2005) 081802, arXiv:hep-ex/0411038.

[9-7]

Search for electron neutrino appearance in a 250-km long- baseline experiment, Ahn, M. H. et al. (K2K), Phys. Rev. Lett. 93 (2004) 051801, arXiv:hep-ex/0402017.

[9-8]

Indications of Neutrino Oscillation in a 250 km Long- baseline Experiment, Ahn, M. H. et al. (K2K), Phys. Rev. Lett. 90 (2003) 041801, arXiv:hep-ex/0212007.
From the abstract: The K2K experiment observes indications of neutrino oscillation: a reduction of flux together with a distortion of the energy spectrum. Fifty-six beam neutrino events are observed in Super-Kamiokande (SK), 250 km from the neutrino production point, with an expectation of .
From the article: Best Fit: , .... The measured oscillation parameters are consistent with the ones suggested by atmospheric neutrinos. At the time of this letter the K2K experiment has collected approximately one-half of its planned protons on target.

[9-9]

Detection of accelerator produced neutrinos at a distance of 250-km, Ahn, S. H. et al. (K2K), Phys. Lett. B511 (2001) 178-184, arXiv:hep-ex/0103001.

[10-1]

Current NuMI/MINOS Oscillation Results, A. Habig (MINOS), arXiv:0805.2317, 2008. Moriond Electroweak conference, March 1-8 2008.

[10-2]

K2K results, T. Nakaya (K2K), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/nakaya.pdf.
Comment: See Recent Results From K2K.

[11-1]

Latest Results from the MINOS Experiment, A. Blake (MINOS), 2007. TAUP 2007. http://www.awa.tohoku.ac.jp/taup2007/slides/workshop14/roomB/02-TAUP2007_MINOS.pdf.

[12-1]

Measurement of the atmospheric muon charge ratio with the OPERA detector, N. Agafonova et al. (OPERA), arXiv:1003.1907, 2010.

[12-2]

Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope, J. A. Aguilar et al. (Antares), arXiv:0910.4843, 2009.

[12-3]

Measurement of the atmospheric muon flux with the NEMO Phase-1 detector, S. Aiello et al. (The NEMO), arXiv:0910.1269, 2009.

[12-4]

Observation of muon intensity variations by season with the MINOS far detector, Adamson, P. et al. (MINOS), Phys. Rev. D81 (2010) 012001, arXiv:0909.4012.

[12-5]

Time variations in the deep underground muon flux, S. Cecchini et al., Europhys. Lett. 87 (2009) 39001, arXiv:0907.5235.

[12-6]

Atmospheric MUons from PArametric formulas: a fast GEnerator for neutrino telescopes (MUPAGE), G. Carminati, A. Margiotta, M. Spurio, Comput. Phys. Commun. 179 (2008) 915-923, arXiv:0802.0562.

[12-7]

Study of multi-muon bundles in cosmic ray showers detected with the DELPHI detector at LEP, J. Abdallah et al. (DELPHI), Astropart. Phys. 28 (2007) 273-286, arXiv:0706.2561.

[12-8]

Measurement of the Atmospheric Muon Charge Ratio at TeV Energies with MINOS, P. Adamson et al. (MINOS), Phys. Rev. D76 (2007) 052003, arXiv:0705.3815.

[12-9]

Measurements of integral muon intensity at large zenith angles, A.N. Dmitrieva et al., arXiv:hep-ex/0611051, 2006.

[12-10]

Muon Flux at the Geographical South Pole, X. Bai et al., Astropart. Phys. 25 (2006) 361-367, arXiv:astro-ph/0602381.

[12-11]

Flux of atmospheric muons: Comparison between AIRES simulations and CAPRICE98 data, Hansen, P., Carlson, P., Mocchiutti, E., Sciutto, S. J., Boezio, M., Phys. Rev. D68 (2003) 103001, arXiv:hep-ph/0307199.

[12-12]

Measurements of Proton, Helium and Muon Spectra at Small Atmospheric Depths with the BESS Spectrometer, Abe, K. et al., Phys. Lett. B564 (2003) 8, arXiv:astro-ph/0304102.

[12-13]

Measurement of the residual energy of muons in the Gran Sasso underground Laboratories, M. Ambrosio et al. (MACRO), Astropart. Phys. 19 (2003) 313, arXiv:hep-ex/0207043.

[12-14]

Measurements of atmospheric muon spectra at mountain altitude, Sanuki, T. et al., Phys. Lett. B541 (2002) 234-242, arXiv:astro-ph/0205427.

[12-15]

Precise measurements of atmospheric muon fluxes with the BESS spectrometer, Motoki, M. et al., Astropart. Phys. 19 (2003) 113, arXiv:astro-ph/0205344.

[12-16]

Measurement of the flux of atmospheric muons with the CAPRICE94 apparatus, Boezio, M. et al. (WiZard/CAPRICE), Phys. Rev. D62 (2000) 032007, arXiv:hep-ex/0004014.

[12-17]

Energy spectra, altitude profiles and charge ratios of atmospheric muons, Coutu, S. et al., Phys. Rev. D62 (2000) 032001, arXiv:hep-ex/0004010.

[12-18]

Balloon measurements of cosmic ray muon spectra in the atmosphere along with those of primary protons and helium nuclei over mid-latitude, Bellotti, R. et al. (WiZard/MASS2), Phys. Rev. D60 (1999) 052002, arXiv:hep-ex/9905012.

[12-19]

A Measurement of the negative muon spectrum between 0.3- GeV/c and 40-GeV/c in the atmosphere, Bellotti, R. et al., Phys. Rev. D53 (1996) 35-43.

[12-20]

Zenith-angle dependence of cosmic ray muons, Bergeson, H. E. et al., Phys. Rev. Lett. 27 (1971) 160-163.

[12-21]

Cosmic ray muon intensity deep underground versus depth, Meyer, B. S. et al., Phys. Rev. D1 (1970) 2229-2244.

[13-1]

Measurement of the atmospheric muon flux with the ANTARES detector, Marco Bazzotti et al. (ANTARES), arXiv:0911.3055, 2009. 31st ICRC, Lodz 2009.

[13-2]

Direct Measurement of the Atmospheric Muon Energy Spectrum with IceCube, Patrick Berghaus (IceCube), arXiv:0909.0679, 2009. 31st ICRC, Lodz, Poland, July 2009.

[13-3]

Large Scale Cosmic Ray Anisotropy With IceCube, Abbasi, Rasha, Desiati, Paolo, Collaboration, for the IceCube, arXiv:0907.0498, 2009. ICRC (2009).

[13-4]

MINOS Observations of Shadowing in the Muon Flux Underground, Grashorn, E. W. (MINOS), arXiv:0710.1617, 2007. 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007.

[13-5]

Observation of Seasonal Variations with the MINOS Far Detector, E.W. Grashorn (MINOS), arXiv:0710.1616, 2007. 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007.

[13-6]

The Maximum Detectable Momentum for cosmic ray muons in the MINOS far detector, Maury Goodman (MINOS), arXiv:0706.0539, 2007. 30th International Cosmic Ray Conference, Merida Mexico 2007.

[13-7]

Interpretation of the atmospheric muon charge ratio in MINOS, Philip Schreiner, Maury Goodman (MINOS), arXiv:0706.0538, 2007. 30th International Cosmic Ray Conference, Merida Mexico 2007.

[13-8]

Measurement of the atmospheric muon spectrum from 20 to 2000 GeV, Michael Unger et al. (L3), eConf C030626 (2003) FRAP03, arXiv:hep-ex/0309002. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.

[14-1]

Atmospheric gamma-ray observation with the BETS detector for calibrating atmospheric neutrino flux calculations, Kasahara, K. et al., Phys. Rev. D66 (2002) 052004, arXiv:hep-ex/0206055.
From the article: The observed gamma-ray fluxes are compared with calculations employed by the HKKM group [15-40] wich were used in comparison with the Kamioka neutrino data. It is found that the interaction model used in the HKKM calculations is not a very good model.

[15-1]

Atmospheric lepton fluxes at ultrahigh energies, J.I. Illana, M. Masip, D. Meloni, JCAP 0909 (2009) 008, arXiv:0907.1412.

[15-2]

Prompt neutrino fluxes from atmospheric charm, Rikard Enberg, Mary Hall Reno, Ina Sarcevic, Phys. Rev. D78 (2008) 043005, arXiv:0806.0418.

[15-3]

Calculation of atmospheric neutrino flux using the interaction model calibrated with atmospheric muon data, M. Honda et al., Phys. Rev. D75 (2007) 043006, arXiv:astro-ph/0611418.

[15-4]

Uncertainties in Atmospheric Neutrino Fluxes, G.D. Barr, T.K. Gaisser, S. Robbins, T. Stanev, Phys. Rev. D74 (2006) 094009, arXiv:astro-ph/0611266.

[15-5]

Study of cosmic ray interaction model based on atmospheric muons for the neutrino flux calculation, T. Sanuki et al., Phys. Rev. D75 (2007) 043005, arXiv:astro-ph/0611201.

[15-6]

Simulation of neutrino and charged particle production and propagation in the atmosphere, L. Derome, Phys. Rev. D74 (2006) 105002, arXiv:astro-ph/0607619.

[15-7]

A semi-analytic calculation on the atmospheric tau neutrino flux due to oscillations, Fei-Fan Lee, Guey-Lin Lin, Astropart. Phys. 25 (2006) 64, arXiv:hep-ph/0412383.

[15-8]

Fluxes of Atmospheric Leptons at 600 GeV - 60 TeV, Dmitry Chirkin, arXiv:hep-ph/0407078, 2004.

[15-9]

A New calculation of the atmospheric neutrino flux in a 3-dimensional scheme, M.Honda, T.Kajita, K.Kasahara, S.Midorikawa, Phys. Rev. D70 (2004) 043008, arXiv:astro-ph/0404457.
From the abstract: We estimate the total uncertainty of the atmospheric neutrino flux prediction is reduced to below 10 GeV.... The uncertainty of the absolute normalization of the atmospheric neutrino is still large above 10 GeV due to the uncertainty of the primary cosmic ray flux above 100 GeV. However, the zenith angle variation is not affected by these uncertainties.

[15-10]

A three-dimensional calculation of atmospheric neutrinos, G.D. Barr et al., Phys. Rev. D70 (2004) 023006, arXiv:astro-ph/0403630.
From the article: We have extended the 1-dimensional neutrino flux calculation~[15-47,] to three dimensions. We compare results of the 3D and 1D calculations for neutrino energies from 100 MeV to 10 GeV over the full solid angle. Results are given for Kamioka, which is at low geomagnetic latitude, and for SNO and Soudan at high latitude.
The angle-averaged fluxes are identical within statistics for ~GeV, with approximately a 3% excess in the 3D calculation for sub-GeV neutrinos. The differences are much more noticeable in the zenith angle distributions for ~GeV, which show a significant excess in the 3D calculation for and a smaller deficit for . The differences largely cancel in the angular integral, leaving the small (3%) overall difference mentioned above. The zenith-angle differences decrease with energy and become completely negligible for ~GeV.
Corresponding to the horizontal excess in the 3D calculation is a contribution to the path length distribution of near horizontal neutrinos which reduces the average path length for horizontal neutrinos with ~MeV by 15% relative to the 1D calculation. The corresponding reduction decreases to 4% for ~GeV.

[15-11]

A 3-d simulation of the atmospheric neutrinos, Favier, J., Kossakowski, R., Vialle, J. P, Phys. Rev. D68 (2003) 093006, arXiv:astro-ph/0305460.

[15-12]

Calculation of fluxes of charged particles and neutrinos from atmospheric showers, Plyaskin, V., arXiv:hep-ph/0303146, 2003.

[15-13]

Prompt neutrinos from atmospheric c-cbar and b-bbar production and the gluon at very small x, A.D. Martin, M.G. Ryskin, A.M. Stasto, Acta Phys. Polon. B34 (2003) 3273, arXiv:hep-ph/0302140.

[15-14]

Simulation of Atmospheric Muon and Neutrino Fluxes with CORSIKA, Wentz, J. et al., Phys. Rev. D67 (2003) 073020, arXiv:hep-ph/0301199.
Comment: Comparisons at the Kamioka site between CORSIKA and FLUKA vertical neutrino fluxes are given in corsika.pdf (courtesy of G. Battistoni).

[15-15]

Atmospheric neutrino flux from 3-dimensional simulation, Liu, Yong, Derome, L., Buenerd, M., Phys. Rev. D67 (2003) 073022, arXiv:astro-ph/0211632.
From the abstract: The flux obtained at the Super-Kamiokande experiment location are reported and compared with other calculations. For low neutrino energies the flux obtained is significantly smaller than that used in the data analysis of underground experiment.

[15-16]

The FLUKA atmospheric neutrino flux calculation, Battistoni, G., Ferrari, A., Montaruli, T., Sala, P. R., Astropart. Phys. 19 (2003) 269, arXiv:hep-ph/0207035.
Comment: Fig. 17 and Fig. 18 give a crude comparison between the new FLUKA-3D calculation at the Super-Kamiokande site and the old neutrino flux calculations of Ref. [] and [15-40] that have been used extensively as input to the detector simulation. The new absolute flux normalization is clearly lower. (M.L.).

[15-17]

Comparison of the FLUKA calculations with CAPRICE94 data on muons in atmosphere, Battistoni, G., Ferrari, A., Montaruli, T., Sala, P. R., Astropart. Phys. 17 (2002) 477-488, arXiv:hep-ph/0107241.

[15-18]

Semi-analytic approximations for production of atmospheric muons and neutrinos, Gaisser, Thomas K., Astropart. Phys. 16 (2002) 285-294, arXiv:astro-ph/0104327.

[15-19]

Comparison of 3-dimensional and 1-dimensional schemes in the calculation of atmospheric neutrinos, Honda, M., Kajita, T., Kasahara, K., Midorikawa, S., Phys. Rev. D64 (2001) 053011, arXiv:hep-ph/0103328.

[15-20]

Atmospheric neutrino flux supported by recent muon experiments, Fiorentini, Giovanni, Naumov, Vadim A., Villante, Francesco L., Phys. Lett. B510 (2001) 173-188, arXiv:hep-ph/0103322.
From the abstract: A comparison with the muon fluxes and charge ratios measured in several modern balloon-borne experiments suggests that the atmospheric neutrino flux is essentially lower than one used for the standard analyses of the sub-GeV and multi-Gev neutrino induced events in underground detectors.

[15-21]

Calculation of atmospheric neutrino flux, Plyaskin, Vassily (AMS), Phys. Lett. B516 (2001) 213-235, arXiv:hep-ph/0103286.
From the article: The simulation correctly describes the fluxes of protons and leptons () measured by AMS. The results of our Monte Carlo study of propagation in space and interaction with the atmosphere of cosmic particle show that the primary proton flux in the vicinity of the Earth is essentially anisotropic at the directions approaching the horizontal plane. The horizontal region is the most important for determination of the up/down asymmetry of the atmospheric neutrino fluxes and consequently the result of the present study may affect the eventual experimental measurement of the neutrino oscillation parameter . The atmospheric neutrinos produced in our simulation have the energy spectra, relative fluxes and angular distributions different from those obtained in the previous atmospheric flux calculations.

[15-22]

The fluxes of sub-cutoff particles detected by AMS, the cosmic ray albedo and atmospheric neutrinos, Lipari, Paolo, Astropart. Phys. 16 (2002) 295-323, arXiv:astro-ph/0101559.

[15-23]

Fluxes of cosmic ray muons and atmospheric neutrinos at high energies, Volkova, L. V., Zatsepin, G. T., Phys. Atom. Nucl. 64 (2001) 266-274.

[15-24]

The east-west effect for atmospheric neutrinos, Lipari, Paolo, Astropart. Phys. 14 (2000) 171-188, arXiv:hep-ph/0003013.

[15-25]

The geometry of atmospheric neutrino production, Lipari, Paolo, Astropart. Phys. 14 (2000) 153-170, arXiv:hep-ph/0002282.

[15-26]

Primary cosmic rays, antiprotons and atmospheric neutrinos, Gaisser, T. K., Phys. Scripta T85 (2000) 100-105.

[15-27]

A three-dimensional calculation of atmospheric neutrino fluxes, Tserkovnyak, Yaroslav, Komar, Robert, Nally, Christian, Waltham, Chris, Astropart. Phys. 18 (2003) 449, arXiv:hep-ph/9907450.

[15-28]

A 3-dimensional calculation of atmospheric neutrino flux, Battistoni, G. et al., Astropart. Phys. 12 (2000) 315-333, arXiv:hep-ph/9907408.

[15-29]

Uncertainties in prompt atmospheric neutrino flux calculations, Volkova, L. V., Zatsepin, G. T., Phys. Lett. B462 (1999) 211-216.

[15-30]

Lepton fluxes from atmospheric charm, Pasquali, L., Reno, M. H., Sarcevic, I., Phys. Rev. D59 (1999) 034020, arXiv:hep-ph/9806428.

[15-31]

Atmospheric muon flux at sea level, underground and underwater, Bugaev, E. V. et al., Phys. Rev. D58 (1998) 054001, arXiv:hep-ph/9803488.

[15-32]

Geomagnetic effects on atmospheric neutrinos, Lipari, Paolo, Stanev, Todor, Gaisser, T. K., Phys. Rev. D58 (1998) 073003, arXiv:astro-ph/9803093.

[15-33]

The K(l3) form factors and atmospheric neutrino flavor ratio at high energies, Naumov, V. A., Sinegovskaya, T. S., Sinegovsky, S. I., Nuovo Cim. A111 (1998) 129-148, arXiv:hep-ph/9802410.

[15-34]

New calculation of atmospheric neutrino fluxes, Mitsui, K., Minorikawa, Y., Takazawa, M., Nuovo Cim. C21 (1998) 99-112.

[15-35]

Path length distributions of atmospheric neutrinos, Gaisser, T. K., Stanev, Todor, Phys. Rev. D57 (1998) 1977-1982, arXiv:astro-ph/9708146.

[15-36]

New limitation onto the cosmic neutrino flux recorded on earth, Volkova, L. V., Zatsepin, G. T., Bull. Russ. Acad. Sci. Phys. 61 (1997) 474-476.

[15-37]

Comparison of atmospheric neutrino flux calculations at low energies, Gaisser, T. K. et al., Phys. Rev. D54 (1996) 5578-5584, arXiv:hep-ph/9608253.

[15-38]

Atmospheric neutrino flux above 1 GeV, Agrawal, Vivek, Gaisser, T. K., Lipari, Paolo, Stanev, Todor, Phys. Rev. D53 (1996) 1314-1323, arXiv:hep-ph/9509423.

[15-39]

Charm production and high energy atmospheric muon and neutrino fluxes, Gondolo, P., Ingelman, G., Thunman, M., Astropart. Phys. 5 (1996) 309-332, arXiv:hep-ph/9505417.

[15-40]

Calculation of the flux of atmospheric neutrinos, Honda, M., Kajita, T., Kasahara, K., Midorikawa, S., Phys. Rev. D52 (1995) 4985-5005, arXiv:hep-ph/9503439.

[15-41]

A New calculation of atmospheric neutrino fluxes, Perkins, D. H., Astropart. Phys. 2 (1994) 249-256.

[15-42]

Lepton spectra in the earth's atmosphere, Lipari, P., Astropart. Phys. 1 (1993) 195-227.

[15-43]

Calculation of atmospheric neutrino fluxes, Kawasaki, M., Mizuta, S., Phys. Rev. D43 (1991) 2900-2908.

[15-44]

Atmospheric neutrino fluxes, Honda, M., Kasahara, K., Hidaka, K., Midorikawa, S., Phys. Lett. B248 (1990) 193-198.

[15-45]

A new calculation of atmospheric neutrino flux, Lee, Hae-shim, Nuovo Cim. B105 (1990) 883-887.

[15-46]

On the interpretation of the Kamiokande neutrino experiment, Bugaev, E. V., Naumov, Vadim A., Phys. Lett. B232 (1989) 391-397.

[15-47]

Flux of atmospheric neutrinos, Barr, G., Gaisser, T. K., Stanev, T., Phys. Rev. D39 (1989) 3532-3534.

[15-48]

Ratio of electron-neutrino / muon-neutrino in atmospheric neutrinos, Barr, Stephen M., Gaisser, T. K., Lipari, Paolo, Tilav, Serap, Phys. Lett. B214 (1988) 147.

[15-49]

Cosmic ray neutrinos in the atmosphere, Gaisser, T. K., Stanev, Todor, Barr, Giles, Phys. Rev. D38 (1988) 85.

[19-7]

Interactions of atmospheric neutrinos in nuclei at low- energy, Gaisser, T. K., O'Connell, J. S., Phys. Rev. D34 (1986) 822-825.

[15-51]

Spectra of atmospheric muons and neutrinos of prompt generation, Volkova, L. V., Zatsepin, G. T., Bull. Russ. Acad. Sci. Phys. 49 (1985) NO.7143.

[15-52]

Neutrino induced muon flux deep underground and search for neutrino oscillations, Gaisser, T. K., Stanev, Todor, Phys. Rev. D30 (1984) 985.

[15-53]

Prompt lepton generation - atmospheric muon and neutrino spectra at high-energies, Volkova, L. V., Zatsepin, G. T., Sov. J. Nucl. Phys. 37 (1983) 212.

[15-54]

The flux of atmospheric neutrinos, Gaisser, T. K., Stanev, Todor, Bludman, S. A., Lee, Hae-shim, Phys. Rev. Lett. 51 (1983) 223-226.

[15-55]

Energy spectra and angular distributions of atmospheric neutrinos, Volkova, L. V., Sov. J. Nucl. Phys. 31 (1980) 784-790.

[15-56]

Cosmic ray muon spectrum at sea level - primary cosmic ray nucleon spectrum, Volkova, L. V., Zatsepin, G. T., Kuzmichev, L. A., Sov. J. Nucl. Phys. 29 (1979) 645. Yad. Fiz. 29 (1979) 1252.

[15-57]

G. T. Zatsepin, V. A. Kuzmin, Sov. Phys. JETP 14 (1962) 1294.

[15-58]

On high energy neutrino physics in cosmic rays, M. A. Markov, I. M. Zheleznykh, Nucl. Phys. 27 (1961) 385-394.

[16-1]

FLUKA as a new high energy cosmic ray generator, Giuseppe Battistoni, Annarita Margiotta, Silvia Muraro, Maximiliano Sioli, arXiv:1002.4655, 2010. Very Large Volume neutrino Telescope Workshop 2009 - VLVnT09, Athens, October 2009.

[16-2]

Impact of high-energy hadron interactions on the atmospheric neutrino flux predictions, Kochanov, A. A., Sinegovskaya, T. S., Sinegovsky, S. I., arXiv:0906.0671, 2009. 31th ICRC, 7-15 July 2009, Lodz, Poland.

[16-3]

About possible contribution of intrinsic charm component to inclusive spectra of charmed mesons, E.V. Bugaev, P.A. Klimai, arXiv:0905.2309, 2009. 31st International Cosmic Ray Conference, to be held in Lodz, Poland, 2009.

[16-4]

The hadronic models for cosmic ray physics: the FLUKA code solutions, G. Battistoni et al., Nucl. Phys. Proc. Suppl. 175 (2008) 88-95, arXiv:hep-ph/0612075. ISVHECRI2006, International Symposium on Very High Energy Cosmic Rays, Weihai, China, August 15 - 22 2006.

[16-5]

Atmospheric Neutrino Fluxes, Thomas K. Gaisser, Phys. Scripta T121 (2005) 51, arXiv:astro-ph/0502380. Nobel Symposium 129 Neutrino Physics.

[16-6]

The FLUKA Monte Carlo, non-perturbative QCD and Cosmic Ray cascades, G. Battistoni et al., arXiv:hep-ph/0412178, 2004. QCD at Cosmic Ray Energies, Erice, Aug. 30 - Sep. 4 2004, Italy.

[16-7]

Atmospheric neutrino fluxes, G. Barr, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/barr.pdf.

[16-8]

The physics models of FLUKA: status and recent development, Fasso', A. et al., eConf C0303241 (2003) MOMT005, arXiv:hep-ph/0306267. 2003 Computing in High Energy and Nuclear Physics (CHEP03), La Jolla, Ca, USA, March 2003.

[16-9]

The FLUKA code: present applications and future developments, A. Fasso' et al., eConf C0303241 (2003) MOMT004, arXiv:physics/0306162. 2003 Computing in High Energy and Nuclear Physics (CHEP03), La Jolla, Ca, USA, March 2003.

[16-10]

High energy extension of the FLUKA atmospheric neutrino flux, G.Battistoni, A.Ferrari, T.Montaruli, P.R.Sala, arXiv:hep-ph/0305208, 2003. ICRC 2003.

[16-11]

The calculation of atmospheric neutrino flux, Honda, M., 2003. 4th Workshop on "Neutrino Oscillations and their Origin" (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/12/Honda-flux.pdf.

[16-12]

Atmospheric neutrino fluxes, Gaisser, Thomas K., Nucl. Phys. Proc. Suppl. 118 (2003) 109, arXiv:hep-ph/0209195. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/gaisser.

[16-13]

Atmospheric muons and neutrinos, Naumov, Vadim A., arXiv:hep-ph/0201310, 2002. 2nd Workshop on Methodical Aspects of Underwater/Ice Neutrino Telescopes, Hamburg, Germany, 15-16 Aug 2001.

[16-14]

Progresses in the validation of the FLUKA atmospheric nu flux calculations, Battistoni, G., Ferrari, A., Montaruli, T., Sala, P. R., Nucl. Phys. Proc. Suppl. 110 (2002) 336-338, arXiv:hep-ph/0112072.

[16-15]

Atmospheric proton and neutron spectra at energies above 1- GeV, Naumov, V. A., Sinegovskaya, T. S., arXiv:hep-ph/0106015, 2001.

[16-16]

Atmospheric neutrino flux and muon data, Fiorentini, G., Naumov, V. A., Villante, F. L., arXiv:hep-ph/0106014, 2001.

[16-17]

Atmospheric neutrino flux calculations, Battistoni, G., Nucl. Phys. Proc. Suppl. 100 (2001) 101-106.

[16-18]

Review of sources of atmospheric neutrinos, Lipari, P., Nucl. Phys. Proc. Suppl. 91 (2001) 159-166.

[16-19]

Systematic uncertainties in the prediction of the atmospheric nu fluxes, Lipari, P., Nucl. Phys. Proc. Suppl. 100 (2001) 136-138.

[16-20]

Neutrini al Gran Sasso, Vissani, F., 2001. Neutrini al Gran Sasso - 25 March 2002, Padova, Italy. http://www.pd.infn.it/~laveder/cngspd/trasparenze/Vissani.pdf.
Comment: Slide n.10 gives the comparison between Superkamiokande atmospheric neutrino data (Sub-Gev and Multi-GeV samples as a function of zenith angle) and various MC neutrino flux calculations. In green FLUKA, in blue the NEW HONDA, in red the OLD HONDA. The comparison is taken from M.Shiozawa's Review on experimental results on cosmic ray neutrinos - AMS collaboration meeting - October 2001 - Trento - Italy. In the case of FLUKA MC calculation an excess of electron-like data events is clearly visible in both the Sub-GeV and the Multi-GeV samples. (M.L.).

[16-21]

Atmospheric neutrino sources: A review, Lipari, P., 2001. Published in "Venice 2001, Neutrino Telescopes, vol. 1" 221-246.

[16-22]

A Three-dimensional calculation of atmospheric neutrino fluxes, Tserkovnyak, Y., Komar, R. J., Nally, C. W., Waltham, C. E., 2001. 27th International Cosmic Ray Conference (ICRC 2001), Hamburg, Germany, 7-15 Aug 2001.

[16-23]

Primary spectrum to 1-TeV and beyond, Gaisser, T. K., Stanev, T., Honda, M., Lipari, P., 2001. 27th International Cosmic Ray Conference (ICRC 2001), Hamburg, Germany, 7-15 Aug 2001. http://www.copernicus.org/icrc/papers/ici6694_p.pdf.

[16-24]

Uncertainties on atmospheric neutrino flux calculations, Battistoni, G., Nucl. Phys. Proc. Suppl. 100 (2000) 101-106, arXiv:hep-ph/0012268.

[16-25]

Atmospheric neutrino flux: A review of calculations, Gaisser, T. K., Nucl. Phys. Proc. Suppl. 87 (2000) 145-151, arXiv:hep-ph/0001027.

[16-26]

The primary protons and the atmospheric neutrino fluxes, Lipari, Paolo, arXiv:hep-ph/9905506, 1999.

[16-27]

Fluxes of muons and showers with a given energy release from atmospheric neutrinos at energies 10^3-GeV to 10^7- GeV, Volkova, L. V., Zatsepin, G. T., Bull. Russ. Acad. Sci. Phys. 63 (1999) 459-461.

[16-28]

A new calculation of atmospheric neutrino flux: The FLUKA approach, Battistoni, G. et al., Nucl. Phys. Proc. Suppl. 70 (1999) 358-360.

[16-29]

Limits on calculated atmospheric neutrino fluxes at high energies, Volkova, L. V., 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.

[16-30]

Calculation of atmospheric neutrino and the sensitivity of angular dependences to various models, Honda, M., Kasahara, K., Midorikawa, S., 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.

[16-31]

Uncertainty of the atmospheric neutrino fluxes, Honda, M., Nucl. Phys. Proc. Suppl. 77 (1999) 140-145, arXiv:hep-ph/9811504.

[16-32]

Fluxes of atmospheric neutrinos and related cosmic rays, Gaisser, T. K., Nucl. Phys. Proc. Suppl. 77 (1999) 133-139, arXiv:hep-ph/9811315.

[16-33]

Primary cosmic-ray spectrum and the intensity of atmospheric neutrinos, Gaisser, Thomas K., arXiv:hep-ph/9811314, 1998.

[16-34]

Muon and muon-neutrino fluxes from atmospheric charm, Pasquali, L., Reno, M. H., Sarcevic, I., Nucl. Phys. Proc. Suppl. 70 (1999) 361-363, arXiv:hep-ph/9711457. 5th International Workshop on Topics in Astroparticle and Underground Physics (TAUP 97), Gran Sasso, Italy, 7-11 Sep 1997.

[16-35]

Atmospheric Neutrinos, Honda, Morihiro, Kajita, Takaaki, Kasahara, Katsuaki, Midorikawa, Shoichi, Prog. Theor. Phys. Suppl. 123 (1996) 483-490, arXiv:hep-ph/9511223.

[16-36]

Fluxes of muon-neutrino and electron-neutrino in the atmosphere: Is there an anomaly?, Gaisser, T. K., Nucl. Phys. Proc. Suppl. 35 (1994) 209-215.

[16-37]

Calculation of low-energy atmospheric neutrino fluxes, Honda, M., 1994.

[16-38]

Atmopheric neutrino event rates: The Expectations, Gaisser, T. K., 1993. Neutrino Astronomy Discussion Meeting, London, England, 9-10 June 1993.

[16-39]

Atmospheric neutrinos, Stanev, T., 1993. 5th International Symposium on Neutrino Telescopes, Venice, Italy, 2-4 Mar 1993.

[16-40]

The anomalous atmospheric neutrino flux and the possibility of neutrino oscillation, Midorikawa, S., Honda, M., Kasahara, K., 1991. 5th Workshop on Elementary-Particle Picture of the Universe, Izu, Japan, 19 Nov 1991.

[16-41]

Cosmic ray muons and atmospheric neutrinos, Volkova, L. V., 1990. High energy phenomenology, Campinas 1990.

[16-42]

A Comment on electron-neutrino / muon-neutrino ratio in atmospheric neutrino fluxes, Volkova, L. V., 1988. Cosmic gamma rays, neutrinos, and related astrophysics, Erice 1988.

[16-43]

Atmospheric muons and neutrinos of low and medium energies, Bugaev, E. V., Naumov, Vadim A., 1987. 20th International Cosmic Ray Conference, Moscow, USSR, 2-15 Aug 1987.

[16-44]

Muons and neutrinos, Stanev, T., 1985. 9th Int. Conf. on Cosmic Rays, San Diego, CA, Aug 11-23, 1985.

[16-45]

Atmospheric neutrinos in underground detectors, Gaisser, T. K., Stanev, T., 1984. Neutrino Physics and Astrophysics, Nordkirchen 1984.

[16-46]

Interaction rates of atmospheric neutrinos, Gaisser, T. K., Stanev, Todor, 1984. ICOBAN '84, Park City, Utah, Jan 4-7, 1984.

[16-47]

Atmospheric neutrino fluxes at low-energy, Stanev, T., Gaisser, T. K., 1984. Solar neutrinos and neutrino astronomy, Kyoto 1979.

[16-48]

High-energy cosmic ray atmospheric neutrinos, Volkova, L. V., 1979. 16th International Cosmic Ray Conference, Muenchen 1975.

16-49.

R. Cowsik, 1963. Eighth International Conference on Cosmic Rays, Jaipur, India, December 1963.

16-50.

K. Greisen, 1960. International Conference on Instrumentation for High-Energy Physics, Berkeley, California, September 1960.

[17-1]

Ultra-high Energy Predictions of proton-air Cross Sections from Accelerator Data, Block, M. M., Phys. Rev. D76 (2007) 111503, arXiv:0705.3037.

[18-1]

Results from HARP and their implications for neutrino physics, Boris A. Popov (HARP), arXiv:0705.3512, 2007. XLIInd Rencontres de Moriond on Electroweak Interactions and Unified Theories.

[18-2]

The Elusive p-air Cross Section, Martin M. Block, Czech. J. Phys. 56 (2006) A77-A90, arXiv:hep-ph/0606186. c2cr2005 Conference, Prague, September 7-13, 2005.

[18-3]

Low-Energy Hadron Production Data and Current Status of CERN Measurements, Giles Barr, Ralph Engel, Nucl. Phys. Proc. Suppl. 151 (2006) 175, arXiv:astro-ph/0504356. XIII ISVHECRI, Pylos (Greece), Sept. 2004.

[18-4]

First physics results from the HARP experiment at CERN, A. Cervera Villanueva, arXiv:hep-ex/0406053, 2004. Rencontres de Moriond 2004.

[19-1]

Quasi-elastic neutrino charged-current scattering cross sections on oxygen, Butkevich, A. V., Kulagin, S. A., Phys. Rev. C76 (2007) 045502, arXiv:0705.1051.

[19-2]

Local density and the RPA corrections in charge current quasielastic neutrino on oxygen, argon and iron scattering, Graczyk, Krzysztof M., arXiv:nucl-th/0401053, 2004.

[19-3]

Low energy neutrino cross sections: Comparison of various Monte Carlo predictions to experimental data, Zeller, G. P., arXiv:hep-ex/0312061, 2003.

[19-4]

Nuclear correlation effects in neutrino oxygen interactions and the atmospheric neutrino anomaly, Marteau, J., Delorme, J., Ericson, M., Nucl. Phys. A663 (2000) 783-786.

[19-5]

Atmospheric neutrino absorption cross-sections in Ar-40, Athar, M. Sajjad, Singh, S. K., Phys. Rev. C61 (2000) 028501.

[19-6]

Simulation of nuclear effects in quasi elastic and resonant neutrino interactions, Battistoni, G., Lipari, P., Ranft, J., Scapparone, E., arXiv:hep-ph/9801426, 1998.

[19-7]

Interactions of atmospheric neutrinos in nuclei at low- energy, Gaisser, T. K., O'Connell, J. S., Phys. Rev. D34 (1986) 822-825.

[20-1]

Neutrino oscillation studies and the neutrino cross section, Lipari, Paolo, Nucl. Phys. Proc. Suppl. 112 (2002) 274-287, arXiv:hep-ph/0207172. 1st workshop on neutrino-nucleus interactions in the few GeV region (NuInt01), Tsukuba, Japan, 13-16 Dec 2001.

[20-2]

Comparisons of real and simulated data, Zeller, G., 2002. Second International Workshop on Neutrino-Nucleus Interactions in the few-GeV Region, NUINT'02, December 12-15, 2002 University of California, Irvine. http://www.ps.uci.edu/~nuint/slides/Zeller.pdf.

[21-1]

Reconstruction of Composite Events in Neutrino Telescopes, Mathieu Ribordy, Nucl. Instrum. Meth. A574 (2007) 137-143, arXiv:astro-ph/0611604.

[22-1]

Long range forces, oscillation parameters and mass hierarchy with atmospheric neutrinos at a magnetized muon detector, Abhijit Samanta, arXiv:1001.5344, 2010.

[22-2]

Updated global fit to three neutrino mixing: status of the hints of theta13 > 0, M.C. Gonzalez-Garcia, Michele Maltoni, Jordi Salvado, arXiv:1001.4524, 2010.

[22-3]

High energy leptons from muons in transit, Alexander Bulmahn, Mary Hall Reno, arXiv:0912.1385, 2009.

[22-4]

Prospects of measuring the leptonic CP phase with atmospheric neutrinos, Abhijit Samanta, Phys. Rev. D80 (2009) 073008, arXiv:0907.3978.

[22-5]

A comparison of the ways of resolving mass hierarchy with atmospheric neutrinos, Abhijit Samanta, Phys. Rev. D 81 (2010) 037302, arXiv:0907.3540.

[22-6]

Neutrino mass hierarchy determination for , Raj Gandhi, Pomita Ghoshal, Srubabati Goswami, S Uma Sankar, arXiv:0905.2382, 2009.

[22-7]

Implications of the Super-K atmospheric data for the mixing angles and , Roa, J. E., Latimer, D. C., Ernst, D. J., Phys. Rev. C81 (2010) 015501, arXiv:0904.3930.

[22-8]

Sensitivity on Earth Core and Mantle densities using Atmospheric Neutrinos, E. Borriello et al., JCAP 0906 (2009) 030, arXiv:0904.0796.

[22-9]

Oscillations of very low energy atmospheric neutrinos, Peres, O. L. G., Smirnov, A. Yu., Phys. Rev. D79 (2009) 113002, arXiv:0903.5323.

[22-10]

The physics impact of proton track identification in future megaton-scale water Cherenkov detectors, M. Fechner, C.W. Walter, JHEP 11 (2009) 040, arXiv:0901.1950.

[22-11]

A comparison of the sensitivities of the parameters with atmospheric neutrinos for different analysis methods, Abhijit Samanta, Phys. Rev. D79 (2009) 053011, arXiv:0812.4640.

[22-12]

Exceptional sensitivities of neutrino mixing parameters with atmospheric neutrinos, Abhijit Samanta, Phys. Rev. D80 (2009) 113003, arXiv:0812.4639.

[22-13]

Vetoing atmospheric neutrinos in a high energy neutrino telescope, Schonert, Stefan, Gaisser, Thomas K., Resconi, Elisa, Schulz, Olaf, Phys. Rev. D79 (2009) 043009, arXiv:0812.4308.

[22-14]

Three-flavour neutrino oscillation update, Schwetz, Thomas, Tortola, Mariam, Valle, Jose W. F., New J. Phys. 10 (2008) 113011, arXiv:0808.2016.

[22-15]

Resolving the Mass Hierarchy with Atmospheric Neutrinos using a Liquid Argon Detector, Gandhi, Raj, Ghoshal, Pomita, Goswami, Srubabati, Sankar, S Uma, Phys. Rev. D78 (2008) 073001, arXiv:0807.2759.

[22-16]

Mass hierarchy determination using atmospheric neutrinos for small , Gandhi, Raj, Ghoshal, Pomita, Goswami, Srubabati, Sankar, S. Uma, arXiv:0805.3474, 2008.

[22-17]

Atmospheric neutrino oscillation data constraints on , Escamilla, J., Latimer, D. C., Ernst, D. J., Phys. Rev. Lett. 103 (2009) 061804, arXiv:0805.2924.

[22-18]

Observables sensitive to absolute neutrino masses (Addendum), Fogli, G. L. et al., Phys. Rev. D78 (2008) 033010, arXiv:0805.2517.

[22-19]

Neutrino oscillograms of the Earth: effects of 1-2 mixing and CP-violation, Evgeny Kh. Akhmedov, Michele Maltoni, Alexei Yu. Smirnov, JHEP 06 (2008) 072, arXiv:0804.1466.

[22-20]

Neutrino mass hierarchy extraction using atmospheric neutrinos in ice, Olga Mena, Irina Mocioiu, Soebur Razzaque, Phys. Rev. D78 (2008) 093003, arXiv:0803.3044.

[22-21]

Status of Oscillation plus Decay of Atmospheric and Long-Baseline Neutrinos, M.C. Gonzalez-Garcia, M. Maltoni, Phys. Lett. B663 (2008) 405-409, arXiv:0802.3699.

[22-22]

Probing new physics with long-lived charged particles produced by atmospheric and astrophysical neutrinos, Shin'ichiro Ando, John F. Beacom, Stefano Profumo, David Rainwater, JCAP 0804 (2008) 029, arXiv:0711.2908.

[22-23]

Signature of sterile species in atmospheric neutrino data at neutrino telescopes, Choubey, Sandhya, JHEP 12 (2007) 014, arXiv:0709.1937.

[22-24]

Mass Hierarchy Determination via future Atmospheric Neutrino Detectors, Raj Gandhi et al., Phys. Rev. D76 (2007) 073012, arXiv:0707.1723.

[22-25]

Challenging Lorentz noninvariant neutrino oscillations without neutrino masses, Barger, V., Marfatia, D., Whisnant, K., Phys. Lett. B653 (2007) 267-277, arXiv:0706.1085.

[22-26]

Detecting atmospheric neutrino oscillations in ATLAS, Kopp, Joachim, Lindner, Manfred, Phys. Rev. D76 (2007) 093003, arXiv:0705.2595.

[22-27]

Probing Lorentz invariance violation in atmospheric neutrino oscillations with a neutrino telescope, Dean Morgan, Elizabeth Winstanley, Jurgen Brunner, Lee F. Thompson, arXiv:0705.1897, 2007.

[22-28]

A GEANT-based study of atmospheric neutrino oscillation parameters at INO, Abhijit Samanta et al., Int. J. Mod. Phys. A23 (2008) 233-245, arXiv:hep-ph/0702180.

[22-29]

1-3 leptonic mixing and the neutrino oscillograms of the Earth, Evgeny Kh. Akhmedov, Michele Maltoni, Alexei Yu. Smirnov, JHEP 05 (2007) 077, arXiv:hep-ph/0612285.

[22-30]

The mass hierarchy with atmospheric neutrinos at INO, Abhijit Samanta, Phys. Lett. B673 (2009) 37-46, arXiv:hep-ph/0610196.

[22-31]

Determination of the Atmospheric Neutrino Fluxes from Atmospheric Neutrino Data, M.C. Gonzalez-Garcia, M. Maltoni, J. Rojo, JHEP 10 (2006) 075, arXiv:hep-ph/0607324.

[22-32]

What does the muon-neutrino oscillate into?, Debajyoti Choudhury, Anindya Datta, arXiv:hep-ph/0606100, 2006.

[22-33]

Neutrino oscillation probabilities: Sensitivity to parameters, Indumathi, D., Murthy, M. V. N., Rajasekaran, G., Sinha, Nita, Phys. Rev. D74 (2006) 053004, arXiv:hep-ph/0603264.

[22-34]

Determining the Neutrino Mass Hierarchy with Atmospheric Neutrinos, S.T. Petcov, T. Schwetz, Nucl. Phys. B740 (2006) 1, arXiv:hep-ph/0511277.

[22-35]

Earth matter density uncertainty in atmospheric neutrino oscillations, Pei-Hong Gu, Phys. Rev. D72 (2005) 097301, arXiv:hep-ph/0511028.

[22-36]

Probing the deviation from maximal mixing of atmospheric neutrinos, Sandhya Choubey, Probir Roy, Phys. Rev. D73 (2006) 013006, arXiv:hep-ph/0509197.

[22-37]

Probing the Neutrino Mass Hierarchy via Atmospheric Survival Rates in Megaton Water Cerenkov Detectors, Raj Gandhi et al., arXiv:hep-ph/0506145, 2005.

[22-38]

A test of tau neutrino interactions with atmospheric neutrinos and K2K, Alexander Friedland, Cecilia Lunardini, Phys. Rev. D72 (2005) 053009, arXiv:hep-ph/0506143.

[22-39]

Neutrino Data and Neutrino-Antineutrino Transition, E.N. Alexeyev, L.V. Volkova, arXiv:hep-ph/0504282, 2005.

[22-40]

Another possible way to determine the neutrino mass hierarchy, Nunokawa, Hiroshi, Parke, Stephen, Funchal, Renata Zukanovich, Phys. Rev. D72 (2005) 013009, arXiv:hep-ph/0503283.

[22-41]

Search for a Lorentz invariance violation contribution in atmospheric neutrino oscillations using MACRO data, Battistoni, G. et al., Phys. Lett. B615 (2005) 14, arXiv:hep-ex/0503015.

[22-42]

Physics Reach of High-Energy and High-Statistics IceCube Atmospheric Neutrino Data, M.C. Gonzalez-Garcia, F. Halzen, M. Maltoni, Phys. Rev. D71 (2005) 093010, arXiv:hep-ph/0502223.

[22-43]

Resolving parameter degeneracies in long-baseline experiments by atmospheric neutrino data, Huber, P., Maltoni, M., Schwetz, T., Phys. Rev. D71 (2005) 053006, arXiv:hep-ph/0501037.

[22-44]

Probing quantum decoherence in atmospheric neutrino oscillations with a neutrino telescope, Dean Morgan, Elizabeth Winstanley, Jurgen Brunner, Lee F. Thompson, Astropart. Phys. 25 (2006) 311-327, arXiv:astro-ph/0412618.

[22-45]

Three neutrino flavor oscillations and the atmospheric tau neutrinos, H. Athar, arXiv:hep-ph/0411303, 2004.

[22-46]

Flavor symmetry L(e) - L(mu) - L(tau), atmospheric neutrino mixing and CP violation in the lepton sector, Petcov, S. T., Rodejohann, W., Phys. Rev. D71 (2005) 073002, arXiv:hep-ph/0409135.

[22-47]

Shower Power: Isolating the Prompt Atmospheric Neutrino Flux Using Electron Neutrinos, John F. Beacom, Julian Candia, JCAP 0411 (2004) 009, arXiv:hep-ph/0409046.

[22-48]

Large Matter Effects in Oscillations, Raj Gandhi et al., Phys. Rev. Lett. 94 (2005) 051801, arXiv:hep-ph/0408361.

[22-49]

Atmospheric neutrinos as probes of neutrino-matter interactions, Friedland, Alexander, Lunardini, Cecilia, Maltoni, Michele, Phys. Rev. D70 (2004) 111301, arXiv:hep-ph/0408264.

[22-50]

Measuring the deviation of the 2-3 lepton mixing from maximal with atmospheric neutrinos, Gonzalez-Garcia, M. C., Maltoni, M., Smirnov, A. Yu., Phys. Rev. D70 (2004) 093005, arXiv:hep-ph/0408170.

[22-51]

A question of hierarchy: matter effects with atmospheric neutrinos and anti-neutrinos, D. Indumathi, M.V.N. Murthy, Phys. Rev. D71 (2005) 013001, arXiv:hep-ph/0407336.

[22-52]

Atmospheric Neutrino Constraints on Lorentz Violation, Sheldon Lee Glashow, arXiv:hep-ph/0407087, 2004.

[22-53]

Possible neutrino gravitoelectric dipole moments and atmospheric and solar neutrino anomalies, An. S. Kuznetsov, arXiv:hep-ph/0407031, 2004.

[22-54]

Three-Neutrino Oscillations of Atmospheric Neutrinos, , Neutrino Mass Hierarchy and Iron Magnetized Detectors, Sergio Palomares-Ruiz, S.T. Petcov, Nucl. Phys. B712 (2005) 392, arXiv:hep-ph/0406096.

[22-55]

Detector Depth Dependence of the High Energy Atmospheric Neutrino Flux, John M. LoSecco, Phys. Rev. D70 (2004) 097301, arXiv:hep-ex/0406072.

[22-56]

Atmospheric Neutrino Oscillations and New Physics, M.C. Gonzalez-Garcia, Michele Maltoni, Phys. Rev. D70 (2004) 033010, arXiv:hep-ph/0404085.

[22-57]

Probing oscillations into sterile neutrinos with cosmology, astrophysics and experiments, Marco Cirelli, Guido Marandella, Alessandro Strumia, Francesco Vissani, Nucl. Phys. B708 (2005) 215, arXiv:hep-ph/0403158.

[22-58]

Deviation of Atmospheric Mixing from Maximal and Structure in the Leptonic Flavor Sector, Andre de Gouvea, Phys. Rev. D69 (2004) 093007, arXiv:hep-ph/0401220.

[22-59]

Atmospheric neutrinos and nu-mass hierarchy, Jose Bernabeu, Sergio Palomares-Ruiz, Nucl. Phys. Proc. Suppl. 138 (2005) 398, arXiv:hep-ph/0312038.

[22-60]

Atmospheric Neutrinos as a Probe of CPT and Lorentz Violation, Anindya Datta, Raj Gandhi, Poonam Mehta, S Uma Sankar, Phys. Lett. B597 (2004) 356, arXiv:hep-ph/0312027.

[22-61]

Constraints on flavour-dependent long-range forces from atmospheric neutrino observations at Super-Kamiokande, Anjan S. Joshipura, Subhendra Mohanty, Phys. Lett. B584 (2004) 103, arXiv:hep-ph/0310210.

[22-62]

Three-neutrino model analysis of the world's oscillation data, D. C. Latimer, D. J. Ernst, arXiv:nucl-th/0310083, 2003.
Comment: Another junk paper in which it is claimed that solar, atmospheric and LSND data can be fitted in a three-neutrino model.
Important data (energy spectra) are omitted and the analysis is very approximate.
The claimed best-fit values of the largest are either or .
The smaller value give in LSND. Therefore, this case is equivalent to neglect LSND.
The larger values obviously cannot fit the energy spectra of atmospheric neutrinos, which have been omitted in the analysis.
[C.G.].

[22-63]

Atmospheric neutrinos: LMA oscillations, Ue3 induced interference and CP-violation, O. L. G. Peres, A. Yu. Smirnov, Nucl. Phys. B680 (2004) 479, arXiv:hep-ph/0309312.

[22-64]

Three-Neutrino Mixing after the First Results from K2K and KamLAND, M. C. Gonzalez-Garcia, Carlos Pena-Garay, Phys. Rev. D68 (2003) 093003, arXiv:hep-ph/0306001.

[22-65]

Atmospheric Neutrino Oscillations, theta(13) and Neutrino Mass Hierarchy, J. Bernabeu, Sergio Palomares-Ruiz, S. T. Petcov, Nucl. Phys. B669 (2003) 255, arXiv:hep-ph/0305152.

[22-66]

Status of atmospheric oscillations and decoherence after the first K2K spectral data, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Rev. D67 (2003) 093006, arXiv:hep-ph/0303064.

[22-67]

Some comments on Super-Kamiokande's multi-ring analysis, R. Foot, arXiv:hep-ph/0303005, 2003.

[22-68]

Neutral-Current Atmospheric Neutrino Flux Measurement Using Neutrino-Proton Elastic Scattering in Super-Kamiokande, J. F. Beacom, Sergio Palomares-Ruiz, Phys. Rev. D67 (2003) 093001, arXiv:hep-ph/0301060.

[22-69]

Charge ratio of muons from atmospheric neutrinos, T.K. Gaisser, Todor Stanev, Phys. Lett. B561 (2003) 125, arXiv:astro-ph/0210512.

[22-70]

Identification problems of muon and electron events in the Super-Kamiokande detector, Mitsui, K., Kitamura, T., Wada, T., Okei, K., J. Phys. G29 (2003) 2281, arXiv:hep-ex/0209041.
From the article: ... we conclude that due to the uncertainty of the identification capability for muon and electron events in Super K. detector one cannot yet firmly establish the existence of an atmospheric neutrino anomaly.

[22-71]

The nuance Neutrino Simulation, and the Future, Casper, D., Nucl. Phys. Proc. Suppl. 112 (2002) 161-170, arXiv:hep-ph/0208030.

[22-72]

Three-flavor solar neutrino oscillations with terrestrial neutrino constraints, Fogli, G. L. et al., Phys. Rev. D66 (2002) 093008, arXiv:hep-ph/0208026.

[22-73]

Constraining neutrino oscillation parameters with current solar and atmospheric data, Maltoni, M., Schwetz, T., Tortola, M. A., Valle, J. W. F., Phys. Rev. D67 (2003) 013011, arXiv:hep-ph/0207227.

[22-74]

Ruling out four-neutrino oscillation interpretations of the LSND anomaly?, Maltoni, M., Schwetz, T., Tortola, M. A., Valle, J. W. F., Nucl. Phys. B643 (2002) 321-338, arXiv:hep-ph/0207157.
From the abstract: ... all four-neutrino descriptions of the LSND anomaly, both in (2+2) as well as (3+1) realizations, are highly disfavoured. Our analysis brings the LSND hint to a more puzzling status.
From the article: The exclusion of four-neutrino oscillation schemes of the (2+2)-type is based on the improved sensitivity of solar and atmospheric neutrino experiments to oscillations into a sterile neutrino, thanks to recent experimental data. This is a very robust result, independent of whether the LSND experiment is confirmed or disproved. The exclusion of (3+1) schemes depends somehow on the used LSND data. Furthermore, it heavily relies on the results of negative SBL experiments, especially on the Bugey and CDHS disappearance experiments.

[22-75]

Prospects of measuring and the sign of with a massive magnetized detector for atmospheric neutrinos, Tabarelli de Fatis, T., Eur. Phys. J. C24 (2002) 43-50, arXiv:hep-ph/0202232.

[22-76]

Two mass-scale oscillation analysis of atmospheric and reactor data, Gonzalez-Garcia, M. C., Maltoni, M., Eur. Phys. J. C26 (2003) 417, arXiv:hep-ph/0202218.

[22-77]

The earth mantle-core effect in matter-induced asymmetries for atmospheric neutrino oscillations, Bernabeu, J., Palomares-Ruiz, S., Perez, A., Petcov, S. T., Phys. Lett. B531 (2002) 90-98, arXiv:hep-ph/0110071.

[22-78]

Non-standard interactions: Atmospheric versus neutrino factory experiments, Huber, P., Valle, J. W. F., Phys. Lett. B523 (2001) 151-160, arXiv:hep-ph/0108193.

[22-79]

Probing neutrino non-standard interactions with atmospheric neutrino data, Fornengo, N., Maltoni, M., Bayo, R. Tomas, Valle, J. W. F., Phys. Rev. D65 (2002) 013010, arXiv:hep-ph/0108043.

[22-80]

Is right-handed neutrino degeneracy compatible with the solar and atmospheric neutrino data?, Gonzalez Felipe, R., Joaquim, F. R., JHEP 09 (2001) 015, arXiv:hep-ph/0106226.

[22-81]

Combining LSND and atmospheric anomalies in a three- neutrino picture, Barenboim, Gabriela, Dighe, Amol, Skadhauge, Solveig, Phys. Rev. D65 (2002) 053001, arXiv:hep-ph/0106002.

[22-82]

Solar and atmospheric four-neutrino oscillations, Gonzalez-Garcia, M. C., Maltoni, M., Pena-Garay, Carlos, Phys. Rev. D64 (2001) 093001, arXiv:hep-ph/0105269.

[22-83]

Solutions of the atmospheric, solar and LSND neutrino anomalies from TeV scale quark lepton unification, Yoon, T. L., Foot, R., Phys. Rev. D65 (2002) 015002, arXiv:hep-ph/0105101.

[22-84]

Medium effects for terrestrial and atmospheric neutrino oscillations, Banuls, M. C., Barenboim, G., Bernabeu, J., Phys. Lett. B513 (2001) 391-400, arXiv:hep-ph/0102184.

[22-85]

Measuring atmospheric neutrino oscillations with neutrino telescopes, Albuquerque, Ivone F. M., Smoot, George F., Phys. Rev. D64 (2001) 053008, arXiv:hep-ph/0102078.

[22-86]

The Relevance of the muon charge ratio for the atmospheric neutrino anomaly, Wentz, J. et al., J. Phys. G27 (2001) 1699-1708.

[22-87]

Weak and electromagnetic nuclear decay signatures for neutrino reactions in Super-Kamiokande, Nussinov, S., Shrock, R., Phys. Rev. Lett. 86 (2001) 2223-2226, arXiv:hep-ph/0009334.

[22-88]

Four-neutrino oscillation solutions of the atmospheric neutrino anomaly, Fogli, Gian Luigi, Lisi, E., Marrone, A., Phys. Rev. D63 (2001) 053008, arXiv:hep-ph/0009299.

[22-89]

Analysis of the Super-Kamiokande atmospheric neutrino data in the framework of four neutrino mixings, Yasuda, Osamu, Nucl. Instrum. Meth. A472 (2000) 343-347, arXiv:hep-ph/0007076.

[22-90]

Is the -> oscillation solution to the atmospheric neutrino anomaly excluded by the Super-Kamiokande data?, Foot, R., Phys. Lett. B496 (2000) 169-174, arXiv:hep-ph/0007065.

[22-91]

Neutrino masses and mixings from supersymmetry with bilinear R-parity violation: A theory for solar and atmospheric neutrino oscillations, Hirsch, M., Diaz, M. A., Porod, W., Romao, J. C., Valle, J. W. F., Phys. Rev. D62 (2000) 113008, arXiv:hep-ph/0004115.

[22-92]

A three generation oscillation analysis of the Super- Kamiokande atmospheric neutrino data beyond one mass scale dominance approximation, Choubey, Sandhya, Goswami, Srubabati, Kar, Kamales, Astropart. Phys. 17 (2002) 51-73, arXiv:hep-ph/0004100.

[22-93]

Analysis of atmospheric neutrino oscillations in three- flavor neutrinos, Teshima, T., Sakai, T., Phys. Rev. D62 (2000) 113010, arXiv:hep-ph/0003038.

[22-94]

Updated global analysis of the atmospheric neutrino data in terms of neutrino oscillations, Fornengo, N., Gonzalez-Garcia, M. C., Valle, J. W. F., Nucl. Phys. B580 (2000) 58-82, arXiv:hep-ph/0002147.

[22-95]

Probing possible decoherence effects in atmospheric neutrino oscillations, Lisi, E., Marrone, A., Montanino, D., Phys. Rev. Lett. 85 (2000) 1166-1169, arXiv:hep-ph/0002053.

[22-96]

The atmospheric neutrino anomaly without maximal mixing?, De Rujula, A., Gavela, M. B., Hernandez, P., Phys. Rev. D63 (2001) 033001, arXiv:hep-ph/0001124.

[22-97]

The role of muons for the atmospheric neutrino anomaly, Wentz, J., Rom. J. Phys. 45 (2000) 255-258.

[22-98]

Can lepton flavor violating interactions explain the atmospheric neutrino problem?, Bergmann, Sven, Grossman, Yuval, Pierce, Damien M., Phys. Rev. D61 (2000) 053005, arXiv:hep-ph/9909390.

[22-99]

A mass matrix for atmospheric, solar, and LSND neutrino oscillations, Gelb, James M., Rosen, S. P., Phys. Rev. D62 (2000) 013003, arXiv:hep-ph/9909293.

[22-100]

An SU(2)L x U(1)Y x S(3) x D model for atmospheric and solar neutrino deficits, Ray, Asim K., Sarkar, Saswati, Phys. Rev. D61 (2000) 035007, arXiv:hep-ph/9908294.

[22-101]

The interpretation of the atmospheric neutrino data and cosmological constraints, Di Bari, Pasquale, Lipari, Paolo, Lusignoli, Maurizio, Int. J. Mod. Phys. A15 (2000) 2289-2328, arXiv:hep-ph/9907548.

[22-102]

A supersymmetric solution to the solar and atmospheric neutrino problems, Romao, J. C., Diaz, M. A., Hirsch, M., Porod, W., Valle, J. W. F, Phys. Rev. D61 (2000) 071703, arXiv:hep-ph/9907499.

[22-103]

Neutrino decay and atmospheric neutrinos, Barger, V. D. et al., Phys. Lett. B462 (1999) 109-114, arXiv:hep-ph/9907421.

[22-104]

On the interpretation of the atmospheric neutrino data in terms of flavor changing neutrino interactions, Fornengo, N., Gonzalez-Garcia, M. C., Valle, J. W. F., JHEP 07 (2000) 006, arXiv:hep-ph/9906539.

[22-105]

Is neutrino decay really ruled out as a solution to the atmospheric neutrino problem from Super-Kamiokande data?, Choubey, Sandhya, Goswami, Srubabati, Astropart. Phys. 14 (2000) 67-78, arXiv:hep-ph/9904257.

[22-106]

Testing violations of special and general relativity through the energy dependence of <-> oscillations in the Super-Kamiokande atmospheric neutrino experiment, Fogli, Gian Luigi, Lisi, E., Marrone, A., Scioscia, G., Phys. Rev. D60 (1999) 053006, arXiv:hep-ph/9904248.

[22-107]

Atmospheric and solar neutrinos from single right-handed neutrino dominance and U(1) family symmetry, King, S. F., Nucl. Phys. B562 (1999) 57-77, arXiv:hep-ph/9904210.

[22-108]

Can the Super-Kamiokande atmospheric data predict the solar neutrino deficit?, Stancu, Ion, Mod. Phys. Lett. A14 (1999) 689-700, arXiv:hep-ph/9903552.

[22-109]

Four-neutrino mass spectra and the Super-Kamiokande atmospheric up-down asymmetry, Bilenky, Samoil M., Giunti, C., Grimus, W., Schwetz, T., Phys. Rev. D60 (1999) 073007, arXiv:hep-ph/9903454.

[22-110]

Simple connection between atmospheric and solar neutrino vacuum oscillations, Ma, Ernest, Phys. Rev. Lett. 83 (1999) 2514-2517, arXiv:hep-ph/9902392.

[22-111]

Testing the solar neutrino conversion with atmospheric neutrinos, Peres, O. L. G., Smirnov, A. Yu., Phys. Lett. B456 (1999) 204-213, arXiv:hep-ph/9902312.

[22-112]

Super-Kamiokande data and atmospheric neutrino decay, Fogli, Gian Luigi, Lisi, E., Marrone, A., Scioscia, G., Phys. Rev. D59 (1999) 117303, arXiv:hep-ph/9902267.

[22-113]

On exotic solutions of the atmospheric neutrino problem, Lipari, Paolo, Lusignoli, Maurizio, Phys. Rev. D60 (1999) 013003, arXiv:hep-ph/9901350.

[22-114]

Solar and atmospheric neutrino oscillations from bilinear R-parity violation, Kaplan, D. Elazzar, Nelson, Ann E., JHEP 01 (2000) 033, arXiv:hep-ph/9901254.

[22-115]

Atmospheric neutrino oscillations in three-flavor neutrinos. II, Sakai, Toyokazu, Teshima, Tadayuki, Prog. Theor. Phys. 102 (1999) 629-644, arXiv:hep-ph/9901219.

[22-116]

LSND, solar and atmospheric neutrino oscillation experiments, and R-parity violating supersymmetry, Adhikari, Rathin, Omanovic, Gordana, Phys. Rev. D59 (1999) 073003.

[22-117]

Bounds and implications of neutrino magnetic moments from atmospheric neutrino data, Kang, Sin Kyu, Kim, Jihn E., Lee, Jae Sik, Phys. Rev. D60 (1999) 033008, arXiv:hep-ph/9812531.

[22-118]

Neutrino mixing and masses from long baseline and atmospheric oscillation experiments, Barenboim, Gabriela, Scheck, Florian, Phys. Lett. B450 (1999) 189-195, arXiv:hep-ph/9812351.

[22-119]

Global three-neutrino vacuum oscillation fits to the solar and atmospheric anomalies, Barger, V. D., Whisnant, K., Phys. Rev. D59 (1999) 093007, arXiv:hep-ph/9812273.

[22-120]

Atmospheric and solar neutrino oscillations in nuMSSM and beyond, Shafi, Qaisar, Tavartkiladze, Zurab, Phys. Lett. B448 (1999) 46-56, arXiv:hep-ph/9811463.

[22-121]

Atmospheric and solar neutrino masses from horizontal U(1) symmetry, Choi, Kiwoon, Hwang, Kyuwan, Chun, Eung Jin, Phys. Rev. D60 (1999) 031301, arXiv:hep-ph/9811363.

[22-122]

Minimal see-saw model for atmospheric and solar neutrino oscillations, Ma, Ernest, Roy, D. P., Phys. Rev. D59 (1999) 097702, arXiv:hep-ph/9811266.

[22-123]

Solar and atmospheric neutrino oscillations and lepton flavor violation in supersymmetric models with the right- handed neutrinos, Hisano, J., Nomura, Daisuke, Phys. Rev. D59 (1999) 116005, arXiv:hep-ph/9810479.

[22-124]

Tau appearance in atmospheric neutrino interactions, Hall, Lawrence J., Murayama, Hitoshi, Phys. Lett. B463 (1999) 241-247, arXiv:hep-ph/9810468.

[22-125]

A see-saw model for atmospheric and solar neutrino oscillations, Ma, Ernest, Roy, D. P., Sarkar, Utpal, Phys. Lett. B444 (1998) 391-396, arXiv:hep-ph/9810309.

[22-126]

Neutrino decay as an explanation of atmospheric neutrino observations, Barger, V. D., Learned, J. G., Pakvasa, S., Weiler, Thomas J., Phys. Rev. Lett. 82 (1999) 2640-2643, arXiv:astro-ph/9810121.

[22-127]

Atmospheric neutrino observations and flavor changing interactions, Gonzalez-Garcia, M. C. et al., Phys. Rev. Lett. 82 (1999) 3202-3205, arXiv:hep-ph/9809531.

[22-128]

What the atmospheric neutrino anomaly is not, LoSecco, J. M., arXiv:hep-ph/9809499, 1998.

[22-129]

Comment on the possible electron-neutrino excess in the Super-Kamiokande atmospheric neutrino experiment, Kim, C. W., Lee, U. W., Phys. Lett. B444 (1998) 204-207, arXiv:hep-ph/9809491.

[22-130]

Atmospheric neutrino tests of neutrino oscillation mechanisms, Foot, R., Leung, C. N., Yasuda, O., Phys. Lett. B443 (1998) 185-190, arXiv:hep-ph/9809458.

[22-131]

Implications of the -> solution to the atmospheric neutrino anomaly for early universe cosmology, Foot, R., Astropart. Phys. 10 (1999) 253-273, arXiv:hep-ph/9809315.

[22-132]

Do the Super-Kamiokande atmospheric neutrino results explain electric charge quantisation?, Foot, R., Volkas, R. R., Phys. Rev. D59 (1999) 097301, arXiv:hep-ph/9808388.

[22-133]

Textures for atmospheric and solar neutrino oscillations, Barbieri, Riccardo, Hall, Lawrence J., Strumia, A., Phys. Lett. B445 (1999) 407-411, arXiv:hep-ph/9808333.

[22-134]

Atmospheric neutrinos at Super-Kamiokande and parametric resonance in neutrino oscillations, Akhmedov, E. K., Dighe, A., Lipari, P., Smirnov, A. Y., Nucl. Phys. B542 (1999) 3-30, arXiv:hep-ph/9808270.

[22-135]

Super-Kamiokande atmospheric neutrino data, zenith distributions, and three-flavor oscillations, Fogli, Gian Luigi, Lisi, E., Marrone, A., Scioscia, G., Phys. Rev. D59 (1999) 033001, arXiv:hep-ph/9808205.

[22-136]

Atmospheric deficit from decoherence, Grossman, Y., Worah, M. P., arXiv:hep-ph/9807511, 1998.

[22-137]

Dynamical neutrino mass matrix: Large (small) mixing solution to atmospheric (solar) neutrino oscillations, Ma, Ernest, Phys. Lett. B442 (1998) 238-242, arXiv:hep-ph/9807386.

[22-138]

Problems with atmospheric neutrino oscillations, LoSecco, J. M., arXiv:hep-ph/9807359, 1998.

[22-139]

Generalized neutrino mixing from the atmospheric anomaly, Barger, V. D., Weiler, Thomas J., Whisnant, K., Phys. Lett. B440 (1998) 1-6, arXiv:hep-ph/9807319.

[22-140]

Active-active and active-sterile neutrino oscillation solutions to the atmospheric neutrino anomaly, Gonzalez-Garcia, M. C., Nunokawa, H., Peres, O. L. G., Valle, J. W. F., Nucl. Phys. B543 (1999) 3-19, arXiv:hep-ph/9807305.

[22-141]

Atmospheric neutrino anomaly and supersymmetric inflation, Lazarides, G., Vlachos, N. D., Phys. Lett. B441 (1998) 46-51, arXiv:hep-ph/9807253.

[22-142]

Interpreting the atmospheric neutrino anomaly, Thun, R. P., McKee, S., Phys. Lett. B439 (1998) 123-129, arXiv:hep-ph/9806534.

[22-143]

Measuring the to ratio in a high statistics atmospheric neutrino experiment, LoSecco, J. M., Phys. Rev. D59 (1999) 117302, arXiv:hep-ph/9806318.

[22-144]

Atmospheric neutrino oscillations in three-flavor neutrinos, Teshima, T., Sakai, T., Prog. Theor. Phys. 101 (1999) 147, arXiv:hep-ph/9805386.

[22-145]

Parametric resonance of neutrino oscillations and passage of solar and atmospheric neutrinos through the earth, Akhmedov, E. K., Nucl. Phys. B538 (1999) 25-51, arXiv:hep-ph/9805272.

[22-146]

Three flavor neutrino oscillation analysis of the Super-Kamiokande atmospheric neutrino data, Yasuda, Osamu, Phys. Rev. D58 (1998) 091301, arXiv:hep-ph/9804400.

[22-147]

Comparison of <-> and <-> oscillations as solutions of the atmospheric neutrino problem, Lipari, Paolo, Lusignoli, Maurizio, Phys. Rev. D58 (1998) 073005, arXiv:hep-ph/9803440.

[22-148]

Parametric resonance in oscillations of atmospheric neutrinos?, Liu, Q. Y., Mikheyev, S. P., Smirnov, A. Yu., Phys. Lett. B440 (1998) 319-326, arXiv:hep-ph/9803415.

[22-149]

A minimality condition and atmospheric neutrino oscillations, Albright, Carl H., Babu, K. S., Barr, Stephen M., Phys. Rev. Lett. 81 (1998) 1167-1170, arXiv:hep-ph/9802314.

[22-150]

Confronting solutions to the atmospheric neutrino anomaly involving large angle -> oscillations with Super-Kamiokande and CHOOZ, Foot, R., Volkas, R. R., Yasuda, O., Phys. Lett. B433 (1998) 82-87, arXiv:hep-ph/9802287.

[22-151]

Comparing and contrasting the -> and -> solutions to the atmospheric neutrino problem with Super-Kamiokande data, Foot, R., Volkas, R. R., Yasuda, O., Phys. Rev. D58 (1998) 013006, arXiv:hep-ph/9801431.

[22-152]

Examination of neutrino oscillations using high-energy atmospheric neutrino data from Kamiokande, Oyama, Yuichi, Phys. Rev. D57 (1998) 6594-6598.

[22-153]

Mass matrix ansatz for degenerate neutrinos consistent with solar and atmospheric neutrino data, Kang, K., Kang, S. K., Kim, J. E., Ko, P., Phys. Lett. B442 (1998) 249-254.

[22-154]

Implications of CHOOZ results for the decoupling of solar and atmospheric neutrino oscillations, Bilenky, Samoil M., Giunti, C., Phys. Lett. B444 (1998) 379-386.

[22-155]

Neutrino mass spectrum with -> oscillations of atmospheric neutrinos, Liu, Q. Y., Smirnov, A. Yu., Nucl. Phys. B524 (1998) 505-523, arXiv:hep-ph/9712493.

[22-156]

A supersymmetric resolution of solar and atmospheric neutrino puzzles, Drees, Manuel, Pakvasa, S., Tata, X., ter Veldhuis, T., Phys. Rev. D57 (1998) 5335-5339, arXiv:hep-ph/9712392.

[22-157]

Zenith distribution of atmospheric neutrino events and electron neutrino mixing, Fogli, Gian Luigi, Lisi, E., Marrone, A., Montanino, D., Phys. Lett. B425 (1998) 341-344, arXiv:hep-ph/9711421.

[22-158]

Atmospheric neutrino oscillation and large lepton flavour violation in the SUSY SU(5) GUT, Hisano, J., Nomura, Daisuke, Yanagida, T., Phys. Lett. B437 (1998) 351-358, arXiv:hep-ph/9711348.

[22-159]

Neutral-to-charged current events ratio in atmospheric neutrinos and neutrino oscillations, Vissani, Francesco, Smirnov, Alexei Yu., Phys. Lett. B432 (1998) 376-382, arXiv:hep-ph/9710565.

[22-160]

Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios, Foot, R., Volkas, R. R., Yasuda, O., Phys. Lett. B421 (1998) 245-249, arXiv:hep-ph/9710403.

[22-161]

Unified explanation of the solar and atmospheric neutrino puzzles in a minimal supersymmetric SO(10) model, Brahmachari, B., Mohapatra, R. N., Phys. Rev. D58 (1998) 015001, arXiv:hep-ph/9710371.

[22-162]

Testing maximal electron and muon neutrino oscillations with sub-GeV Super-Kamiokande atmospheric neutrino data, Foot, R., Volkas, R. R., Yasuda, O., Phys. Rev. D57 (1998) 1345-1349, arXiv:hep-ph/9709483.

[22-163]

Atmospheric neutrino oscillations with three neutrinos and a mass hierarchy, Giunti, C., Kim, C. W., Monteno, M., Nucl. Phys. B521 (1998) 3-36, arXiv:hep-ph/9709439.

[22-164]

Up-down asymmetry: A diagnostic for neutrino oscillations, Flanagan, John W., Learned, John G., Pakvasa, Sandip, Phys. Rev. D57 (1998) 2649-2652, arXiv:hep-ph/9709438.

[22-165]

Atmospheric neutrino oscillation and a phenomenological lepton mass matrix, Fukugita, M., Tanimoto, M., Yanagida, T., Phys. Rev. D57 (1998) 4429-4432, arXiv:hep-ph/9709388.

[22-166]

Bounds on dark matter from the *atmospheric neutrino anomaly*, LoSecco, J. M., Phys. Rev. D56 (1997) 4416-4418, arXiv:hep-ph/9706368.

[22-167]

Effects for atmospheric neutrino experiments from electron neutrino oscillations, Bunn, J., Foot, R., Volkas, R. R., Phys. Lett. B413 (1997) 109-113, arXiv:hep-ph/9702429.

[22-168]

Three-flavor atmospheric neutrino anomaly, Fogli, Gian Luigi, Lisi, E., Montanino, D., Scioscia, G., Phys. Rev. D55 (1997) 4385-4404, arXiv:hep-ph/9607251.

[22-169]

Accelerator, reactor, solar and atmospheric neutrino oscillation: Beyond three generations, Goswami, Srubabati, Phys. Rev. D55 (1997) 2931-2949, arXiv:hep-ph/9507212.

[22-170]

Accelerator, reactor and atmospheric neutrino data: A Three flavor oscillation analysis, Goswami, Srubabati, Kar, Kamales, Raychaudhuri, Amitava, Int. J. Mod. Phys. A12 (1997) 781-800, arXiv:hep-ph/9505395.

[22-171]

Neutrino physics and the mirror world: How exact parity symmetry explains the solar neutrino deficit, the atmospheric neutrino anomaly and the LSND experiment, Foot, R., Volkas, R. R., Phys. Rev. D52 (1995) 6595-6606, arXiv:hep-ph/9505359.

[22-172]

Atmospheric neutrino oscillations among three neutrino flavors and long baseline experiments, Bilenky, Samoil M., Giunti, C., Kim, C. W., Astropart. Phys. 4 (1996) 241-251, arXiv:hep-ph/9505301.

[22-173]

Solar and atmospheric neutrino oscillations with three flavors, Narayan, Mohan, Murthy, M. V. N., Rajasekaran, G., Uma Sankar, S., Phys. Rev. D53 (1996) 2809-2819, arXiv:hep-ph/9505281.

[22-174]

Comment on the Kamiokande atmospheric neutrino deficit, Saltzberg, David, Phys. Lett. B355 (1995) 499-500, arXiv:hep-ph/9504343.

[22-175]

On the atmospheric neutrino anomaly and its statistical significance, Fogli, Gian Luigi, Lisi, E., Phys. Rev. D52 (1995) 2775-2782, arXiv:hep-ph/9504287.

[22-176]

Possible implications of the atmospheric, the Bugey, and the Los Alamos neutrino experiments, Minakata, Hisakazu, Phys. Rev. D52 (1995) 6630-6633, arXiv:hep-ph/9503417.

[22-177]

Possible revelation of seesaw mass pattern in solar and atmospheric neutrino data, Ma, Ernest, Pantaleone, J., Phys. Rev. D52 (1995) 3763-3767, arXiv:hep-ph/9503312.

[22-178]

Threefold maximal lepton mixing and the solar and atmospheric neutrino deficits, Harrison, P. F., Perkins, D. H., Scott, W. G., Phys. Lett. B349 (1995) 137-144.

[22-179]

The Neutrino cross-section and upward going muons, Lipari, Paolo, Lusignoli, Maurizio, Sartogo, Francesca, Phys. Rev. Lett. 74 (1995) 4384-4387, arXiv:hep-ph/9411341.

[22-180]

Simple radiative neutrino mass matrix for solar and atmospheric oscillations, Ma, Ernest, Phys. Rev. D51 (1995) 3145-3148, arXiv:hep-ph/9411315.

[22-181]

Atmospheric neutrino problem in maximally mixed three generations of neutrinos, Giunti, C., Kim, C. W., Kim, J. D., Phys. Lett. B352 (1995) 357-364, arXiv:hep-ph/9411219.

[22-182]

Reconciling cold dark matter with COBE / IRAS plus solar and atmospheric neutrino data, Joshipura, Anjan S., Valle, J. W. F., Nucl. Phys. B440 (1995) 647-660, arXiv:hep-ph/9410259.

[22-183]

Accommodating solar and atmospheric neutrino deficits, hot dark matter, and a double beta decay signal, Caldwell, David O., Mohapatra, Rabindra N., Phys. Rev. D50 (1994) 3477-3483, arXiv:hep-ph/9402231.

[22-184]

A comprehensive analysis of solar, atmospheric, accelerator and reactor neutrino experiments in a hierarchical three generation scheme, Fogli, Gian Luigi, Lisi, E., Montanino, D., Phys. Rev. D49 (1994) 3626-3642.

[22-185]

Constraints on three neutrino mixing from atmospheric and reactor data, Pantaleone, J., Phys. Rev. D49 (1994) 2152-2155, arXiv:hep-ph/9310363.

[22-186]

Common origin for the solar and atmospheric neutrino deficits, Joshipura, Anjan S., Krastev, P. I., Phys. Rev. D50 (1994) 3484-3490, arXiv:hep-ph/9308348.

[22-187]

A Common explanation for the atmospheric, solar neutrino and double beta decay anomalies, Burgess, C. P., Hernandez, Oscar, Phys. Rev. D48 (1993) 4326-4336, arXiv:hep-ph/9306252.

[22-188]

Quasielastic neutrino scattering from oxygen and the atmospheric neutrino problem, Engel, J., Kolbe, E., Langanke, K., Vogel, P., Phys. Rev. D48 (1993) 3048-3054, arXiv:nucl-th/9304017.

[22-189]

Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter, Caldwell, David O., Mohapatra, Rabindra N., Phys. Rev. D48 (1993) 3259-3263.

[22-190]

The Atmospheric neutrino problem: A Critique, Perkins, D. H., Nucl. Phys. B399 (1993) 3-16.

[22-191]

Neutrino cross-sections and the small atmospheric muon- neutrino / electron-neutrino ratio, Mann, A. K., Phys. Rev. D48 (1993) 422-424.

[22-192]

Low-energy atmospheric neutrino data interpretations, Volkova, L. V., Phys. Lett. B316 (1993) 178-180.

[22-193]

Unified treatment of solar and atmospheric neutrino oscillations, Babu, K. S., Shafi, Q., Nucl. Phys. Proc. Suppl. 31 (1993) 242-244.

[22-194]

Atmospheric neutrino data and neutrino oscillations, Frati, W., Gaisser, T. K., Mann, A. K., Stanev, Todor, Phys. Rev. D48 (1993) 1140-1149.

[22-195]

A Single solution to the atmospheric and solar neutrino anomalies, Acker, A., Learned, J. G., Pakvasa, S., Weiler, T. J., Phys. Lett. B298 (1993) 149-153.

[22-196]

Matter effects in atmospheric neutrino oscillations, Akhmedov, E., Lipari, P., Lusignoli, M., Phys. Lett. B300 (1993) 128-136, arXiv:hep-ph/9211320.

[22-197]

Simultaneous solutions to the solar and atmospheric neutrino problems via Fritzsch type lepton mass matrices, Davies, A. J., He, Xiao-Gang, Phys. Rev. D46 (1992) 3208-3210.

[22-198]

The Atmospheric flux muon-neutrino / electron-neutrino anomaly as manifestation of proton decay p e+ neutrino neutrino, Mann, W. A., Kafka, T., Leeson, W., Phys. Lett. B291 (1992) 200-205.

[22-199]

Atmospheric neutrino fluxes and sterile-neutrinos, Enqvist, K., Kainulainen, K., Thomson, Mark J., Phys. Lett. B288 (1992) 145-147.

[22-200]

A Neutrino decay model, solar anti-neutrinos and atmospheric neutrinos, Acker, A., Joshipura, A., Pakvasa, S., Phys. Lett. B285 (1992) 371-375.

[22-201]

Determination of pion intranuclear rescattering rates in muon-neutrino Ne versus muon-neutrino D interactions for the atmospheric neutrino flux, Merenyi, R. et al., Phys. Rev. D45 (1992) 743-751.

[22-202]

Survey of atmospheric neutrino data and implications for neutrino mass and mixing, Beier, E. W. et al., Phys. Lett. B283 (1992) 446-453.

[22-203]

Unified treatment of solar and atmospheric neutrino oscillations, Babu, K. S., Shafi, Q., Phys. Lett. B294 (1992) 235-242.

[22-204]

Neutrino oscillations and the atmospheric neutrino fluxes, Dass, G. V., Sarma, K. V. L., Phys. Rev. D30 (1984) 80.

[22-205]

Neutrino oscillation search with cosmic ray neutrinos, Ayres, D. S. et al., Phys. Rev. D29 (1984) 902.

[22-206]

Atmospheric neutrinos, astrophysical neutrinos and proton decay experiments, Dar, A., Phys. Rev. Lett. 51 (1983) 227.

[22-207]

Time averaged neutrino oscillations, Frampton, P. H., Glashow, S. L., Phys. Rev. D25 (1982) 1982.

[22-208]

Possible indications of neutrino oscillations, Barger, Vernon D., Whisnant, K., Cline, D., Phillips, R. J. N., Phys. Lett. B93 (1980) 194.

[22-209]

Three neutrino oscillations and present experimental data, Barger, Vernon D., Whisnant, K., Phillips, R. J. N., Phys. Rev. D22 (1980) 1636.

[22-210]

Muons produced by atmospheric neutrinos: Analysis, Chen, H. H., Kropp, W. R., Sobel, H. W., Reines, F., Phys. Rev. D4 (1971) 99-121.

[22-211]

On the analysis of neutrino experiments in cosmic rays, Volkova, L. V., Zatsepin, G. T., Sov. J. Nucl. Phys. 14 (1971) 117. Yad. Fiz. 14 (1971) 211-220.

[23-1]

Atmospheric neutrinos in the context of muon and neutrino radiography, Thomas K. Gaisser, Earth Planets Space 62 (2010) 195-199, arXiv:0901.2386. International Workshop on High Energy Earth Science: Muon and Neutrino Radiography.

[23-2]

Three-flavour neutrino oscillation update and comments on possible hints for a non-zero , Michele Maltoni, Thomas Schwetz, PoS IDM2008 (2008) 072, arXiv:0812.3161. IDM2008, Aug. 18-22, 2008, Stockholm, Sweden.

[23-3]

Physics Potential of Future Atmospheric Neutrino Searches, Schwetz, Thomas, Nucl. Phys. Proc. Suppl. 188 (2009) 158-163, arXiv:0812.2392. NOW2008, Conca Specchiulla, Otranto, Italy, September 6-13, 2008.

[23-4]

Prospects and synergies between future atmospheric and long-baseline experiments, Michele Maltoni, PoS NUFACT08 (2008) 037, arXiv:0810.1440. 10th International Workshop on Neutrino Factories, Super beams and Beta beams (NuFact'08), Valencia, Spain, June 30 - July 5, 2008.

[23-5]

Modeling Atmospheric Neutrino Interactions: Duality Constrained Parameterization of Vector and Axial Nucleon Form Factors, Bodek, A., Avvakumov, S., Bradford, R., Budd, H., arXiv:0708.1827, 2007. 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007.

[23-6]

Potentialities of atmospheric neutrinos, Maltoni, Michele, arXiv:0707.1218, 2007. Rencontres de Moriond EW 2007, La Thuile, Italy, March 10-17, 2007.

[23-7]

Non-standard Neutrino Oscillations at Icecube, M.C. Gonzalez-Garcia, arXiv:hep-ph/0612227, 2006. Workshop on Exotic Physics with Neutrino Telescopes, Uppsala, Sweden, September 20-22, 2006.

[23-8]

Can we learn something more on oscillations from atmospheric neutrinos?, Thomas Schwetz, arXiv:hep-ph/0610053, 2006. ICHEP06, July 26-August 2, 2006, Moscow.

[23-9]

Extraction of the atmospheric neutrino fluxes from experimental event rate data, M. C. Gonzalez-Garcia, M. Maltoni, J. Rojo, J. Phys. A40 (2007) 7093-7098, arXiv:hep-ph/0608319. 2nd International Conference on Quantum Theories and Renormalization Group in Gravity and Cosmology, Barcelona, July 2006.

[23-10]

Determination of the atmospheric neutrino fluxes from experimental data, M.C. Gonzalez-Garcia, Michele Maltoni, Joan Rojo, Astrophys. Space Sci. 309 (2007) 447-451, arXiv:astro-ph/0608107. Multi-Messenger Approach to High-Energy Gamma-Ray Sources Conference, Barcelona July 2006.

[23-11]

Atmospheric neutrinos in a Large Liquid Argon detector, G. Battistoni et al., arXiv:hep-ph/0604182, 2006. "Cryogenic Liquid Detectors for Future Particle Physics", LNGS (Italy) March 13th-14th, 2006.

[23-12]

Do Neutrinos Violate CP?, Hisakazu Minakata, arXiv:hep-ph/0604088, 2006. 3rd Interntional Workshop Neutrino Oscillations in Venice (NO-VE 2006): 50 Years after the Neutrino Experimental Discovery, Venice, Italy, 7-10 Feb 2006.

[23-13]

Measuring the deviation from maximal mixing of atmospheric muon neutrinos at INO, Probir Roy, AIP Conf. Proc. 842 (2006) 883-885, arXiv:hep-ph/0601011. PANIC 05, Santa Fe, Oct. 24 - 28, 2005.

[23-14]

The measurement of theta(13) and delta: The role of the uncertainties on the solar and atmospheric parameters, Meloni, D., Nucl. Phys. Proc. Suppl. 155 (2006) 178, arXiv:hep-ph/0509370. NUFACT'05, 21-26 June 2005, Frascati.

[23-15]

Search for exotic contributions to atmospheric neutrino oscillations, Battistoni, G. et al., Phys. Atom. Nucl. 69 (2006) 1842-1846, arXiv:hep-ex/0508041. 29th I.C.R.C., Pune, India (2005).

[23-16]

Issues on neutrino-nucleus reactions in the quasi-free delta production region, Ryoichi Seki, Hiroki Nakamura, arXiv:hep-ph/0504162, 2005. Sub-Dominant Oscillation Effects in Atmospheric Neutrino Experiments.

[23-17]

Global Analysis of Neutrino Oscillation, Srubabati Goswami, Abhijit Bandyopadhyay, Sandhya Choubey, Nucl. Phys. Proc. Suppl. 143 (2005) 121, arXiv:hep-ph/0409224. 21st International Conference on Neutrino Physics and Astrophysics (Neutrino 2004), Paris, France, 14-19 June 2004.

[23-18]

On the Atmospheric Neutrino Oscillations, theta13 and Neutrino Mass Hierarchy, S.T. Petcov, Sergio Palomares-Ruiz, arXiv:hep-ph/0406106, 2004. NOON2004, February 11 - 15, 2004, Tokyo, Japan.

[23-19]

Atmospheric and galactic tau neutrinos, H. Athar, Mod. Phys. Lett. A19 (2004) 1171, arXiv:hep-ph/0401242. CosPA 2003, 13-15 Nov, 2003, Taipei, Taiwan.

[23-20]

Neutrino Oscillations: A Global Analysis, G.L. Fogli et al., eConf C030626 (2003) THAT05, arXiv:hep-ph/0310012. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.

[23-21]

Inconsistencies in Interpreting the Atmospheric Neutrino Anomaly, John M. LoSecco, Pramana 62 (2004) 635, arXiv:hep-ph/0305022. PASCOS-2003.

[23-22]

Neutrino Oscillations: Global Fits, Schwetz, T., 2003. MPI-TUM Ringberg Workshop on Neutrinos and Astroparticle Physics, July 24-25, 2003, Ringberg Castle, Tegernsee, Germany. http://www1.physik.tu-muenchen.de/~sfb375/Server/ringberg_2003/schwetz.pdf.

[23-23]

Standard and Non-Standard Physics in Neutrino Oscillations, Maltoni, M., Nucl. Phys. Proc. Suppl. 114 (2003) 191-196, arXiv:hep-ph/0210111. XXX International Meeting on Fundamental Physics (Jaca, Spain, 28/01-1/02/2002).

[23-24]

Standard and non-standard neutrino properties, Valle, J. W. F., Nucl. Phys. Proc. Suppl. 118 (2003) 255, arXiv:hep-ph/0209047. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/valle.

[23-25]

LMA parameters and non-zero U(e3) effects on atmospheric nu data?, Peres, O. L. G., Smirnov, A. Yu., Nucl. Phys. Proc. Suppl. 110 (2002) 355-357, arXiv:hep-ph/0201069. TAUP 2001: Topics in Astroparticle and Underground Physics, Assergi, Italy, 8-12 Sep 2001.

[23-26]

From Atmospheric Neutrinos to Accelerator Neutrinos, Lipari, P., 2002. Workshop Neutrini al Gran Sasso - 25 March 2002, Padova, Italy. http://www.pd.infn.it/~laveder/cngspd/trasparenze/Lipari.pdf.

[23-27]

(Mis)understanding the atmospheric neutrino anomaly, LoSecco, J. M., Nucl. Phys. Proc. Suppl. 98 (2001) 182-188, arXiv:hep-ph/0011117.

[23-28]

Statistical tests for zenith angle dependences of up-going mu-like neutrino events for multi-GeV region, Kitamura, T. et al., Nucl. Phys. Proc. Suppl. 75A (1999) 403-405.

[24-1]

High-energy Atmospheric Muon Flux Expected at India-Based Neutrino Obs ervatory, Sukanta Panda, Sergei I. Sinegovsky, Int. J. Mod. Phys. A23 (2008) 2933-2942, arXiv:0710.3125.

[24-2]

Calculation of the atmospheric muon flux motivated by the ATIC-2 experiment, A.A. Kochanov, A.D. Panov, T.S. Sinegovskaya, S.I. Sinegovsky, arXiv:0706.4389, 2007.

[24-3]

On the deficit of calculated muon flux at sea level for energies GeV, Lagutin, A. A., Tyumentsev, A. G., Yushkov, A. V., Int. J. Mod. Phys. A20 (2005) 6959, arXiv:astro-ph/0503092.

[24-4]

The influence of the geomagnetic field and of the uncertainties in the primary spectrum on the development of the muon flux in the atmosphere, P. Hansen, T.K. Gaisser, T. Stanev, S.J. Sciutto, Phys. Rev. D71 (2005) 083012, arXiv:astro-ph/0411634.

[24-5]

Fluxes of atmospheric muons underwater depending on the small-x gluon density, A. Misaki, T. S. Sinegovskaya, S. I. Sinegovsky, N. Takahashi, J. Phys. G 29 (2003) 387, arXiv:hep-ph/0302183.

[25-1]

Calculation of muon fluxes at the small atmospheric depths, Abe, Koh et al., arXiv:astro-ph/0312632, 2003. 28th International Cosmic Ray Conferences (ICRC 2003), Tsukuba, Japan, 31 Jul - 7 Aug 2003.

[26-1]

Atmospheric Neutrino Mixing and b-s Transitions: Testing Lopsided SO(10) Flavor Structure in B physics, Xiangdong Ji, Yingchuan Li, Yue Zhang, Phys. Rev. D75 (2007) 055016, arXiv:hep-ph/0612114.

[27-1]

Comprehensive Analysis of Neutrinos in SK part 3 - L/E Analysis for Single Ring Muon Events II -, Konishi, E. et al., arXiv:0808.3508, 2008.

[27-2]

Comprehensive Analysis of Neutrinos in SK part II - L/E Analysis for Single Ring Muon Events I -, Konishi, E. et al., arXiv:0808.3313, 2008.

[27-3]

On the Capability Of Super-Kamiokande Detector To Define the Primary Parameters Of Muon And Electron Events, V.I. Galkin, A.M. Anokhina, E. Konishi, A. Misaki, arXiv:0808.0824, 2008.

[27-4]

Comprehensive Analysis of Neutrinos in SK part I -Directions of the Incident Neutrinos and the Produced Leptons-, E. Konishi et al., arXiv:0808.0664, 2008.

[27-5]

The numerical computer experiment for the neutrino events with the SK neutrino oscillation parameters occurring outside the Superkamiokande detector, Takahashi, N., Konishi, E., Misaki, A., arXiv:0802.2422, 2008.

[27-6]

The Reliability on the Direction of the Incident Neutrino for the Fully Contained Events and Partially Contained Events due to QEL in the Super-Kamiokande, E. Konishi et al., arXiv:0704.0190, 2007.

[27-7]

Can One Extract the Neutrino Oscillation Signature from the SuperKamiokande Experiment? An Analysis of Neutrino Events Occurring outside the Detector, Takahashi, N., Misaki, A., arXiv:hep-ex/0505020, 2005.

[27-8]

A discrimination procedure between muon and electron in Superkamiokande experiment based on the angular distribution function method, Galkin, V. I., Anokhina, A. M., Konishi, E., Misaki, A., arXiv:hep-ex/0501058, 2005.

[27-9]

A theory of pattern recognition for the discrimination between muon and electron in the Super-Kamiokande, Galkin, V. I., Anokhina, A. M., Konishi, E., Misaki, A., arXiv:hep-ex/0412059, 2004.

[27-10]

Have Superkamiokande really measured the direction of the atmospheric neutrinos which produce fully contained events and partially contained events?, Konishi, E., Minorikawa, Y., Galkin, V. I., Ishiwata, M., Misaki, A., arXiv:hep-ex/0407015, 2004.

[27-11]

The Zenith Angle Distribution of Fully Contained Events in SuperKamiokande and the Impact of Quasi Elastic Scattering on their Direction, Konishi, Eiichi, Minorikawa, Y., Galkin, V. I., Ishiwata, M., Misaki, A., arXiv:astro-ph/0406497, 2004.