Atmospheric Neutrinos

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References

1 - Books

[1-1]
Introduction to the physics of massive and mixed neutrinos, Samoil Bilenky, Springer-Verlag Berlin Heidelberg, 2010. Lecture Notes in Physics, Volume 817; ISBN 978-3-642-14042-6. http://www.springer.com/physics/book/978-3-642-14042-6.
[Bilenky:2010zza]
[1-2]
Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. ISBN 978-0-19-850871-7. http://www.oup.com/uk/catalogue/?ci=9780198508717.
[Giunti:2007ry]
[1-3]
Physics and Astrophysics Of Neutrinos, (ed.) Fukugita, M., (ed.) Suzuki, A., Springer, 1994.
[Fukugita:1994wx]
[1-4]
Cosmic Rays and Particle Physics, T. K. Gaisser, Cambridge University Press, 1990.
[Gaisser:1990vg]

2 - Reviews - Experiment

[2-1]
History of 'Anomalous' Atmospheric Neutrino Events: A First Person Account, John M. LoSecco, Phys.Perspect. 18 (2016) 209-241, arXiv:1606.00665.
[LoSecco:2016eom]
[2-2]
Measurement of atmospheric neutrino oscillations with very large volume neutrino telescopes, J. P. Yanez, A. Kouchner, Adv. High Energy Phys. 2015 (2015) 271968, arXiv:1509.08404.
[Yanez:2015uta]
[2-3]
Nobel Lecture: Discovery of atmospheric neutrino oscillations, Takaaki Kajita, Rev. Mod. Phys. 88 (2016) 030501.
[Kajita:2016cak]
[2-4]
Discovery of atmospheric neutrino oscillations, Takaaki Kajita, Annalen Phys. 528 (2016) 459-468. Nobel Lecture.
[Kajita:2016tyc]
[2-5]
MINOS neutrino oscillation results, Alec Habig, Mod. Phys. Lett. A25 (2010) 1219-1231, arXiv:1004.2647.
[Habig:2010vw]
[2-6]
Discovery of neutrino oscillations, T. Kajita, Rept. Prog. Phys. 69 (2006) 1607-1635.
[Kajita:2006cy]
[2-7]
Atmospheric neutrinos, T. Kajita, New J. Phys. 6 (2004) 194. http://www.iop.org/EJ/abstract/1367-2630/6/1/194.
[Kajita:2004ga]
[2-8]
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 $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by different atmospheric neutrino experiments. [M.L.].
[McDonald:2003xn]
[2-9]
Oscillations of atmospheric neutrinos, C. K. Jung, C. McGrew, T. Kajita, T. Mann, 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.
[Jung:2001dh]
[2-10]
Observation of atmospheric neutrinos, T. Kajita, Y. Totsuka, Rev. Mod. Phys. 73 (2001) 85-118.
[Kajita:2000mr]
[2-11]
The atmospheric neutrino anomaly: Muon neutrino disappearance, J. G. Learned (SuperKamioKande), arXiv:hep-ex/0007056, 2000.
[Learned:2000qq]
[2-12]
Neutrino astronomy, Yoji Totsuka, Rept. Prog. Phys. 55 (1992) 377-430.
[Totsuka:1992dm]
[2-13]
Observational neutrino astrophysics, M. Koshiba, Phys. Rep. 220 (1992) 229-381.
[Koshiba:1992yb]

3 - Reviews - Experiment - Conference Proceedings

[3-1]
Atmospheric Neutrino Status, E. O'Sullivan, arXiv:1605.00612, 2016. NuPhys2015 (London, 16-18 December 2015).
[OSullivan:2016fue]
[3-2]
Atmospheric muons: experimental aspects, Stefano Cecchini, Maurizio Spurio, arXiv:1208.1171, 2012. Muon and Neutrino Radiography 2012 (MNR 2012), Clermont Ferrand (France), April 2012.
[Cecchini:2012uj]
[3-3]
Muon Neutrino Disappearance and Tau Neutrino Appearance, M. C. Sanchez, arXiv:1112.0618, 2011. XXXI Conference on Physics in Collision, Vancouver, Canada, August 28 to September 1, 2011.
[Sanchez:2011np]
[3-4]
Atmospheric $\nu$ and Long Baseline $\nu$ experiments II, Giorgio Giacomelli, arXiv:1102.0650, 2011. Carpatian Summer School of Physics 2010, Sinaia, Romania.
[Giacomelli:2011ut]
[3-5]
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.
[Giacomelli:2007bd]
[3-6]
Atmospheric neutrino oscillations, G. Giacomelli, M. Giorgini (MACRO), arXiv:hep-ex/0504002, 2005. 7th School on Non-Accelerator Astroparticle Physics, Trieste, Italy, 2004.
[Giacomelli:2005br]
[3-7]
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.
[Heeger:2004mp]
[3-8]
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.
[Wang:2004wu]
[3-9]
Neutrinos underground, H. Sobel, 2004. AAAS meeting 2004, 17-21 Feb. 2004, Washington, DC, US. http://harv11.fnal.gov/~smaria/aaas04/hank_aaas04.pdf.
[Sobel:AAAS2004]
[3-10]
Neutrino Physics: Experimental Status, T. Kajita, 2003. 19th International Workshop on Weak Interactions and Neutrinos, WIN2003, October 6-11, Lake Geneva, Wisconsin, USA. http://conferences.fnal.gov/win03/Talks/Takaaki%20Kajita.pdf.
Comment: The slide n. 19 shows the $ 90 \% $ C.L. allowed contours for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by different atmospheric neutrino experiments. The figure in slide n.24 shows the $ 90 \% $ C.L. allowed contour for $\nu_\mu \rightarrow \nu_\tau$ oscillations obtained by Super-Kamiokande. [M.L.].
[Kajita:WIN2003]
[3-11]
Results and status of current accelerator neutrino experiments, K. Nishikawa, 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 $ 90 \% C.L. $ sensitivity on $\theta_{13}$ of different projects. [M.L.].
[Nishikawa:LP2003]
[3-12]
Atmospheric Neutrinos in 2002, Edward T. Kearns, Frascati Phys. Ser. 28 (2002) 413-426, arXiv:hep-ex/0210019. Heavy Quarks and Leptons 2002, Vietri sul Mare, Italy, May 27-June 1, 2002. http://hep.bu.edu/~kearns/pub/kearns-atmnu2002-hql.pdf.
From the article: ... recent developments in neutrino flux calculation is a key input to more detailed understanding of the data.... in neutrino oscillation studies the flux normalization is allowed to float as a free parameter.
Comment: In Ref.[Fukuda and others, Phys. Rev. Lett.81, 1562 (1998)] the overall normalization was estimated to have a 25% uncertainty but was fitted as a free parameter. An interesting question is whether now, after recent Monte Carlo calculations, the error on the total normalization could be reduced of a relevant factor and be used in the fit of neutrino oscillation studies.
Slide n.9 shows results of SK Fit using 3D Flux Calculations.
(M.L.).

[Kearns:2002jh]
[3-13]
Atmospheric and long baseline neutrino, T. Nakaya (Super-Kamiokande), eConf C020620 (2002) SAAT01, arXiv:hep-ex/0209036. 22nd Physics in Collision Conference (PIC 2002), Stanford, California, 20-22 June 2002.
[Nakaya:2002ki]
[3-14]
Status and prospects of neutrino oscillations: Atmospheric, T. Kajita, 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.
[Kajita-talk:2002c]
[3-15]
Atmospheric Neutrinos and K2K, K. Nishikawa, 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.
[Nishikawa-talk:2002b]
[3-16]
Experimental measurements of atmospheric neutrinos, Edward Kearns, Nucl. Phys. Proc. Suppl. 70 (1999) 315-323, arXiv:hep-ex/9803007.
[Kearns:1997jn]

4 - Reviews - Phenomenology

[4-1]
Atmospheric Neutrinos: Status and Prospects, Sandhya Choubey, Nucl. Phys. B908 (2016) 235-249, arXiv:1603.06841.
[Choubey:2016gps]
[4-2]
Neutrino oscillations, G. Bellini, L. Ludhova, G. Ranucci, F.L. Villante, Adv.High Energy Phys. 2014 (2014) 191960, arXiv:1310.7858.
[Bellini:2013wra]
[4-3]
Neutrino Propagation in Matter, Mattias Blennow, Alexei Yu. Smirnov, Adv.High Energy Phys. 2013 (2013) 972485, arXiv:1306.2903.
[Blennow:2013rca]
[4-4]
Atmospheric leptons, the search for a prompt component, Thomas K. Gaisser, EPJ Web Conf. 52 (2013) 09004, arXiv:1303.1431.
[Gaisser:2013ira]
[4-5]
Phenomenology with Massive Neutrinos, M. C. Gonzalez-Garcia, Michele Maltoni, Phys. Rept. 460 (2008) 1-129, arXiv:0704.1800.
[GonzalezGarcia:2007ib]
[4-6]
Global analysis of three-flavor neutrino masses and mixings, G. L. Fogli, E. Lisi, A. Marrone, A. Palazzo, Prog. Part. Nucl. Phys. 57 (2006) 742-795, arXiv:hep-ph/0506083.
[Fogli:2005cq]
[4-7]
Atmospheric neutrinos and neutrino oscillations, Takaaki Kajita, Paolo Lipari, Comptes Rendus Physique 6 (2005) 739-748.
[Kajita-Lipari-CRP6-739-2005]
[4-8]
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.
[Back:2004qi]
[4-9]
Neutrino Masses and Oscillations: Triumphs and Challenges, R.D. McKeown, P. Vogel, Phys. Rep. 394 (2004) 315, arXiv:hep-ph/0402025.
[McKeown:2004yq]
[4-10]
Cosmic rays, T. K. Gaisser, T. Stanev, Phys. Lett. B592 (2004) 228-234. The Review of Particle Properties 2004. http://pdg.lbl.gov/2004/reviews/cosmicrayrpp.pdf.
[Gaisser:2004eh]
[4-11]
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.
[Giunti:2003qt]
[4-12]
Flux of Atmospheric Neutrinos, T. K. Gaisser, M. Honda, Ann. Rev. Nucl. Part. Sci. 52 (2002) 153, arXiv:hep-ph/0203272.
[Gaisser:2002jj]
[4-13]
Neutrino Masses and Mixing: Evidence and Implications, M.C. Gonzalez-Garcia, Y. Nir, Rev. Mod. Phys. 75 (2003) 345-402, arXiv:hep-ph/0202058.
[GonzalezGarcia:2002dz]
[4-14]
Finally neutrino has mass?, S. M. Bilenky, C. Giunti, C. W. Kim, Int. J. Mod. Phys. A15 (2000) 625-650, arXiv:hep-ph/9902462.
[Bilenky:1999mf]
[4-15]
Phenomenology of neutrino oscillations, S. M. Bilenky, C. Giunti, W. Grimus, Prog. Part. Nucl. Phys. 43 (1999) 1, arXiv:hep-ph/9812360.
[Bilenky:1998dt]
[4-16]
Cosmic ray showers, K. Greisen, Ann. Rev. Nucl. Part. Sci. 10 (1960) 63-108.
[Greisen:1960wc]

5 - Reviews - Phenomenology - Conference Proceedings

[5-1]
Atmospheric Neutrinos, Thomas K. Gaisser, J. Phys. Conf. Ser. 718 (2016) 052014, arXiv:1605.03073. TAUP 2015.
[Gaisser:2016obt]
[5-2]
Neutrino 2012: Outlook - theory, A. Yu. Smirnov, Nucl. Phys. Proc. Suppl. 235-236 (2013) 431-440, arXiv:1210.4061. XXV International Conference on Neutrino Physics and Astrophysics, June 3 - 9, 2012, Kyoto, Japan.
[Smirnov:2012ei]
[5-3]
Muons and Neutrinos 2007, Thomas K. Gaisser, arXiv:0801.4542, 2008. 30th International Cosmic Ray Conference, Merida, Yucatan, July, 2007.
[Gaisser:2008cp]
[5-4]
Atmospheric Neutrinos, Thomas K. Gaisser, AIP Conf. Proc. 944 (2007) 140-142, arXiv:astro-ph/0612274. Neutrino 2006.
[Gaisser:2006np]
[5-5]
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.
[Schwetz:2006dh]
[5-6]
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.
[Schwetz:2005jr]
[5-7]
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.
[Fogli:2005gs]
[5-8]
Atmospheric neutrino challenges, Todor Stanev, Nucl. Phys. Proc. Suppl. 145 (2005) 69, arXiv:astro-ph/0412395. NOW 2004.
[Stanev:2004js]
[5-9]
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.
[Akhmedov:2004ve]
[5-10]
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.
[Valle:2004cr]
[5-11]
Neutrino 2004: Concluding Talk, Guido Altarelli, Nucl. Phys. Proc. Suppl. 143 (2005) 470, arXiv:hep-ph/0410101. Neutrino 2004, Paris, 14-19 June 2004.
[Altarelli:2004cp]
[5-12]
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.
[GonzalezGarcia:2004jd]
[5-13]
Neutrino physics, recent results, E. Lisi, 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.
[Lisi:IFAE2004]
[5-14]
Global analysis of neutrino oscillation, S. Goswami, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/goswami.pdf.
[Goswami-Nu2004]
[5-15]
Neutrino masses twenty-five years later, J W F Valle, Aip Conf. Proc. 687 (2003) 16, arXiv:hep-ph/0307192. MRST'03 (Joe-Fest), Syracuse, NY, May 2003.
[Valle:2003rh]
[5-16]
Neutrino oscillations in the framework of the tree-neutrino mixing, S. M. Bilenky, arXiv:hep-ph/0307186, 2003. Ist Yamada Symposium Om neutrinos and Dark Matter in Nuclear Physics, June 9-14, 2003, Nara, Japan.
[Bilenky:2003rb]
[5-17]
Neutrino Physics after KamLAND, Alexei Yu. Smirnov, 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.
[Smirnov:2003uu]
[5-18]
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.
[Giunti:2003vf]
[5-19]
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).
[GonzalezGarcia:2002sm]
[5-20]
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.
[GonzalezGarcia:2002sz]
[5-21]
Current Status of Neutrino Masses and Mixings, C. Giunti, Nucl. Phys. Proc. Suppl. 117 (2003) 24-28, arXiv:hep-ph/0209103. 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.
[Giunti:2002sr]

6 - PhD Theses

[6-1]
New physics with atmospheric Neutrinos, C. A. Arguelles, 2015. PhD thesis, ISBN 978-1-339-06088-0. https://docushare.icecube.wisc.edu/dsweb/Get/Document-75669/tesis.pdf.
[Arguelles:2015a]
[6-2]
Sterile Neutrinos in Cold Climates, Benjamin J. P. Jones, 2015. PhD thesis, FERMILAB-THESIS-2015-17. http://lss.fnal.gov/archive/thesis/2000/fermilab-thesis-2015-17.pdf.
[Jones:2015bya]
[6-3]
First Evidence For Atmospheric Neutrino-Induced Cascades with the IceCube Detector, Michelangelo D'Agostino, arXiv:0910.2555, 2009.
[DAgostino:2009wft]

7 - Experiment

[7-1]
Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation, E. Richard et al. (Super-Kamiokande), Phys. Rev. D94 (2016) 052001, arXiv:1510.08127.
[Richard:2015aua]
[7-2]
Measurement of the Atmospheric $\nu_e$ Spectrum with IceCube, M. G. Aartsen et al. (IceCube), Phys. Rev. D91 (2015) 122004, arXiv:1504.03753.
[Aartsen:2015xup]
[7-3]
Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data, M. G. Aartsen et al. (IceCube), Phys. Rev. D91 (2015) 072004, arXiv:1410.7227.
[Aartsen:2014yll]
[7-4]
Test of Lorentz Invariance with Atmospheric Neutrinos, K. Abe et al. (Super-Kamiokande), Phys. Rev. D91 (2015) 052003, arXiv:1410.4267.
[Abe:2014wla]
[7-5]
Limits on Sterile Neutrino Mixing using Atmospheric Neutrinos in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D91 (2015) 052019, arXiv:1410.2008.
[Abe:2014gda]
[7-6]
Atmospheric and Astrophysical Neutrinos above 1 TeV Interacting in IceCube, M. G. Aartsen et al. (IceCube), Phys. Rev. D91 (2015) 022001, arXiv:1410.1749.
[Aartsen:2014muf]
[7-7]
Development of a General Analysis and Unfolding Scheme and its Application to Measure the Energy Spectrum of Atmospheric Neutrinos with IceCube, M. G. Aartsen et al. (IceCube), Eur.Phys.J. C75 (2015) 116, arXiv:1409.4535.
[Aartsen:2014qna]
[7-8]
Measurement of the atmospheric $\nu_\mu$ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope, S. Adrian-Martinez et al. (ANTARES), Eur.Phys.J. C73 (2013) 2606, arXiv:1308.1599.
[Adrian-Martinez:2013bqq]
[7-9]
Measurement of Atmospheric Neutrino Oscillations with IceCube, M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 111, 081801 (2013) 081801, arXiv:1305.3909.
[Aartsen:2013jza]
[7-10]
Ultrahigh Energy Neutrinos at the Pierre Auger Observatory, P. Abreu et al. (Pierre Auger), Adv.High Energy Phys. 2013 (2013) 708680, arXiv:1304.1630.
[Abreu:2013zbq]
[7-11]
Measurement of the Atmospheric $\nu_e$ flux in IceCube, M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 110 (2013) 151105, arXiv:1212.4760.
[Aartsen:2012uu]
[7-12]
Measurements of atmospheric neutrinos and antineutrinos in the MINOS Far Detector, P. Adamson et al. (MINOS), Phys. Rev. D86 (2012) 052007, arXiv:1208.2915.
[Adamson:2012gt]
[7-13]
Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope, ANTARES collaboration, S. Adrian-Martinez et al. (ANTARES), Phys. Lett. B714 (2012) 224-230, arXiv:1206.0645.
[AdrianMartinez:2012ph]
[7-14]
A Measurement of the Appearance of Atmospheric Tau Neutrinos by Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 110 (2013) 181802, arXiv:1206.0328.
[Abe:2012jj]
[7-15]
Study of Non-Standard Neutrino Interactions with Atmospheric Neutrino Data in Super-Kamiokande I and II, G. Mitsuka et al. (Kamiokande), Phys. Rev. D84 (2011) 113008, arXiv:1109.1889.
[Mitsuka:2011ty]
[7-16]
Search for Differences in Oscillation Parameters for Atmospheric Neutrinos and Antineutrinos at Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 107 (2011) 241801, arXiv:1109.1621.
[Abe:2011ph]
[7-17]
First search for atmospheric and extraterrestrial neutrino-induced cascades with the IceCube detector, R. Abbasi et al. (IceCube), Phys. Rev. D84 (2011) 072001, arXiv:1101.1692.
[Abbasi:2011ui]
[7-18]
Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube, R. Abbasi et al. (IceCube), Phys. Rev. D83 (2011) 012001, arXiv:1010.3980.
[Abbasi:2010ie]
[7-19]
The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory, R. Abbasi et al. (IceCube), Phys. Rev. D82 (2010) 072003, arXiv:1009.1442.
[Abbasi:2010ak]
[7-20]
The Energy Spectrum of Atmospheric Neutrinos between 2 and 200 TeV with the AMANDA-II Detector, R. Abbasi et al. (IceCube), Astropart. Phys. 34 (2010) 48-58, arXiv:1004.2357.
[Abbasi:2010qv]
[7-21]
Atmospheric neutrino oscillation analysis with sub-leading effects in Super-Kamiokande I, II, and III, R. Wendell et al. (Super-Kamiokande), Phys. Rev. D81 (2010) 092004, arXiv:1002.3471.
[Wendell:2010md]
[7-22]
Measurement of the Cosmic Ray and Neutrino-Induced Muon Flux at the Sudbury Neutrino Observatory, SNO Collaboration (SNO), Phys. Rev. D80 (2009) 012001, arXiv:0902.2776.
[Aharmim:2009zm]
[7-23]
Determination of the Atmospheric Neutrino Flux and Searches for New Physics with AMANDA-II, R. Abbasi et al. (IceCube), Phys. Rev. D79 (2009) 102005, arXiv:0902.0675.
[Abbasi:2009nfa]
[7-24]
Kinematic reconstruction of atmospheric neutrino events in a large water Cherenkov detector with proton identification, M. Fechner et al. (Super-Kamiokande), Phys. Rev. D79 (2009) 112010, arXiv:0901.1645.
[Fechner:2009aa]
[7-25]
Search for Matter-Dependent Atmospheric Neutrino Oscillations in Super-Kamiokande, K. Abe et al. (Super-Kamiokande), Phys. Rev. D77 (2008) 052001, arXiv:0801.0776.
[Abe:2008zza]
[7-26]
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.
[Mine:2008rt]
[7-27]
Detection of Atmospheric Muon Neutrinos with the IceCube 9-String Detector, A. Achterberg et al. (IceCube), Phys. Rev. D76 (2007) 027101, arXiv:0705.1781.
[Achterberg:2007bi]
[7-28]
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.
[Adamson:2007vt]
[7-29]
A Measurement of Atmospheric Neutrino Flux Consistent with Tau Neutrino Appearance, K. Abe et al. (Super-Kamiokande), Phys. Rev. Lett. 97 (2006) 171801, arXiv:hep-ex/0607059.
From the abstract: The Super-Kamiokande-I atmospheric neutrino data for 1489.2 days, which find a best fit tau neutrino appearance signal of $ 138 \pm 48 \text{(stat.)} {}^{+15}_{-32} \text{(sys.)} $, disfavor the hypothesis of no tau neutrino appearance by 2.4 sigma.
[Abe:2006fu]
[7-30]
Three flavor neutrino oscillation analysis of atmospheric neutrinos in Super-Kamiokande, J. Hosaka et al. (Super-Kamiokande), Phys. Rev. D74 (2006) 032002, arXiv:hep-ex/0604011.
[Hosaka:2006zd]
[7-31]
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: $ R_{\mathrm{up/down}}^{\mathrm{data}}/R_{\mathrm{up/down}}^{\mathrm{MC}} = 0.62^{+0.19}_{-0.14} \pm 0.02 $... The ratio of $\bar{\nu}_\mu$ to $\nu_\mu$ events in the data is compared to the Monte Carlo expectation assuming neutrinos and anti-neutrinos oscillate in same manner giving: $ R_{\mathrm{\bar{\nu}_\mu/\nu_\mu}}^{\mathrm{data}}/R_{\mathrm{\bar{\nu}_\mu/\nu_\mu}}^{\mathrm{MC}} = 0.96^{+0.38}_{-0.27} \pm 0.15 $... Although the statistics are limited, this is the first direct observation of atmospheric neutrino interactions separately for $\nu_\mu$ and $\bar\nu_\mu$.
[Adamson:2005qc]
[7-32]
Neutrino Oscillation Effects in Soudan-2 Upward-stopping muons, W. W. M. Allison et al. (Soudan-2), Phys. Rev. D72 (2005) 052005, arXiv:hep-ex/0507068.
[Allison:2005dt]
[7-33]
A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I, Y. Ashie et al. (Super-Kamiokande), Phys. Rev. D71 (2005) 112005, arXiv:hep-ex/0501064.
[Ashie:2005ik]
[7-34]
Evidence for an oscillatory signature in atmospheric neutrino oscillation, Y. Ashie et al. (Super-Kamiokande), Phys. Rev. Lett. 93 (2004) 101801, arXiv:hep-ex/0404034.
From the abstract: Muon neutrino disappearance probability as a function of neutrino flight length $L$ over neutrino energy $E$ was studied.
A dip in the $L/E$ distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation.
The observed $L/E$ distribution constrained $\nu_\mu \leftrightarrow \nu_\tau$ neutrino oscillation parameters; $1.9 \times 10^{-3} < \Delta m^2 < 3.0 \times 10^{-3} \, \mathrm{eV}^2$ and $\sin^22\theta > 0.90$ at 90% confidence level.

[Ashie:2004mr]
[7-35]
Observation of Atmospheric Neutrino Oscillations in Soudan 2, M. Sanchez et al. (Soudan 2), Phys. Rev. D68 (2003) 113004, arXiv:hep-ex/0307069.
[Sanchez:2003rb]
[7-36]
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.
[Ambrosio:2003yz]
[7-37]
Matter effects in upward-going muons and sterile neutrino oscillations, M. Ambrosio et al. (MACRO), Phys. Lett. B517 (2001) 59-66, arXiv:hep-ex/0106049.
[Ambrosio:2001je]
[7-38]
Tau neutrinos favored over sterile neutrinos in atmospheric muon neutrino oscillations, S. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 85 (2000) 3999-4003, arXiv:hep-ex/0009001.
[Fukuda:2000np]
[7-39]
Low energy atmospheric muon neutrinos in MACRO, M. Ambrosio et al. (MACRO), Phys. Lett. B478 (2000) 5-13.
[Ambrosio:2000qy]
[7-40]
The atmospheric neutrino flavor ratio from a 3.9 fiducial kiloton-year exposure of Soudan 2, W. W. M. Allison et al. (Soudan-2), Phys. Lett. B449 (1999) 137-144, arXiv:hep-ex/9901024.
[Allison:1999ms]
[7-41]
Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 82 (1999) 2644-2648, arXiv:hep-ex/9812014.
[Fukuda:1998ah]
[7-42]
Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO, M. Ambrosio et al. (MACRO), Phys. Lett. B434 (1998) 451-457, arXiv:hep-ex/9807005.
[Ambrosio:1998wu]
[7-43]
Evidence for oscillation of atmospheric neutrinos, Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81 (1998) 1562-1567, arXiv:hep-ex/9807003.
[Fukuda:1998mi]
[7-44]
Measurement of the flux and zenith angle distribution of upward through-going muons in Kamiokande II + III, S. Hatakeyama et al. (Kamiokande), Phys. Rev. Lett. 81 (1998) 2016-2019, arXiv:hep-ex/9806038.
[Hatakeyama:1998ea]
[7-45]
Study of the atmospheric neutrino flux in the multi-GeV energy range, Y. Fukuda et al. (Super-Kamiokande), Phys. Lett. B436 (1998) 33-41, arXiv:hep-ex/9805006.
[Fukuda:1998ub]
[7-46]
Measurement of a small atmospheric nu/mu / nu/e ratio, Y. Fukuda et al. (Super-Kamiokande), Phys. Lett. B433 (1998) 9-18, arXiv:hep-ex/9803006.
[Fukuda:1998tw]
[7-47]
The Baksan underground scintillation telescope, E. N. Alekseev et al., Phys. Part. Nucl. 29 (1998) 254-256.
[Alekseev:1998ib]
[7-48]
Atmospheric muon-neutrino fraction above 1-GeV, R. Clark et al. (IMB), Phys. Rev. Lett. 79 (1997) 345-348.
[Clark:1997cb]
[7-49]
Study of neutron background in the atmospheric neutrino sample in Kamiokande, Y. Fukuda et al. (Kamiokande), Phys. Lett. B388 (1996) 397-401.
[Fukuda:1996sy]
[7-50]
Determination of the atmospheric neutrino spectra with the Frejus detector, K. Daum (Frejus.), Z. Phys. C66 (1995) 417-428.
[Daum:1994bf]
[7-51]
Atmospheric muon-neutrino / electron-neutrino ratio in the multiGeV energy range, Y. Fukuda et al. (Kamiokande), Phys. Lett. B335 (1994) 237-245.
[Fukuda:1994mc]
[7-52]
IMB-3: A Large water Cerenkov detector for nucleon decay and neutrino interactions, R. Becker-Szendy et al. (IMB), Nucl. Instrum. Meth. A324 (1993) 363-382.
[BeckerSzendy:1993mb]
[7-53]
Observation of a small atmospheric $\nu_\mu / \nu_e $ ratio in Kamiokande, K. S. Hirata et al. (Kamiokande), Phys. Lett. B280 (1992) 146-152.
[Hirata:1992ku]
[7-54]
Survey of atmospheric neutrino data and implications for neutrino mass and mixing, E. W. Beier et al., Phys. Lett. B283 (1992) 446-453.
[Beier:1992sf]
[7-55]
The electron-neutrino and muon-neutrino content of the atmospheric flux, R. Becker-Szendy et al. (IMB), Phys. Rev. D46 (1992) 3720-3724.
[BeckerSzendy:1992hq]
[7-56]
A Search for muon-neutrino oscillations with the IMB detector, R. Becker-Szendy et al. (IMB), Phys. Rev. Lett. 69 (1992) 1010-1013.
[BeckerSzendy:1992ym]
[7-57]
Experimental study of upward stopping muons in NUSEX, M. Aglietta et al., Europhys. Lett. 15 (1991) 559-564.
[Aglietta:1991um]
[7-58]
Flux and angular distribution of muons created by cosmic ray neutrinos, M. M. Boliev et al., Bull. Russ. Acad. Sci. Phys. 55 (1991) NO.4126.
[Boliev:1991sp]
[7-59]
Measurement of atmospheric neutrino composition with IMB-3, D. Casper et al. (IMB), Phys. Rev. Lett. 66 (1991) 2561-2564.
[Casper:1990ac]
[7-60]
A Study of atmospheric neutrino oscillations in the Frejus experiment, Christoph Berger et al. (Frejus), Phys. Lett. B245 (1990) 305-310.
[Berger:1990rd]
[7-61]
Experimental study of atmospheric neutrino flux in the NUSEX experiment, M. Aglietta et al. (The NUSEX), Europhys. Lett. 8 (1989) 611-614.
[Aglietta:1988be]
[7-62]
Experimental study of upward going muons in Kamiokande, Y. Oyama et al. (Kamiokande), Phys. Rev. D39 (1989) 1481.
[Oyama:1989sw]
[7-63]
Study of atmospheric neutrino interactions with the Frejus detector, Christoph Berger et al. (Frejus), Phys. Lett. B227 (1989) 489.
[Berger:1989wy]
[7-64]
Experimental study of the atmospheric neutrino flux, K. S. Hirata et al. (Kamiokande), Phys. Lett. B205 (1988) 416.
[Hirata:1988uy]
[7-65]
Contained neutrino interactions in an underground water detector, R. M. Bionta et al. (IMB), Phys. Rev. D38 (1988) 768-775.
[Bionta:1988an]
[7-66]
Calculation of atmospheric neutrino induced backgrounds in a nucleon decay search, T. J. Haines et al. (IMB), Phys. Rev. Lett. 57 (1986) 1986-1989.
[Haines:1986yf]
[7-67]
Atmospheric neutrino background and pion nuclear effect for Kamioka nucleon decay experiment, Masayuki Nakahata et al. (Kamiokande), J. Phys. Soc. Jap. 55 (1986) 3786.
[Nakahata:1986zp]
[7-68]
Status of the Frejus experiment and preliminary results on contained events, P. Bareyre et al. (AACHEN-ORSAY-PALAISEAU-SACLAY-WUPPERTAL), Nuovo Cim. C9 (1986) 159-166.
[Bareyre:1986er]
[7-69]
Test of neutrino oscillations using atmospheric neutrinos, J. M. LoSecco et al. (IMB), Phys. Rev. Lett. 54 (1985) 2299.
[LoSecco:1985py]
[7-70]
Nucleon stability, magnetic monopoles and atmospheric neutrinos in the Mont Blanc experiment, G. Battistoni et al., Phys. Lett. B133 (1983) 454.
[Battistoni:1983ka]
[7-71]
Neutrino backgrounds in the Kolar Gold Field nucleon decay experiment, M. r. Krishnaswamy et al., Pramana 19 (1982) 525-554.
[Krishnaswamy:1982sr]
[7-72]
Fully contained events in the Mont Blanc nucleon decay detector, G. Battistoni et al., Phys. Lett. B118 (1982) 461.
[Battistoni:1982vv]
[7-73]
Limitations on parameters of neutrino oscillations according to data of the baksan underground telescope, M. M. Boliev et al., Yad. Fiz. 34 (1981) 1418-1421. In Russian.
[Boliev:1981tc]
[7-74]
Cosmic ray muon fluxes deep underground: intensity versus depth, and the neutrino induced component, M. F. Crouch et al., Phys. Rev. D18 (1978) 2239-2252.
[Crouch:1978mg]
[7-75]
Evidence for the production of a new particle in neutrino interactions, M. R. Krishnaswamy et al., Phys. Lett. B57 (1975) 105.
[Krishnaswamy:1975zu]
[7-76]
Neutrino-induced muons deep underground, H. E. Bergeson, G. L. Cassiday, M. B. Hendricks, Phys. Rev. Lett. 31 (1973) 66-70.
[Bergeson:1973kp]
[7-77]
Muons produced by atmospheric neutrinos: Analysis, H. H. Chen, W. R. Kropp, H. W. Sobel, F. Reines, Phys. Rev. D4 (1971) 99-121.
[Chen:1971ma]
[7-78]
Muons produced by atmospheric neutrinos: Experiment, F. Reines et al., Phys. Rev. D4 (1971) 80-98.
[Reines:1971qh]
[7-79]
M. R. Krishnaswamy et al., Proc. R. Soc. London A323 (1971) 489.
[Krishnaswamy:1971]
[7-80]
Detection of muons produced by cosmic ray neutrinos deep underground, C. V. Achar et al., Phys. Lett. 18 (1965) 196-199.
[Achar-etal-PL18-196-1965]
[7-81]
Observation of a non-elastic cosmic ray neutrino interaction, C. V. Achar et al., Phys. Lett. 19 (1965) 78-80.
[Achar-etal-PL19-78-1965]
[7-82]
Evidence for high-energy cosmic ray neutrino interactions, F. Reines et al., Phys. Rev. Lett. 15 (1965) 429-433.
[Reines:1965qk]

8 - Experiment - Conference Proceedings

[8-1]
Constraints on atmospheric charmed-meson production from IceCube, Tomasz Palczewski (IceCube), EPJ Web Conf. 130 (2016) 05015, arXiv:1611.00816. Meson 2016.
[Palczewski:2016ucy]
[8-2]
Atmospheric Results from Super-Kamiokande, Roger Wendell (Super-Kamiokande), AIP Conf. Proc. 1666 (2015) 100001, arXiv:1412.5234. XXVI International Conference on Neutrino Physics and Astrophysics (Neutrino 2014).
[Wendell:2014dka]
[8-3]
Recent Atmospheric Neutrino Results from Super-Kamiokande, Alexander Himmel (Super-Kamiokande), AIP Conf.Proc. 1604 (2014) 345-352, arXiv:1310.6677. VII International Conference on Interconnections between Particle Physics and Cosmology (PPC2013).
[Himmel:2013jva]
[8-4]
The IceCube Neutrino Observatory Part II: Atmospheric and Diffuse UHE Neutrino Searches of All Flavors, M. G. Aartsen et al. (IceCube), arXiv:1309.7003, 2013. 33nd International Cosmic Ray Conference, Rio de Janeiro 2013.
[Aartsen:2013jla]
[8-5]
A view of prompt atmospheric neutrinos with IceCube, Anne Schukraft (IceCube), Nucl. Phys.B, Proc.Suppl.237-238 2013 (2013) 266-268, arXiv:1302.0127. NOW 2012.
[Schukraft:2013ya]
[8-6]
Atmospheric Neutrino Oscillations in IceCube, Andreas Gros (IceCube), Nucl. Phys.B, Proc.Suppl.237-238 2013 (2013) 272-274, arXiv:1301.4339. NOW 2012.
[Gross:2013iq]
[8-7]
Detection of Cascades induced by Atmospheric Neutrinos in the 79-string IceCube Detector, Chang Hyon Ha (IceCube), arXiv:1209.0698, 2012. CIPANP 2012.
[ChangHyonHaIceCube:2012aza]
[8-8]
The First Year IceCube-DeepCore Results, Chang Hyon Ha (IceCube), J. Phys. Conf. Ser. 375 (2012) 052034, arXiv:1201.0801. TAUP 2011.
[Ha:2012np]
[8-9]
Results from Super-Kamiokande, Yasuo Takeuchi (Super-Kamiokande), Nucl. Phys.B, Proc.Suppl.229-232 2012 (2012) 79-84, arXiv:1112.3425. XXIV International Conference on Neutrino Physics and Astrophysics (Neutrino 2010).
[Takeuchi:2011aa]
[8-10]
The IceCube Neutrino Observatory VI: Neutrino Oscillations, Supernova Searches, Ice Properties, R. Abbasi et al. (IceCube), arXiv:1111.2731, 2011. 32nd International Cosmic Ray Conference, Beijing 2011.
[Abbasi:2011eva]
[8-11]
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.
[Gaisser:2009cz]
[8-12]
Neutrino Oscillation Measurements with IceCube, Carsten Rott (IceCube), arXiv:0810.3698, 2008. ICHEP08.
[Rott:2008uq]
[8-13]
Recent Results from Super-Kamiokande, H. Sekiya et al. (Super-Kamiokande), arXiv:0810.0595, 2008. ICHEP08, Philadelphia, USA, July 2008.
[Sekiya:2008nb]
[8-14]
The Super-Kamiokande Experiment, C.W. Walter, arXiv:0802.1041, 2008. Neutrino Oscillations: Present Status and Future Plans.
[Walter:2008ys]
[8-15]
The MACRO Experiment at Gran Sasso, G. Giacomelli, A. Margiotta, arXiv:0707.1691, 2007. Charles Peck - Fest, Caltech, 2005.
[Giacomelli:2007sk]
[8-16]
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.
[Silvestri:2007hi]
[8-17]
Neutrino-induced muons observed with MINOS, Alec T. Habig (MINOS), arXiv:hep-ex/0507010, 2005. 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, 3-11 Aug 2005.
[Habig:2005gu]
[8-18]
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.
[Giacomelli:2005kr]
[8-19]
Upward Showering Muons in Super-Kamiokande, S. Desai, A. Habig (Super-Kamiokande), 2005. 29th International Cosmic Ray Conference (ICRC 2005), Pune, India, 3-11 Aug 2005. http://budoe.bu.edu/~shantanu/icrc05showering.sxi.pdf.
[DesaiHabig-ICRC05:]
[8-20]
SuperK recent results, K. Scholberg (Super-Kamiokande), 2005. 20th International Workshop on Weak Interactions and Neutrinos (WIN'05), June 6-11, 2005, Delphi, Greece. http://conferences.phys.uoa.gr/win05/WIN05_WG3/scholberg.ppt.
Comment: Atmospheric neutrino results from a new (320 bins) analysis are presented. [M.L.].
[Scholberg:WIN2005]
[8-21]
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.
[Giacomelli:2004va]
[8-22]
Super Kamiokande results: atmospheric and solar neutrinos, M.Ishitsuka, Super-Kamiokande (Super-Kamiokande), arXiv:hep-ex/0406076, 2004. XXXIXth Rencontres de Moriond on Electroweak Interactions (2004).
[Ishitsuka:2004un]
[8-23]
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.
[Giacomelli:2004cw]
[8-24]
Direct oscillatory evidence from the L/E analysis in Super-Kamiokande, M. Ishitsuka (Super-Kamiokande), 2004. NOON2004, The 5th Workshop on 'Neutrino Oscillations and their Origin', 11-15 February 2004, Tokyo, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2004/trape/10-ishitsuka.pdf.
Comment: First oscillation dip is observed in L/E data sample (see this figure).
[Ishitsuka-NOON2004]
[8-25]
Atmospheric neutrino results from SuperKamiokande, E. Kearns (Super-Kamiokande), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/kearns.pdf.
[Kearns-Nu2004]
[8-26]
SK atmospheric neutrino, C. Saji (Super-Kamiokande), 2004. NOON2004, The 5th Workshop on 'Neutrino Oscillations and their Origin', 11-15 February 2004, Tokyo, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2004/trape/09-Saji.pdf.
[Saji-NOON2004]
[8-27]
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.
[Gallagher-Nu2004]
[8-28]
Searching for atmospheric neutrino oscillations at MINOS, A. Blake (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.
[Blake:UKIP2004]
[8-29]
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.
[Ayutdinov:2003eh]
[8-30]
Recent results from atmospheric $\nu$ and K2K, Y. Itow, 2003. 2nd International conference on Flavor Physics, ICFP 2003, 6-11 October 2003, Korea Institute for Advanced Study (KIAS). http://newton.kias.re.kr/~hepph/public_html/03icfp/talk/itow1.pdf.
Comment: The figure in slide n.34 shows the K2K excluded region for oscillations of accelerator neutrinos in the $\nu_{\mu} \to \nu_e$ channel as compared with the CHOOZ limit and the Super-Kamiokande allowed region. [M.L.].
[Itow:ICFP2003]
[8-31]
Atmospheric Neutrino Oscillations in Super-Kamiokande I, A. Ahabig (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.
[Ahabig:ICRC2003]
[8-32]
Status of the Super-Kamiokande, the K2K-2 experiment and JHF nu project, Y. Hayato, 2003. EPS2003. http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07Hayato.ppt.
[Hayato:EPS2003]
[8-33]
New Results from Super-K and K2K, R. Jeffrey Wilkes (K2K), eConf C020805 (2002) TTH02, arXiv:hep-ex/0212035. Secrets of the B-Meson, Topical Conference, XXX SLAC Summer Institute, SLAC, August, 2002.
[Wilkes:2002mb]
[8-34]
Other Atmospheric Neutrino Experiments, Maury Goodman, 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.
[Goodman:2002ne]
[8-35]
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.
[Giorgini:2002it]
[8-36]
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.
[Giacomelli:2002nn]
[8-37]
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.
[Smy:2002hr]
[8-38]
Atmospheric neutrino oscillations, G. Giacomelli, M. Giorgini, M. Spurio, arXiv:hep-ex/0201032, 2002.
[Giacomelli:2002tj]
[8-39]
Results from Soudan-2 on Atmospheric Neutrinos and Limits on Matter Instability, T. Mann (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.
[Mann-talk:2002b]
[8-40]
Experimental results on atmospheric neutrinos in Super-Kamiokande-I, M. Shiozawa (Super-Kamiokande), 2002. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/shiozawa.
[Shiozawa-Nu2002]
[8-41]
Atmospheric Neutrinos: Status and Prospects with approved Experiments, M. Shiozawa (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.
[Shiozawa-NNN02]
[8-42]
Atmospheric Neutrinos at Super-Kamiokande, C. Mauger (Super-Kamiokande), 2002. 31st International Conference on High Energy Physics - ICHEP 02 - Amsterdam, Holland, 24-31 July 2002. http://www.ichep02.nl/Transparencies/NEU/NEU-1/NEU-1-4.Mauger.pdf.
[Mauger-ICHEP-2002]
[8-43]
Atmospheric Neutrinos, Y. Totsuka, 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 [15-43]?.
[Totsuka-TAUP2001]
[8-44]
Experiments with Solar and Atmospheric Neutrinos: Evidence for Neutrino Masses and Lepton Mixing. Experimental status and Future Projects, S. Schoenert, 2001. Astroparticle Physics Workshop, DESY - Zeuten, 19-21 June 2001. http://www.desy.de/desy-hs/zeuthen2001/presentations/main/schoenert.pdf.
[Schoenert-DESY-2001]
[8-45]
Atmospheric neutrino results from Super-Kamiokande, M. D. Messier, Int. J. Mod. Phys. A16S1B (2001) 733-735.
[Messier:2001pk]
[8-46]
Atmospheric neutrinos at Super-Kamiokande, Kate Scholberg (Super-Kamiokande), arXiv:hep-ex/9905016, 1999.
[Scholberg:1999ar]

9 - Experiment - Neutrino Oscillations

[9-1]
New measurement of $\theta_{13}$ via neutron capture on hydrogen at Daya Bay, F. P. An et al. (Daya Bay), Phys. Rev. D93 (2016) 072011, arXiv:1603.03549.
[An:2016bvr]
[9-2]
First measurement of muon-neutrino disappearance in NOvA, P. Adamson et al. (NOvA), Phys. Rev. D93 (2016) 051104, arXiv:1601.05037.
[Adamson:2016xxw]
[9-3]
First measurement of electron neutrino appearance in NOvA, P. Adamson et al. (NOvA), Phys. Rev. Lett. 116 (2016) 151806, arXiv:1601.05022.
[Adamson:2016tbq]
[9-4]
Measurement of muon anti-neutrino oscillations with an accelerator-produced off-axis beam, K. Abe et al. (T2K), Phys. Rev. Lett. 116 (2016) 181801, arXiv:1512.02495.
[Abe:2015ibe]
[9-5]
Observation of Energy and Baseline Dependent Reactor Antineutrino Disappearance in the RENO Experiment, J.H. Choi et al. (RENO), Phys. Rev. Lett. 116 (2016) 211801, arXiv:1511.05849.
[RENO:2015ksa]
[9-6]
Measurement of $\theta_{13}$ in Double Chooz using neutron captures on hydrogen with novel background rejection techniques, Y. Abe et al. (Double Chooz), JHEP 01 (2016) 163, arXiv:1510.08937.
[Abe:2015rcp]
[9-7]
Discovery of tau neutrino appearance in the CNGS neutrino beam with the OPERA experiment, N. Agafonova et al. (OPERA), Phys. Rev. Lett. 115 (2015) 121802, arXiv:1507.01417.
[Agafonova:2015jxn]
[9-8]
A new measurement of antineutrino oscillation with the full detector configuration at Daya Bay, F. P. An et al. (Daya Bay), Phys. Rev. Lett. 115 (2015) 111802, arXiv:1505.03456.
[An:2015rpe]
[9-9]
Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam, N. Agafonova et al. (OPERA), JHEP 1506 (2015) 069, arXiv:1503.01876.
[Agafonova:2015neo]
[9-10]
Some conclusive considerations on the comparison of the ICARUS $\nu_\mu \to \nu_e$ oscillation search with the MiniBooNE low-energy event excess, M. Antonello et al., arXiv:1502.04833, 2015.
[Antonello:2015jxa]
[9-11]
Measurements of neutrino oscillation in appearance and disappearance channels by the T2K experiment with 6.6E20 protons on target, K. Abe et al. (T2K), Phys. Rev. D91 (2015) 072010, arXiv:1502.01550.
[Abe:2015awa]
[9-12]
Observation of tau neutrino appearance in the CNGS beam with the OPERA experiment, N. Agafonova et al. (OPERA), PTEP 2014 (2014) 101C01, arXiv:1407.3513.
[Agafonova:2014ptn]
[9-13]
Improved measurements of the neutrino mixing angle $\theta_{13}$ with the Double Chooz detector, Y. Abe et al. (Double Chooz), JHEP 1410 (2014) 86, arXiv:1406.7763.
[Abe:2014bwa]
[9-14]
Independent Measurement of $\vartheta_{13}$ via Neutron Capture on Hydrogen at Daya Bay, F. P. An et al. (Daya Bay), Phys. Rev. D90 (2014) 071101, arXiv:1406.6468.
[An:2014ehw]
[9-15]
Precise Measurement of the Neutrino Mixing Parameter $\theta_{23}$ from Muon Neutrino Disappearance in an Off-axis Beam, K. Abe et al. (T2K), Phys. Rev. Lett. 112 (2014) 181801, arXiv:1403.1532.
[Abe:2014ugx]
[9-16]
Combined analysis of $\nu_{\mu}$ disappearance and $\nu_{\mu} \rightarrow \nu_{e}$ appearance in MINOS using accelerator and atmospheric neutrinos, P. Adamson et al. (MINOS), Phys. Rev. Lett. 112 (2014) 191801, arXiv:1403.0867.
[Adamson:2014vgd]
[9-17]
Background-independent measurement of $\theta_{13}$ in Double Chooz, Y. Abe et al. (Double Chooz), Phys.Lett. B735 (2014) 51-56, arXiv:1401.5981.
[Abe:2014lus]
[9-18]
Evidence for $\nu_\mu\to\nu_\tau$ appearance in the CNGS neutrino beam with the OPERA experiment, N. Agafonova et al. (OPERA), Phys. Rev. D89 (2014) 051102, arXiv:1401.2079.
[Agafonova:2014bcr]
[9-19]
Observation of Electron Neutrino Appearance in a Muon Neutrino Beam, K. Abe et al. (T2K), Phys. Rev. Lett. 112 (2014) 061802, arXiv:1311.4750.
[Abe:2013hdq]
[9-20]
Spectral measurement of electron antineutrino oscillation amplitude and frequency at Daya Bay, F.P. An et al. (Daya Bay), Phys. Rev. Lett. 112 (2014) 061801, arXiv:1310.6732.
[An:2013zwz]
[9-21]
New results on $\nu_\mu \to \nu_\tau$ appearance with the OPERA experiment in the CNGS beam, N. Agafonova et al. (OPERA), JHEP 1311 (2013) 036, arXiv:1308.2553.
[Agafonova:2013dtp]
[9-22]
Measurement of Neutrino Oscillation Parameters from Muon Neutrino Disappearance with an Off-axis Beam, K. Abe et al. (T2K), Phys. Rev. Lett. 111, 211803 (2013) 211803, arXiv:1308.0465.
[Abe:2013fuq]
[9-23]
Search for anomalies in the $\nu_e$ appearance from a $\nu_\mu$ beam, M. Antonello et al. (ICARUS), Eur.Phys.J. C73 (2013) 2599, arXiv:1307.4699.
[Antonello:2013gut]
[9-24]
Measurement of Neutrino and Antineutrino Oscillations Using Beam and Atmospheric Data in MINOS, P. Adamson et al. (MINOS), Phys. Rev. Lett. 110 (2013) 251801, arXiv:1304.6335.
[Adamson:2013whj]
[9-25]
Evidence of Electron Neutrino Appearance in a Muon Neutrino Beam, K. Abe et al. (T2K), Phys. Rev. D88 (2013) 032002, arXiv:1304.0841.
[Abe:2013xua]
[9-26]
Search for $\nu_\mu\to\nu_e$ oscillations with the OPERA experiment in the CNGS beam, N. Agafonova et al. (OPERA), JHEP 1307 (2013) 004, arXiv:1303.3953.
[Agafonova:2013xsk]
[9-27]
Electron neutrino and antineutrino appearance in the full MINOS data sample, P. Adamson et al. (MINOS), Phys. Rev. Lett. 110 (2013) 171801, arXiv:1301.4581.
[Adamson:2013ue]
[9-28]
First Measurement of $\theta_{13}$ from Delayed Neutron Capture on Hydrogen in the Double Chooz Experiment, Y. Abe et al. (Double Chooz), Phys.Lett. B723 (2013) 66-70, arXiv:1301.2948.
[Abe:2013sxa]
[9-29]
Improved Measurement of Electron Antineutrino Disappearance at Daya Bay, F. P. An et al. (Daya Bay), Chin. Phys. C37 (2013) 011001, arXiv:1210.6327.
[An:2012bu]
[9-30]
Experimental search for the LSND anomaly with the ICARUS detector in the CNGS neutrino beam, M Antonello, B Baibussinov, P Benetti, E Calligarich, N Canci et al. (ICARUS), Eur.Phys.J. C73 (2013) 2345, arXiv:1209.0122.
[Antonello:2012pq]
[9-31]
Observation of Reactor Electron Antineutrino Disappearance in the RENO Experiment, Soo-Bong Kim et al. (RENO), Phys. Rev. Lett. 108 (2012) 191802, arXiv:1204.0626.
[Ahn:2012nd]
[9-32]
Demonstration of Communication using Neutrinos, D.D. Stancil et al., Mod. Phys. Lett. A27 (2012) 1250077, arXiv:1203.2847.
[Stancil:2012yc]
[9-33]
Observation of electron-antineutrino disappearance at Daya Bay, F. P. An et al. (Daya Bay), Phys. Rev. Lett. 108 (2012) 171803, arXiv:1203.1669.
[An:2012eh]
[9-34]
A side-by-side comparison of Daya Bay antineutrino detectors, F. P. An et al. (Daya Bay), Nucl. Instrum. Meth. A685 (2012) 78-97, arXiv:1202.6181.
[DayaBay:2012aa]
[9-35]
An improved measurement of muon antineutrino disappearance in MINOS, P. Adamson et al. (MINOS), Phys. Rev. Lett. 108 (2012) 191801, arXiv:1202.2772.
[Adamson:2012rm]
[9-36]
Search for Lorentz invariance and CPT violation with muon antineutrinos in the MINOS Near Detector, P. Adamson et al. (MINOS), Phys. Rev. D85 (2012) 031101, arXiv:1201.2631.
[Adamson:2012hp]
[9-37]
First Muon-Neutrino Disappearance Study with an Off-Axis Beam, K. Abe et al. (T2K), Phys. Rev. D85 (2012) 031103, arXiv:1201.1386.
[Abe:2012gx]
[9-38]
Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment, Y. Abe et al. (DOUBLE-CHOOZ), Phys. Rev. Lett. 108 (2012) 131801, arXiv:1112.6353.
[Abe:2011fz]
[9-39]
Search for the disappearance of muon antineutrinos in the NuMI neutrino beam, P. Adamson et al. (MINOS), Phys. Rev. D84 (2011) 071103, arXiv:1108.1509.
[Adamson:2011ch]
[9-40]
Improved search for muon-neutrino to electron-neutrino oscillations in MINOS, P. Adamson et al. (MINOS), Phys. Rev. Lett. 107 (2011) 181802, arXiv:1108.0015.
[Adamson:2011qu]
[9-41]
Search for $\nu_{\mu}\to\nu_{\tau}$ oscillation with the OPERA experiment in the CNGS beam, N. Agafonova et al. (OPERA), arXiv:1107.2594, 2011.
[OPERA:2011oja]
[9-42]
Indication of Electron Neutrino Appearance from an Accelerator-produced Off-axis Muon Neutrino Beam, K. Abe et al. (T2K), Phys. Rev. Lett. 107 (2011) 041801, arXiv:1106.2822.
[Abe:2011sj]
[9-43]
Active to sterile neutrino mixing limits from neutral-current interactions in MINOS, P. Adamson et al. (MINOS), Phys. Rev. Lett. 107 (2011) 011802, arXiv:1104.3922.
[Adamson:2011ku]
[9-44]
First direct observation of muon antineutrino disappearance, P. Adamson et al. (MINOS), Phys. Rev. Lett. 107 (2011) 021801, arXiv:1104.0344.
[Adamson:2011fa]
[9-45]
Measurement of the neutrino mass splitting and flavor mixing by MINOS, P. Adamson et al. (MINOS), Phys. Rev. Lett. 106 (2011) 181801, arXiv:1103.0340.
[Adamson:2011ig]
[9-46]
A Search for Lorentz Invariance and CPT Violation with the MINOS Far Detector, P. Adamson et al. (MINOS), Phys. Rev. Lett. 105 (2010) 151601, arXiv:1007.2791.
[Adamson:2010rn]
[9-47]
Observation of a first $\nu_\tau$ candidate in the OPERA experiment in the CNGS beam, N. Agafonova et al. (OPERA), Phys. Lett. B691 (2012) 138-145, arXiv:1006.1623.
[Efthymiopoulos:2012wfa]
[9-48]
New constraints on muon-neutrino to electron-neutrino transitions in MINOS, P. Adamson et al. (MINOS), Phys. Rev. D82 (2010) 051102, arXiv:1006.0996.
[Adamson:2010uj]
[9-49]
Search for sterile neutrino mixing in the MINOS long- baseline experiment, P. Adamson et al. (The MINOS), Phys. Rev. D81 (2010) 052004, arXiv:1001.0336.
[Adamson:2010wi]
[9-50]
Search for active neutrino disappearance using neutral-current interactions in the MINOS long-baseline experiment, P. Adamson et al. (MINOS), Phys. Rev. Lett. 101 (2008) 221804, arXiv:0807.2424.
[Adamson:2008jh]
[9-51]
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.
[Adamson:2008zt]
[9-52]
A Study of Muon Neutrino Disappearance Using the Fermilab Main Injector Neutrino Beam, P. Adamson et al. (MINOS), Phys. Rev. D77 (2008) 072002, arXiv:0711.0769.
From the abstract: We report the results of a search for $\nu_{\mu}$ disappearance by the Main Injector Neutrino Oscillation Search [9-55]. 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 $ 336 \pm 14 $ $\nu_{\mu}$ 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 $ \Delta{m}^{2} = 2.74 {}^{+0.44}_{-0.26} \times 10^{-3} \, \text{eV}^{2} $ and $ \sin^2 2\vartheta > 0.87 $ at 68\% confidence level.
[Adamson:2007gu]
[9-53]
First CNGS events detected by LVD, N. Yu. Agafonova et al., Eur. Phys. J. C52 (2007) 849-855, arXiv:0710.1536.
[Agafonova:2007sd]
[9-54]
First events from the CNGS neutrino beam detected in the OPERA experiment, R. Acquafredda et al. (OPERA), New J. Phys. 8 (2006) 303, arXiv:hep-ex/0611023.
[Acquafredda:2006ki]
[9-55]
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 $ |\Delta m^2_{23}| = 2.74 {}^{+0.44}_{-0.26} \times 10^{-3} \, \text{eV}^2/c^4 $ and $ sin^2(2\theta_{23}) > 0.87 $ (68% C.L.).
[Michael:2006rx]
[9-56]
Measurement of neutrino oscillation by the K2K experiment, M. H. Ahn et al. (K2K), Phys. Rev. D74 (2006) 072003, arXiv:hep-ex/0606032.
[Ahn:2006zza]
[9-57]
An improved search for $ \nu_\mu \to \nu_e $ 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 $ \Delta{m}^2 = 2.8 \times 10^{-3} \, \text{eV}^2 $, the best fit value of the K2K $\nu_\mu$ disappearance analysis, we set an upper limit of $ \sin^2 2\theta_{\mu e} < 0.13 $ at 90\% confidence level.
[Yamamoto:2006ty]
[9-58]
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.
[Aliu:2004sq]
[9-59]
Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion, T. Araki et al. (KamLAND), Phys. Rev. Lett. 94 (2005) 081801, arXiv:hep-ex/0406035.
[Araki:2004mb]
[9-60]
Search for electron neutrino appearance in a 250-km long- baseline experiment, M. H. Ahn et al. (K2K), Phys. Rev. Lett. 93 (2004) 051801, arXiv:hep-ex/0402017.
[Ahn:2004te]
[9-61]
Search for neutrino oscillations on a long base-line at the CHOOZ nuclear power station, M. Apollonio et al. (CHOOZ), Eur. Phys. J. C27 (2003) 331, arXiv:hep-ex/0301017.
Comment: The (new) results obtained by using the prescription of Feldman and Cousins with the correct inclusion of systematics indicate that $\bar{\nu}_e \to \bar{\nu}_x$ oscillations are excluded for mixing angles $\sin^2 2 \vartheta \geq 0.16 $ at high $\Delta m^2$ values. The limit obtained here is significantly higher than the one quoted in previous publication : ($\sin^2 2 \vartheta \geq 0.10 $ at high $\Delta m^2$ values). (M.L.).
[Apollonio:2002gd]
[9-62]
First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 90 (2003) 021802, arXiv:hep-ex/0212021.
From the abstract: In an exposure of 162 ton$\cdot$yr (145.1 days) the ratio of the number of observed inverse $\beta$-decay events to the expected number of events without disappearance is $0.611\pm 0.085 {\rm (stat)} \pm 0.041 {\rm (syst)} $ for $\bar{\nu}_e$ energies $>$ 3.4 MeV. The deficit of events is inconsistent with the expected rate for standard $\bar{\nu}_e$ propagation at the 99.95% confidence level. In the context of two-flavor neutrino oscillations with CPT invariance, these results exclude all oscillation solutions but the 'Large Mixing Angle' solution to the solar neutrino problem using reactor $\bar{\nu}_e$ sources.
[Eguchi:2002dm]
[9-63]
Indications of Neutrino Oscillation in a 250 km Long- baseline Experiment, M. H. Ahn 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 $\nu_\mu$ 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 $80.1^{+6.2}_{-5.4}$.
From the article: Best Fit: $ \Delta{m}^2 = 2.8 \times 10^{-3} \, \mathrm{eV}^2 $, $ \sin^22\vartheta = 1.0 $.... 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 $10^{20}$ protons on target.
[Ahn:2002up]
[9-64]
Detection of accelerator produced neutrinos at a distance of 250-km, S. H. Ahn et al. (K2K), Phys. Lett. B511 (2001) 178-184, arXiv:hep-ex/0103001.
[Ahn:2001cq]

10 - Experiment - Neutrino Oscillations - Conference Proceedings

[10-1]
First Antineutrino Oscillation Results from T2K, Kirsty Duffy, arXiv:1605.01626, 2016. NuPhys2015 (London, 16-18 December 2015).
[Duffy:2016iar]
[10-2]
Neutrino Oscillations with MINOS and MINOS+, Leigh H. Whitehead (MINOS), Nucl. Phys. B908 (2016) 130-150, arXiv:1601.05233.
[Whitehead:2016xud]
[10-3]
Latest nH analysis in the Double Chooz experiment, Guang Yang (Double Chooz), arXiv:1511.00068, 2015. DPF 2015 Meeting of the American Physical Society Division of Particles and Fields, Ann Arbor, Michigan, August 4-8, 2015.
[Yang:2015nwf]
[10-4]
Current status of the T2K experiment, Yuichi Oyama (T2K), PoS PLANCK2015 (2015) 094, arXiv:1510.07200. 18th International Conference From the Planck Scale to the Electroweak Scale (Planck2015), Ioannina, Greece, May 25-29, 2015.
[Oyama:2015vea]
[10-5]
First Results of $\nu_e$ Appearance Analysis and Electron Neutrino Identification at NOvA, Jianming Bian (NOvA), arXiv:1510.05708, 2015. DPF 2015 Meeting of the American Physical Society Division of Particles and Fields, Ann Arbor, Michigan, August 4-8, 2015.
[Bian:2015opa]
[10-6]
Search for Sterile Neutrinos at OPERA and other Long-Baseline Experiments, Luca Stanco, PoS EPS-HEP2015 (2016) 057, arXiv:1510.04151. EPS2015, Vienna 22-29 July 2015.
[Stanco:2015sua]
[10-7]
OPERA neutrino oscillation search: status and perspectives, Giuliana Galati (OPERA), arXiv:1510.00343, 2015. CIPANP2015.
[Galati:2015ona]
[10-8]
First muon anti-neutrino disappearance oscillation results from T2K, Blair Jamieson (T2K), arXiv:1509.08889, 2015. CIPANP2015.
[Jamieson:2015rza]
[10-9]
Anti-neutrino oscillations with T2K, M. Ravonel Salzgeber (T2K), arXiv:1508.06153, 2015. EPS-HEP 2015.
[Salzgeber:2015gua]
[10-10]
Results from the MINOS Experiment and New MINOS+ Data, A. Holin (MINOS+), PoS NUFACT2014 (2014) 028, arXiv:1507.08564. 2014 NuFact.
[Holin:2015lya]
[10-11]
Recent Results from Daya Bay, Liang Zhan (Daya Bay), PoS NEUTEL2015 (2015) 017, arXiv:1506.01149. NEUTEL 2015.
[Zhan:2015aha]
[10-12]
Recent Results from Daya Bay Reactor Neutrino Experiment, Bei-Zhen Hu (Daya Bay), arXiv:1505.03641, 2015. Moriond 2015 EW Session.
[Hu:2015gva]
[10-13]
Recent Results From The Daya Bay Experiment, Chao Zhang (Daya Bay), AIP Conf. Proc. 1666 (2015) 080003, arXiv:1501.04991. Neutrino 2014, 2-7 June 2014, Boston, Massachusetts, USA.
[Zhang:2015fya]
[10-14]
Results from T2K, Martin David Haigh, arXiv:1501.04283, 2015. Interplay between Particle and Astroparticle Physics (IPA 2014), 18-22 August 2014 Queen Mary University of London.
[Haigh:2015uja]
[10-15]
Results from MINOS and NOvA, C Backhouse, J. Phys. Conf. Ser. 598 (2015) 012004, arXiv:1501.01016. NuPHYS 2013.
[Backhouse:2015nga]
[10-16]
Operational Status and Power Upgrade Prospects of the Neutrino Experimental Facility at J-PARC, Taku Ishida (T2K Beam Group), JPS Conf. Proc. 8 (2015) 023012, arXiv:1411.5540. 2nd international symposium on science at J-PARC (J-PARC 2014), Tsukuba, Ibaraki, Japan on July 2014.
[Ishida:2014uxa]
[10-17]
New Results from RENO and The 5 MeV Excess, Seon-Hee Seo (RENO), AIP Conf. Proc. 1666 (2015) 080002, arXiv:1410.7987. Neutrino 2014.
[Seon-HeeSeofortheRENO:2014jza]
[10-18]
Opera Highlights, Thomas Strauss (OPERA), Acta Polytech. 53 (2013) 512-517, arXiv:1405.6847. 2012 Volcano Workshop: Frontier Objects in Astrophysics and Particle Physics.
[Strauss:2014qna]
[10-19]
Oscillation results from T2K, Patrick de Perio (T2K), arXiv:1405.3871, 2014. Rencontres de Moriond Electroweak Interactions and Unified Theories Conference 2014.
[dePerio:2014zna]
[10-20]
Double Chooz: results towards the near detector phase, P. Novella (Double Chooz), arXiv:1405.3816, 2014. Rencontres de Moriond 2014.
[Novella:2014wna]
[10-21]
The Status of Double Chooz Experiment as a proceeding of PIC 2013 conference, Guang Yang (Double Chooz), arXiv:1403.6989, 2014.
[Yang:2014fua]
[10-22]
New Results from the Daya Bay Reactor Neutrino Experiment, Bei-Zhen Hu (Daya Bay), arXiv:1402.6439, 2014. 10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
[Hu:2014tia]
[10-23]
Search for Neutrino Oscillations in Appearance Mode with the OPERA Experiment, T. A. Dzhatdoev, V. L. Troshina (OPERA), arXiv:1402.3861, 2014. HEPFT-2013.
[Dzhatdoev:2014qsa]
[10-24]
Recent results of the OPERA experiment, Fabio Pupilli (OPERA), arXiv:1401.6776, 2014. 14th ICATPP Conference, 23-27 September 2013, Villa Olmo - Como (Italy).
[Pupilli:2014xua]
[10-25]
New Results from the T2K Experiment: Observation of $\nu_e$ Appearance in a $\nu_\mu$ Beam, Michael Wilking (T2K), PoS EPS-HEP2013 (2013) 536, arXiv:1311.4114. EPS-HEP 2013.
[Wilking:2013vza]
[10-26]
Systematic Uncertainties at the T2K Experiment for Oscillation Measurements, A. Kaboth (T2K), arXiv:1310.6544, 2013. NuFact2013.
[Kaboth:2013gcw]
[10-27]
The NOvA Experiment: Overview and Status, Jianming Bian, arXiv:1309.7898, 2013. DPF 2013 Meeting of the American Physical Society Division of Particles and Fields, Santa Cruz, California, August 13-17, 2013.
[Bian:2013saa]
[10-28]
Rate-Only analysis with reactor-off data in the Double Chooz experiment, P. Novella (Double Chooz), arXiv:1305.2734, 2013.
[Novella:2013mca]
[10-29]
Study of Neutrino Oscillations in the OPERA Experiment, Umut Kose (OPERA), arXiv:1305.2513, 2013. Lake Louise Winter 2013 Conference, Banff, Alberta, Canada, 17-23 February 2013.
[Kose:2013jca]
[10-30]
The Improved Measurement of Electron-antineutrino Disappearance at Daya Bay, Daniel A. Dwyer (Daya Bay), Nucl. Phys. Proc. Suppl. 235-236 (2013) 30-32, arXiv:1303.3863. 25th International Conference on Neutrino Physics and Astrophysics (Neutrino 2012), Jun. 3-9, 2012, Kyoto, Japan.
[Dwyer:2013wqa]
[10-31]
An Improved Measurement of Electron Antineutrino Disappearance at Daya Bay, David M. Webber (Daya Bay), Nucl. Phys. Proc. Suppl. 233 (2012) 96-101, arXiv:1211.1609. BEACH 2012.
[Webber:2012vh]
[10-32]
Improved Measurement of Electron Antineutrino Disappearance at Daya Bay, Xin Qian (Daya Bay), arXiv:1211.0570, 2012. NuFact 2012.
[Qian:2012df]
[10-33]
First result from the Double Chooz reactor-neutrino experiment, Tsunayuki Matsubara (Double Chooz), arXiv:1205.6685, 2012. 47th Rencontres de Moriond EW session.
[Matsubara:2012uh]
[10-34]
New Results from the MINOS Experiment, Anna Holin (MINOS), PoS EPS-HEP2011 (2011) 088, arXiv:1201.3645. EPS 2011.
[Holin:2012np]
[10-35]
First Oscillation Results for the T2K Experiment, Mark Hartz (T2K), arXiv:1201.1846, 2012. Recontres de Moriond EW 2011.
[Hartz:2012np]
[10-36]
New Oscillation Results from the T2K experiment, Alexander Izmaylov (T2K), arXiv:1112.0273, 2011. 15th Lomonosov Conference, August 18-24, 2011, MSU, Moscow, Russia.
[Izmaylov:2011np]
[10-37]
Latest oscillation results from T2K, Marat Khabibullin (T2K), arXiv:1111.0183, 2011. New Trends in High-Energy Physics, Alushta, Crimea, Ukraine, September 3-10, 2011.
[Khabibullin:2011dt]
[10-38]
T2K Results and Future Plans, Francesca Di Lodovico (T2K), J. Phys. Conf. Ser. 408 (2013) 012004, arXiv:1110.5382. NUFACT 11, XIIIth International Workshop on Neutrino Factories, Super beams and Beta beams, 1-6 August 2011, CERN and University of Geneva.
[DiLodovico:2011gx]
[10-39]
MINOS Search for Sterile Neutrinos, Alexandre Sousa (MINOS), J. Phys. Conf. Ser. 408 (2013) 012026, arXiv:1110.3455. NuFact 2011.
[Sousa:2011rw]
[10-40]
ICARUS and Status of Liquid Argon Technology, Dorota Stefan (ICARUS), J. Phys. Conf. Ser. 408 (2013) 012078, arXiv:1110.1652.
[Stefan:2011ca]
[10-41]
Search for Electron Neutrino Appearance in MINOS, Mhair Orchanian (MINOS), arXiv:1109.6795, 2011. 2011 DPF.
[Orchanian:2011qq]
[10-42]
Latest News from Double Chooz Reactor Neutrino Experiment, Masahiro Kuze (Double Chooz), AIP Conf. Proc. 1441 (2012) 461-463, arXiv:1109.0074. 19th Particles and Nuclei International Conference, PANIC 2011, MIT, Cambridge, MA July 2011.
[Kuze:2011ic]
[10-43]
Current status of the T2K experiment, Yuichi Oyama, T2K (T2K), J. Phys. Conf. Ser. 347 (2012) 012005, arXiv:1108.4457. 2nd International Conference on Particle Physics (ICPP-Istanbul II),Istanbul, Turkey, June 20-25, 2011.
[Oyama:2011pt]
[10-44]
Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment, Umut Kose, arXiv:1106.3871, 2011. Les Rencontres de Physique de la Vall\'ee D'Aoste (La Thuile, February 27-March 5 2011).
[Kose:2011qw]
[10-45]
Search for $\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode in the OPERA experiment, L. S. Esposito (OPERA), arXiv:1105.5239, 2011. WIN'11, Cape Town, South Africa, 31 January - 5 February 2011.
[Esposito:2011as]
[10-46]
Status of the Daya Bay Reactor Neutrino Oscillation Experiment, Cheng-Ju Lin (Daya Bay), PoS ICHEP2010 (2010) 305, arXiv:1101.0261. 35th International Conference of High Energy Physics, July 22-28, 2010, Paris, France.
[Lin:2011pb]
[10-47]
Electron Neutrinos at T2K, Melissa George (T2K), arXiv:1006.1245, 2010.
[George:2010xk]
[10-48]
The OPERA experiment: a direct search of the $\nu_\mu \longrightarrow \nu_\tau$ oscillations, J. Marteau, arXiv:0910.3468, 2009. 11th ICATPP Conference, Villa Olmo, Como, Italy, 5-9 October 2009.
[Marteau:2009rj]
[10-49]
First Observation of Accelerator Muon Antineutrinos in MINOS, Istvan Danko (MINOS), arXiv:0910.3439, 2009. DPF-2009 conference, Detroit, MI, July 27-31, 2009, eConf C090726.
[Danko:2009qw]
[10-50]
Analysis of Neutral Current Interactions in MINOS: A Search for Sterile Neutrinos, Alexandre Sousa (MINOS), arXiv:0910.1369, 2009. DPF-2009, Detroit, MI, July 2009.
[Sousa:2009wp]
[10-51]
The OPERA experiment: on the way to the direct observation of $\nu_\mu \to \nu_\tau$ oscillation, M. De Serio (OPERA), arXiv:0910.0337, 2009. DPF-2009, Detroit, MI, July 2009.
[DeSerio:2009vt]
[10-52]
Initial Results for Electron-Neutrino Appearance in MINOS, Mayly C. Sanchez (MINOS), arXiv:0909.2362, 2009. Rencontres de Moriond EW 2009.
[Sanchez:2009nb]
[10-53]
A High Precision Reactor Neutrino Detector for the Double Chooz Experiment, Fumihiko Suekane (Double Chooz), Nucl. Instrum. Meth. A623 (2010) 440-441, arXiv:0906.1639. TIPP09.
[Suekane:2009fy]
[10-54]
Status of the Double Chooz Experiment, J. V. Dawson (Double Chooz), arXiv:0905.4843, 2009. XIII International Workshop on Neutrino Telescopes (NEUTEL09), Venice, March 10-13, 2009.
[Dawson:2009nea]
[10-55]
The OPERA experiment: Preliminary results from the 2008 run, Guillaume Lutter, arXiv:0905.4521, 2009. Lake Louise Winter Institute 2009.
[Lutter:2009ce]
[10-56]
Status Report on Double Chooz, A. Porta et al. (Double Chooz), arXiv:0905.2560, 2009. 44th Rencontres de Moriond, Electroweak interactions and unified theories, 7-14 March 2009, La Thuile.
[Porta:2009sp]
[10-57]
Recent Results from the MINOS experiment, Milind V. Diwan, arXiv:0904.3706, 2009. XIII International Workshop on Neutrino Telescopes, March 10-13, 2009.
[Diwan:2009pn]
[10-58]
Recent Results and Future Prospects from MINOS, Jonathan M. Paley (MINOS), arXiv:0901.2131, 2009. PANIC 2008.
[Paley:2009sd]
[10-59]
Neutrino Oscillation Studies with MINOS, Patricia Vahle (MINOS), arXiv:0810.3627, 2008. 34th International Conference on High Energy Physics (ICHEP 2008), Philadelphia, Pennsylvania, 30 Jul - 5 Aug 2008.
[Vahle:2008qt]
[10-60]
New Results from the MINOS Experiment, Hugh Gallagher (MINOS), J. Phys. Conf. Ser. 136 (2008) 022014, arXiv:0809.5240. Neutrino 2008 Conference, Christchurch, NZ.
[Gallagher:2008tk]
[10-61]
Neutrino Oscillation Results from MINOS and MiniBooNE, Tobias M. Raufer, arXiv:0808.0392, 2008. Flavor Physics and CP Violation Conference, Taipei, 2008 (FPCP 2008).
[Raufer:2008aa]
[10-62]
Current NuMI/MINOS Oscillation Results, A. Habig (MINOS), arXiv:0805.2317, 2008. Moriond Electroweak conference, March 1-8 2008.
[Habig:2008ee]
[10-63]
Neutrino Spectra and Uncertainties for MINOS, Sacha E. Kopp (MINOS), AIP Conf. Proc. 981 (2008) 142-144, arXiv:0712.1280. NuFact07 (Okayama, Japan).
[Kopp:2007cx]
[10-64]
Preliminary Results from MINOS on Muon Neutrino Disappearance Based on an Exposure of 2.5x1020 120 GeV Protons on the NuMI Target, MINOS (MINOS), arXiv:0708.1495, 2007. XXIII International Symposium on Lepton and Photon Interactions at High Energy, Daegu Korea, August 13-18, 2007.
[MINOS:2007aa]
[10-65]
MINOS Results, Progress and Future Prospects, Tobias M. Raufer (MINOS), arXiv:0705.4655, 2007. XLIInd Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, March 2007.
[Raufer:2007iw]
[10-66]
First MINOS Results with the NuMI Beam, Brian J. Rebel et al. (MINOS), Nucl. Phys. Proc. Suppl. 168 (2007) 195-198, arXiv:hep-ex/0701049. Neutrino Oscillation Workshop 2006.
[Rebel:2007ex]
[10-67]
Recent results from the MINOS experiment, Mary Bishai (MINOS), AIP Conf. Proc. 903 (2007) 271-274.
[Bishai:2007zz]
[10-68]
The Opera Experiment, G. Giacomelli, M. Giorgini (OPERA), arXiv:physics/0609045, 2006. Vulcano Workshop 2006, Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May 2006.
[Giacomelli:2006xn]
[10-69]
First MINOS Results from the NuMI Beam, Nathaniel Tagg et al. (MINOS), eConf C060409 (2006) 019, arXiv:hep-ex/0605058. Flavor Physics and CP Violation Conference, Vancouver, 2006.
[Tagg:2006sx]
[10-70]
Results from K2K and status of T2K, Yuichi Oyama, arXiv:hep-ex/0512041, 2005. International Conference on New Trends in High-Energy Physics (Crimea2005), Yalta, Ukraine, September 10-17, 2005.
[Oyama:2005mi]
[10-71]
The NuMI Neutrino Beam at Fermilab, Sacha E. Kopp, arXiv:physics/0508001, 2005. U.S. Particle Accelerator Conference, Knoxville, TN (May 2005).
[Kopp:2005bt]
[10-72]
Recent Results from K2K Experiment, C. Mariani (K2K), arXiv:hep-ex/0505019, 2005. 2005 Electroweak session, XXXXth Rencontres de Moriond.
[Mariani:2005pj]
[10-73]
HARP Experiment Results and K2K Flux, M. Sorel (Harp), 2005. 5th International Workshop on Neutrino Beams and Instrumentation,July 7-11, 2005, Fermilab, Batavia Illinois. http://www.hep.utexas.edu/nbi2005/transparencies/beamMChadprod/sorel-HARP-results.pdf.
[Sorel:NBI2005]
[10-74]
Recent K2K Results, Takanobu Ishii (K2K), arXiv:hep-ex/0406055, 2004. 5th Workshop on Neutrino Oscillations and their Origin (NOON2004), Tokyo, Japan, February 11-15,2004.
[Ishii:2004wu]
[10-75]
Recent results from K2K, Taiki Iwashita, arXiv:hep-ex/0406051, 2004. XXXIXth Rencontres de Moriond session devoted to Electroweak Interactions and Unified Theories.
[Iwashita:2004sx]
[10-76]
K2K results, T. Iwashita (K2K), 2004. XXXIX Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, 21-28 March 2003. http://moriond.in2p3.fr/EW/2004/transparencies/3_Wednesday/3_2_afternoon/3_2_4_Iwashita/Iwashita.pdf.
[Iwashita:Moriond2004]
[10-77]
Results from the KamLAND experiment, G. Gratta (KamLAND), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/gratta.pdf.
[Gratta-Nu2004]
[10-78]
KamLAND: updated results, K. Inoue, 2004. Neutrino Oscillation Workshop NOW 2004, September 11-17, 2004, Conca Specchiulla (Otranto, Italy). http://www.ba.infn.it/~now2004/talks/12_09_04/plen/KamLAND.pdf.
[Inoue:2004]
[10-79]
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.
[Nakaya-Nu2004]
[10-80]
The Results of Oscillation Analysis in K2K Experiment And An Overview of JHFnu Experiment, I. Kato (K2K), arXiv:hep-ex/0306043, 2003. XXXVIIIth Recontres de Moriond on Electroweak Interaction and Unified Theories, Les Arcs, France, March 15-22, 2003.
[Kato:2003qx]
[10-81]
KamLAND Results, K. Inoue, 2003. The 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/Inoue-KamLAND.pdf.
[Inoue:NOON2003]
[10-82]
Status of the Super-Kamiokande, the K2K-2 experiment and JHF nu project, Y. Hayato, 2003. EPS2003. http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07Hayato.ppt.
[Hayato:EPS2003]
[10-83]
New Results from Super-K and K2K, R. Jeffrey Wilkes (K2K), eConf C020805 (2002) TTH02, arXiv:hep-ex/0212035. Secrets of the B-Meson, Topical Conference, XXX SLAC Summer Institute, SLAC, August, 2002.
[Wilkes:2002mb]
[10-84]
Recent Results from the K2K Experiment, C. W. Walter (K2K), eConf C0209101 (2002) TH03, arXiv:hep-ex/0211059. Seventh International Workshop on Tau Lepton Physics (TAU02), Santa Cruz, Ca, USA, Sept 2002.
[Walter:2002wh]
[10-85]
Present Status of the K2K Experiment, Yuichi Oyama (K2K), arXiv:hep-ex/0210030, 2002. 3rd Conference on Physics beyond the Standard Model - BEYOND THE DESERT 02 - Oulu, Finland, 2-7 June 2002. http://cupp.oulu.fi/trans/Oyama.pdf.
[Oyama:2002hu]
[10-86]
New Results from K2K, Takanobu Ishii (K2K), arXiv:hep-ex/0206033, 2002. Les Rencontres de Physique de la Vallee d'Aoste, La Thuile, Aosta Valley, Italy, March 3-9, 2002. http://www.pi.infn.it/lathuile/2002/talks/ishii.pdf.
[Ishii:2002ez]
[10-87]
An update on progress at KamLAND, S. A. Dazeley (KamLAND), arXiv:hep-ex/0205041, 2002.
[Dazeley:2002yf]
[10-88]
First Results from KamLAND: Evidence for $\bar{\nu}_e$ disappearance, G. Gratta (Kamland), 2002. SLAC Colloquium, December 2002. http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.
[Gratta:SLAC2002]
[10-89]
KamLAND: Examination of the LMA solution with reactor neutrinos, A. Suzuki (Kamland), 2002. XVI International Conference on Particles and Nuclei, Osaka, Japan, September 30 - October 4, 2002. http://www.rcnp.osaka-u.ac.jp/Divisions/np2/PaNic02/Suzuki.pdf.
[Suzuki-Panic02]
[10-90]
K2K Results, K. Nishikawa (K2K), 2002. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/nishikawa.
[Nishikawa-Nu2002]

11 - Experiment - Neutrino Oscillations - Slides

[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.
[Blake-TAUP2007]

12 - Experiment - Muons

[12-1]
Measurement of TeV atmospheric muon charge ratio with the full OPERA data, N. Agafonova et al. (OPERA), Eur. Phys. J. C74 (2014) 2933, arXiv:1403.0244.
[Agafonova:2014mzx]
[12-2]
Measurement of the underground atmospheric muon charge ratio using the MINOS Near Detector, P. Adamson et al. (MINOS), Phys. Rev. D83 (2011) 032011, arXiv:1012.3391.
[Adamson:2010xf]
[12-3]
Observation in the MINOS far detector of the shadowing of cosmic rays by the sun and moon, P. Adamson et al. (MINOS), Astropart. Phys. 34 (2011) 457-466, arXiv:1008.1719.
[Adamson:2010hv]
[12-4]
Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector, J. A. Aguilar et al. (ANTARES), Astropart. Phys. 34 (2010) 179-184, arXiv:1007.1777.
[Aguilar:2010kg]
[12-5]
Measurement of the charge ratio of atmospheric muons with the CMS detector, CMS (CMS), Phys. Lett. B692 (2010) 83-104, arXiv:1005.5332.
[Khachatryan:2010mw]
[12-6]
Measurement of the atmospheric muon charge ratio with the OPERA detector, N. Agafonova et al. (OPERA), Eur. Phys. J. C67 (2010) 25-37, arXiv:1003.1907.
[Agafonova:2010fg]
[12-7]
Measurement of the atmospheric muon flux with a 4 GeV threshold in the ANTARES neutrino telescope, J. A. Aguilar et al. (Antares), Astropart. Phys. 33 (2010) 86-90, arXiv:0910.4843.
[collaboration:2009bw]
[12-8]
Measurement of the atmospheric muon flux with the NEMO Phase-1 detector, S. Aiello et al. (The NEMO), Astropart. Phys. 33 (2010) 263-273, arXiv:0910.1269.
[Aiello:2009uh]
[12-9]
Observation of muon intensity variations by season with the MINOS far detector, P. Adamson et al. (MINOS), Phys. Rev. D81 (2010) 012001, arXiv:0909.4012.
[Adamson:2009zf]
[12-10]
Time variations in the deep underground muon flux, S. Cecchini et al., Europhys. Lett. 87 (2009) 39001, arXiv:0907.5235.
[Cecchini:2009ug]
[12-11]
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.
[Carminati:2008qb]
[12-12]
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.
[Abdallah:2007fk]
[12-13]
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.
[Adamson:2007ww]
[12-14]
Measurements of integral muon intensity at large zenith angles, A.N. Dmitrieva et al., arXiv:hep-ex/0611051, 2006.
[Dmitrieva:2006aj]
[12-15]
Muon Flux at the Geographical South Pole, X. Bai et al., Astropart. Phys. 25 (2006) 361-367, arXiv:astro-ph/0602381.
[Bai:2006mf]
[12-16]
Flux of atmospheric muons: Comparison between AIRES simulations and CAPRICE98 data, P. Hansen, P. Carlson, E. Mocchiutti, S. J. Sciutto, M. Boezio, Phys. Rev. D68 (2003) 103001, arXiv:hep-ph/0307199.
[Hansen:2003rq]
[12-17]
Measurements of Proton, Helium and Muon Spectra at Small Atmospheric Depths with the BESS Spectrometer, K. Abe et al., Phys. Lett. B564 (2003) 8, arXiv:astro-ph/0304102.
[Abe:2003cd]
[12-18]
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.
[Ambrosio:2002id]
[12-19]
Measurements of atmospheric muon spectra at mountain altitude, T. Sanuki et al., Phys. Lett. B541 (2002) 234-242, arXiv:astro-ph/0205427.
[Sanuki:2002tp]
[12-20]
Precise measurements of atmospheric muon fluxes with the BESS spectrometer, M. Motoki et al., Astropart. Phys. 19 (2003) 113, arXiv:astro-ph/0205344.
[Motoki:2002nr]
[12-21]
Measurement of the flux of atmospheric muons with the CAPRICE94 apparatus, M. Boezio et al. (WiZard/CAPRICE), Phys. Rev. D62 (2000) 032007, arXiv:hep-ex/0004014.
[Boezio:2000bc]
[12-22]
Energy spectra, altitude profiles and charge ratios of atmospheric muons, S. Coutu et al., Phys. Rev. D62 (2000) 032001, arXiv:hep-ex/0004010.
[Coutu:2000qj]
[12-23]
Balloon measurements of cosmic ray muon spectra in the atmosphere along with those of primary protons and helium nuclei over mid-latitude, R. Bellotti et al. (WiZard/MASS2), Phys. Rev. D60 (1999) 052002, arXiv:hep-ex/9905012.
[Bellotti:1999pt]
[12-24]
A Measurement of the negative muon spectrum between 0.3- GeV/c and 40-GeV/c in the atmosphere, R. Bellotti et al., Phys. Rev. D53 (1996) 35-43.
[Bellotti:1995db]
[12-25]
Zenith-angle dependence of cosmic ray muons, H. E. Bergeson et al., Phys. Rev. Lett. 27 (1971) 160-163.
[Bergeson:1971zq]
[12-26]
Cosmic ray muon intensity deep underground versus depth, B. S. Meyer et al., Phys. Rev. D1 (1970) 2229-2244.
[Meyer:1970qi]

13 - Experiment - Muons - Conference Proceedings

[13-1]
Composition from high $p_\mathrm{T}$ muons in IceCube, D. Soldin (IceCube), EPJ Web Conf. 99 (2015) 06001, arXiv:1411.4448. International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2014).
[Soldin:2014ouk]
[13-2]
Observations of Large Scale Sidereal Anisotropy in 1 and 11 TeV cosmic rays from the MINOS experiment, J.K. de Jong (MINOS), arXiv:1201.2621, 2012. 32nd International Cosmic Ray Conference, August 2011.
[deJong:2012hk]
[13-3]
Measurement of the atmospheric muon flux with the ANTARES detector, Marco Bazzotti et al. (ANTARES), arXiv:0911.3055, 2009. 31st ICRC, Lodz 2009.
[Bazzotti:2009sy]
[13-4]
Direct Measurement of the Atmospheric Muon Energy Spectrum with IceCube, Patrick Berghaus (IceCube), arXiv:0909.0679, 2009. 31st ICRC, Lodz, Poland, July 2009.
[Berghaus:2009zk]
[13-5]
Large Scale Cosmic Ray Anisotropy With IceCube, Rasha Abbasi, Paolo Desiati, for the IceCube Collaboration (IceCube), Astrophys. J. 718 (2009) L194, arXiv:0907.0498. ICRC (2009).
[Abbasi:2009wm]
[13-6]
MINOS Observations of Shadowing in the Muon Flux Underground, E. W. Grashorn (MINOS), arXiv:0710.1617, 2007. 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007.
[Grashorn:2007tw]
[13-7]
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.
[Grashorn:2007tv]
[13-8]
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.
[Goodman:2007eg]
[13-9]
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.
[Schreiner:2007ef]
[13-10]
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.
[Unger:2003xd]

14 - Experiment - Gamma Rays

[14-1]
Atmospheric gamma-ray observation with the BETS detector for calibrating atmospheric neutrino flux calculations, K. Kasahara 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 [15-55] 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.
[Kasahara:2002ni]

15 - Neutrino Flux

[15-1]
$D$ - meson production at very forward rapidities: estimating the intrinsic charm contribution, F. Carvalho, A. V. Giannini, V. P. Goncalves, F. S. Navarra, arXiv:1701.08451, 2017.
[Carvalho:2017zge]
[15-2]
Uncertainties in Atmospheric Muon-Neutrino Fluxes Arising from Cosmic-Ray Primaries, Justin Evans, Diego Garcia Gamez, Salvatore Davide Porzio, Stefan Soldner-Rembold, Steven Wren, Phys. Rev. D95 (2017) 023012, arXiv:1612.03219.
[Evans:2016obt]
[15-3]
IC at IC: IceCube can constrain the intrinsic charm of the proton, Ranjan Laha, Stanley J. Brodsky, arXiv:1607.08240, 2016.
[Laha:2016dri]
[15-4]
Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects, Atri Bhattacharya et al., JHEP 1611 (2016) 167, arXiv:1607.00193.
[Bhattacharya:2016jce]
[15-5]
On the Charm Contribution to the Atmospheric Neutrino Flux, Francis Halzen, Logan Wille, Phys. Rev. D94 (2016) 014014, arXiv:1605.01409.
[Halzen:2016thi]
[15-6]
Lepton fluxes from atmospheric charm revisited, M.V. Garzelli, S. Moch, G. Sigl, JHEP 10 (2015) 115, arXiv:1507.01570.
[Garzelli:2015psa]
[15-7]
Measurements of cosmic-ray proton and helium spectra from the BESS-Polar long-duration balloon flights over Antarctica, K. Abe et al., Astrophys.J. 822 (2016) 65, arXiv:1506.01267.
[Abe:2015mga]
[15-8]
Atmospheric neutrino flux calculation using the NRLMSISE00 atmospheric model, M. Honda, M. Sajjad Athar, T. Kajita, K. Kasahara, S. Midorikawa, Phys. Rev. D92 (2015) 023004, arXiv:1502.03916.
[Honda:2015fha]
[15-9]
Perturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC, Atri Bhattacharya, Rikard Enberg, Mary Hall Reno, Ina Sarcevic, Anna Stasto, JHEP 1506 (2015) 110, arXiv:1502.01076.
[Bhattacharya:2015jpa]
[15-10]
A new contribution to the conventional atmospheric neutrino flux, Thomas K. Gaisser, Spencer R. Klein, Astropart.Phys. 64 (2014) 13-17, arXiv:1409.4924.
[Gaisser:2014pda]
[15-11]
High-energy neutrino fluxes and flavor ratio in the Earth atmosphere, T.S. Sinegovskaya, A.D. Morozova, S.I. Sinegovsky, Phys. Rev. D91 (2015) 063011, arXiv:1407.3591.
[Sinegovskaya:2014pia]
[15-12]
Atmospheric neutrino flux at INO, South Pole and Pyhasalmi, M. Sajjad Athar, M. Honda, T. Kajita, K. Kasahara, S. Midorikawa, Phys. Lett. B718 (2013) 1375-1380, arXiv:1210.5154.
[Athar:2012it]
[15-13]
Influence of hadronic interaction models and the cosmic ray spectrum on the high energy atmospheric muon and neutrino flux, Anatoli Fedynitch, Julia Becker Tjus, Paolo Desiati, Phys. Rev. D86 (2012) 114024, arXiv:1206.6710.
[Fedynitch:2012fs]
[15-14]
Improvement of low energy atmospheric neutrino flux calculation using the JAM nuclear interaction model, Morihiro Honda, Takaaki Kajita, Katsuaki Kasahara, Shoichi Midorikawa, Phys. Rev. D83 (2011) 123001, arXiv:1102.2688.
[Honda:2011nf]
[15-15]
Atmospheric lepton fluxes at very high energy, J.I. Illana, Paolo Lipari, M. Masip, D. Meloni, Astropart. Phys. 34 (2011) 663-673, arXiv:1010.5084.
[Illana:2010gh]
[15-16]
Atmospheric lepton fluxes at ultrahigh energies, J.I. Illana, M. Masip, D. Meloni, JCAP 0909 (2009) 008, arXiv:0907.1412.
[Illana:2009qv]
[15-17]
Prompt neutrino fluxes from atmospheric charm, Rikard Enberg, Mary Hall Reno, Ina Sarcevic, Phys. Rev. D78 (2008) 043005, arXiv:0806.0418.
[Enberg:2008te]
[15-18]
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.
[Honda:2006qj]
[15-19]
Uncertainties in Atmospheric Neutrino Fluxes, G.D. Barr, T.K. Gaisser, S. Robbins, T. Stanev, Phys. Rev. D74 (2006) 094009, arXiv:astro-ph/0611266.
[Barr:2006it]
[15-20]
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.
[Sanuki:2006yd]
[15-21]
Simulation of neutrino and charged particle production and propagation in the atmosphere, L. Derome, Phys. Rev. D74 (2006) 105002, arXiv:astro-ph/0607619.
[Derome:2006kg]
[15-22]
A semi-analytic calculation on the atmospheric tau neutrino flux due to $\nu_{\mu}\to \nu_{\tau}$ oscillations, Fei-Fan Lee, Guey-Lin Lin, Astropart. Phys. 25 (2006) 64, arXiv:hep-ph/0412383.
[Lee:2004zm]
[15-23]
Fluxes of Atmospheric Leptons at 600 GeV - 60 TeV, Dmitry Chirkin, arXiv:hep-ph/0407078, 2004.
[Chirkin:2004ic]
[15-24]
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 $\lesssim 10\%$ 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.
[Honda:2004yz]
[15-25]
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~[15-62], [15-53] to three dimensions. We compare results of the 3D and 1D calculations for neutrino energies from 100 MeV to 10 GeV over the full $4\pi$ 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 $E_\nu>1$~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 $E_\nu< 1$~GeV, which show a significant excess in the 3D calculation for $-0.1<\cos\theta< 0.1$ and a smaller deficit for $|\cos\theta|> 0.4$. 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 $E_\nu> 5$~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 $300< E_\nu< 500$~MeV by 15\% relative to the 1D calculation. The corresponding reduction decreases to 4\% for $E_\nu > 1$~GeV.

[Barr:2004br]
[15-26]
A 3-d simulation of the atmospheric neutrinos, J. Favier, R. Kossakowski, J. P Vialle, Phys. Rev. D68 (2003) 093006, arXiv:astro-ph/0305460.
[Favier:2003gn]
[15-27]
Calculation of fluxes of charged particles and neutrinos from atmospheric showers, V. Plyaskin, arXiv:hep-ph/0303146, 2003.
[Plyaskin:2003ia]
[15-28]
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.
[Martin:2003us]
[15-29]
Simulation of Atmospheric Muon and Neutrino Fluxes with CORSIKA, J. Wentz 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).
[Wentz:2003bp]
[15-30]
Atmospheric neutrino flux from 3-dimensional simulation, Yong Liu, L. Derome, M. Buenerd, 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.
[Liu:2002sq]
[15-31]
The FLUKA atmospheric neutrino flux calculation, G. Battistoni, A. Ferrari, T. Montaruli, P. R. Sala, 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. [15-53] and [15-55] that have been used extensively as input to the detector simulation. The new absolute flux normalization is clearly lower. (M.L.).
[Battistoni:2002ew]
[15-32]
Comparison of the FLUKA calculations with CAPRICE94 data on muons in atmosphere, G. Battistoni, A. Ferrari, T. Montaruli, P. R. Sala, Astropart. Phys. 17 (2002) 477-488, arXiv:hep-ph/0107241.
[Battistoni:2001fp]
[15-33]
Semi-analytic approximations for production of atmospheric muons and neutrinos, Thomas K. Gaisser, Astropart. Phys. 16 (2002) 285-294, arXiv:astro-ph/0104327.
[Gaisser:2001sd]
[15-34]
Comparison of 3-dimensional and 1-dimensional schemes in the calculation of atmospheric neutrinos, M. Honda, T. Kajita, K. Kasahara, S. Midorikawa, Phys. Rev. D64 (2001) 053011, arXiv:hep-ph/0103328.
[Honda:2001xy]
[15-35]
Atmospheric neutrino flux supported by recent muon experiments, Giovanni Fiorentini, Vadim A. Naumov, Francesco L. Villante, 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.
[Fiorentini:2001wa]
[15-36]
Calculation of atmospheric neutrino flux, Vassily Plyaskin (AMS), Phys. Lett. B516 (2001) 213-235, arXiv:hep-ph/0103286.
From the article: The simulation correctly describes the fluxes of protons and leptons ($e^+,e^-$) 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 $\Delta m^2$. 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.
[Plyaskin:2001ku]
[15-37]
The fluxes of sub-cutoff particles detected by AMS, the cosmic ray albedo and atmospheric neutrinos, Paolo Lipari, Astropart. Phys. 16 (2002) 295-323, arXiv:astro-ph/0101559.
[Lipari:2001rk]
[15-38]
Fluxes of cosmic ray muons and atmospheric neutrinos at high energies, L. V. Volkova, G. T. Zatsepin, Phys. Atom. Nucl. 64 (2001) 266-274.
[Volkova:2001th]
[15-39]
The east-west effect for atmospheric neutrinos, Paolo Lipari, Astropart. Phys. 14 (2000) 171-188, arXiv:hep-ph/0003013.
[Lipari:2000du]
[15-40]
The geometry of atmospheric neutrino production, Paolo Lipari, Astropart. Phys. 14 (2000) 153-170, arXiv:hep-ph/0002282.
[Lipari:2000wu]
[15-41]
Primary cosmic rays, antiprotons and atmospheric neutrinos, T. K. Gaisser, Phys. Scripta T85 (2000) 100-105.
[Gaisser:2000sk]
[15-42]
A three-dimensional calculation of atmospheric neutrino fluxes, Yaroslav Tserkovnyak, Robert Komar, Christian Nally, Chris Waltham, Astropart. Phys. 18 (2003) 449, arXiv:hep-ph/9907450.
[Tserkovnyak:1999ys]
[15-43]
A 3-dimensional calculation of atmospheric neutrino flux, G. Battistoni et al., Astropart. Phys. 12 (2000) 315-333, arXiv:hep-ph/9907408.
[Battistoni:1999at]
[15-44]
Uncertainties in prompt atmospheric neutrino flux calculations, L. V. Volkova, G. T. Zatsepin, Phys. Lett. B462 (1999) 211-216.
[Volkova:1999uz]
[15-45]
Lepton fluxes from atmospheric charm, L. Pasquali, M. H. Reno, I. Sarcevic, Phys. Rev. D59 (1999) 034020, arXiv:hep-ph/9806428.
[Pasquali:1998ji]
[15-46]
Atmospheric muon flux at sea level, underground and underwater, E. V. Bugaev et al., Phys. Rev. D58 (1998) 054001, arXiv:hep-ph/9803488.
[Bugaev:1998bi]
[15-47]
Geomagnetic effects on atmospheric neutrinos, Paolo Lipari, Todor Stanev, T. K. Gaisser, Phys. Rev. D58 (1998) 073003, arXiv:astro-ph/9803093.
[Lipari:1998cm]
[15-48]
The K(l3) form factors and atmospheric neutrino flavor ratio at high energies, V. A. Naumov, T. S. Sinegovskaya, S. I. Sinegovsky, Nuovo Cim. A111 (1998) 129-148, arXiv:hep-ph/9802410.
[Naumov:1998vi]
[15-49]
New calculation of atmospheric neutrino fluxes, K. Mitsui, Y. Minorikawa, M. Takazawa, Nuovo Cim. C21 (1998) 99-112.
[Mitsui:1998uv]
[15-50]
Path length distributions of atmospheric neutrinos, T. K. Gaisser, Todor Stanev, Phys. Rev. D57 (1998) 1977-1982, arXiv:astro-ph/9708146.
[Gaisser:1997eu]
[15-51]
New limitation onto the cosmic neutrino flux recorded on earth, L. V. Volkova, G. T. Zatsepin, Bull. Russ. Acad. Sci. Phys. 61 (1997) 474-476.
[Volkova:1997ut]
[15-52]
Comparison of atmospheric neutrino flux calculations at low energies, T. K. Gaisser et al., Phys. Rev. D54 (1996) 5578-5584, arXiv:hep-ph/9608253.
[Gaisser:1996dz]
[15-53]
Atmospheric neutrino flux above 1 GeV, Vivek Agrawal, T. K. Gaisser, Paolo Lipari, Todor Stanev, Phys. Rev. D53 (1996) 1314-1323, arXiv:hep-ph/9509423.
[Agrawal:1995gk]
[15-54]
Charm production and high energy atmospheric muon and neutrino fluxes, P. Gondolo, G. Ingelman, M. Thunman, Astropart. Phys. 5 (1996) 309-332, arXiv:hep-ph/9505417.
[Gondolo:1995fq]
[15-55]
Calculation of the flux of atmospheric neutrinos, M. Honda, T. Kajita, K. Kasahara, S. Midorikawa, Phys. Rev. D52 (1995) 4985-5005, arXiv:hep-ph/9503439.
[Honda:1995hz]
[15-56]
A New calculation of atmospheric neutrino fluxes, D. H. Perkins, Astropart. Phys. 2 (1994) 249-256.
[Perkins:1994pm]
[15-57]
Lepton spectra in the earth's atmosphere, P. Lipari, Astropart. Phys. 1 (1993) 195-227.
[Lipari:1993hd]
[15-58]
Calculation of atmospheric neutrino fluxes, M. Kawasaki, S. Mizuta, Phys. Rev. D43 (1991) 2900-2908.
[Kawasaki:1991qx]
[15-59]
Atmospheric neutrino fluxes, M. Honda, K. Kasahara, K. Hidaka, S. Midorikawa, Phys. Lett. B248 (1990) 193-198.
[Honda:1990sx]
[15-60]
A new calculation of atmospheric neutrino flux, Hae-shim Lee, Nuovo Cim. B105 (1990) 883-887.
[Lee:1990bw]
[15-61]
On the interpretation of the Kamiokande neutrino experiment, E. V. Bugaev, Vadim A. Naumov, Phys. Lett. B232 (1989) 391-397.
[Bugaev:1989jb]
[15-62]
Flux of atmospheric neutrinos, G. Barr, T. K. Gaisser, T. Stanev, Phys. Rev. D39 (1989) 3532-3534.
[Barr:1989ru]
[15-63]
Cosmic ray neutrinos in the atmosphere, T. K. Gaisser, Todor Stanev, Giles Barr, Phys. Rev. D38 (1988) 85.
[Gaisser:1988ar]
[15-64]
Ratio of electron-neutrino / muon-neutrino in atmospheric neutrinos, Stephen M. Barr, T. K. Gaisser, Paolo Lipari, Serap Tilav, Phys. Lett. B214 (1988) 147.
[Barr:1988rb]
[15-65]
Interactions of atmospheric neutrinos in nuclei at low- energy, T. K. Gaisser, J. S. O'Connell, Phys. Rev. D34 (1986) 822-825.
[Gaisser:1986bv]
[15-66]
Spectra of atmospheric muons and neutrinos of prompt generation, L. V. Volkova, G. T. Zatsepin, Bull. Russ. Acad. Sci. Phys. 49 (1985) NO.7143.
[Volkova:1985vx]
[15-67]
Neutrino induced muon flux deep underground and search for neutrino oscillations, T. K. Gaisser, Todor Stanev, Phys. Rev. D30 (1984) 985.
[Gaisser:1984mx]
[15-68]
The flux of atmospheric neutrinos, T. K. Gaisser, Todor Stanev, S. A. Bludman, Hae-shim Lee, Phys. Rev. Lett. 51 (1983) 223-226.
[Gaisser:1983vc]
[15-69]
Prompt lepton generation - atmospheric muon and neutrino spectra at high-energies, L. V. Volkova, G. T. Zatsepin, Sov. J. Nucl. Phys. 37 (1983) 212.
[Volkova:1983yf]
[15-70]
Energy spectra and angular distributions of atmospheric neutrinos, L. V. Volkova, Sov. J. Nucl. Phys. 31 (1980) 784-790.
[Volkova:1980sw]
[15-71]
Cosmic ray muon spectrum at sea level - primary cosmic ray nucleon spectrum, L. V. Volkova, G. T. Zatsepin, L. A. Kuzmichev, Sov. J. Nucl. Phys. 29 (1979) 645. Yad. Fiz. 29 (1979) 1252.
[Volkova:1979af]
[15-72]
G. T. Zatsepin, V. A. Kuzmin, Sov. Phys. JETP 14 (1962) 1294.
[Zatsepin-Kuzmin-SPJETP14-1962]
[15-73]
On high energy neutrino physics in cosmic rays, M. A. Markov, I. M. Zheleznykh, Nucl. Phys. 27 (1961) 385-394.
[Markov-Zheleznykh-NP27-1961]

16 - Neutrino Flux - Conference Proceedings

[16-1]
Prompt atmospheric neutrino flux from the various QCD models, Yu Seon Jeong et al., arXiv:1611.05540, 2016. ICHEP2016.
[Jeong:2016hya]
[16-2]
Prompt atmospheric neutrino flux, Yu Seon Jeong et al., PoS ICHEP2016 (2016) 083, arXiv:1611.05120. ICHEP2016.
[Jeong:2016cra]
[16-3]
Neutrinos from charm production in the atmosphere, Rikard Enberg, AIP Conf.Proc. 1630 (2014) 44-49, arXiv:1402.0880. Very Large Volume Neutrino Telescope Workshop 2013.
[Enberg:2014tua]
[16-4]
High-energy fluxes of atmospheric neutrinos, T.S. Sinegovskaya, E.V. Ogorodnikova, S.I. Sinegovsky, arXiv:1306.5907, 2013. 33rd International Cosmic Ray Conference (ICRC2013), Rio de Janeiro, Brazil, 2-9 July, 2013.
[Sinegovskaya:2013wgm]
[16-5]
High-energy spectrum and zenith-angle distribution of atmospheric neutrinos, S. I. Sinegovsky, O. N. Petrova, T. S. Sinegovskaya, arXiv:1109.3576, 2011. 32nd ICRC (Beijing, China, 11-18 Aug. 2011).
[Sinegovsky:2011ab]
[16-6]
FLUKA as a new high energy cosmic ray generator, Giuseppe Battistoni, Annarita Margiotta, Silvia Muraro, Maximiliano Sioli, Nucl. Instrum. Meth. A626-627 (2011) S191-S192, arXiv:1002.4655. Very Large Volume neutrino Telescope Workshop 2009 - VLVnT09, Athens, October 2009.
[Battistoni:2010vf]
[16-7]
Impact of high-energy hadron interactions on the atmospheric neutrino flux predictions, A. A. Kochanov, T. S. Sinegovskaya, S. I. Sinegovsky, arXiv:0906.0671, 2009. 31th ICRC, 7-15 July 2009, Lodz, Poland.
[Kochanov:2009rba]
[16-8]
About possible contribution of intrinsic charm component to inclusive spectra of charmed mesons, E.V. Bugaev, P.A. Klimai, J. Phys. G 37 (2010) 055004, arXiv:0905.2309. 31st International Cosmic Ray Conference, to be held in Lodz, Poland, 2009.
[Bugaev:2009jw]
[16-9]
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.
[Battistoni:2006en]
[16-10]
Atmospheric Neutrino Fluxes, Thomas K. Gaisser, Phys. Scripta T121 (2005) 51, arXiv:astro-ph/0502380. Nobel Symposium 129 Neutrino Physics.
[Gaisser:2005dt]
[16-11]
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.
[Battistoni:2004bm]
[16-12]
Atmospheric neutrino fluxes, G. Barr, 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/tuesday/barr.pdf.
[Barr-Nu2004]
[16-13]
The physics models of FLUKA: status and recent development, A. Fasso' 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.
[Fasso:2003xz]
[16-14]
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.
[Fasso:2003bh]
[16-15]
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.
[Battistoni:2003ju]
[16-16]
The calculation of atmospheric neutrino flux, M. Honda, 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.
[Honda:NOON2003]
[16-17]
Atmospheric neutrino fluxes, Thomas K. Gaisser, 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.
[Gaisser:2002mi]
[16-18]
Atmospheric muons and neutrinos, Vadim A. Naumov, arXiv:hep-ph/0201310, 2002. 2nd Workshop on Methodical Aspects of Underwater/Ice Neutrino Telescopes, Hamburg, Germany, 15-16 Aug 2001.
[Naumov:2002dm]
[16-19]
Progresses in the validation of the FLUKA atmospheric nu flux calculations, G. Battistoni, A. Ferrari, T. Montaruli, P. R. Sala, Nucl. Phys. Proc. Suppl. 110 (2002) 336-338, arXiv:hep-ph/0112072.
[Battistoni:2001sw]
[16-20]
Atmospheric proton and neutron spectra at energies above 1- GeV, V. A. Naumov, T. S. Sinegovskaya, arXiv:hep-ph/0106015, 2001.
[Naumov:2001uc]
[16-21]
Atmospheric neutrino flux and muon data, G. Fiorentini, V. A. Naumov, F. L. Villante, arXiv:hep-ph/0106014, 2001.
[Fiorentini:2001ub]
[16-22]
Review of sources of atmospheric neutrinos, P. Lipari, Nucl. Phys. Proc. Suppl. 91 (2001) 159-166.
[Lipari:2001tm]
[16-23]
Atmospheric neutrino sources: A review, P. Lipari, 2001. Published in 'Venice 2001, Neutrino Telescopes, vol. 1' 221-246.
[Lipari:2001vj]
[16-24]
A Three-dimensional calculation of atmospheric neutrino fluxes, Y. Tserkovnyak, R. J. Komar, C. W. Nally, C. E. Waltham, 2001. 27th International Cosmic Ray Conference (ICRC 2001), Hamburg, Germany, 7-15 Aug 2001.
[Tserkovnyak:2001ke]
[16-25]
Systematic uncertainties in the prediction of the atmospheric nu fluxes, P. Lipari, Nucl. Phys. Proc. Suppl. 100 (2001) 136-138.
[Lipari:2001aa]
[16-26]
Primary spectrum to 1-TeV and beyond, T. K. Gaisser, T. Stanev, M. Honda, P. Lipari, 2001. 27th International Cosmic Ray Conference (ICRC 2001), Hamburg, Germany, 7-15 Aug 2001. http://www.copernicus.org/icrc/papers/ici6694_p.pdf.
[Gaisser:2001jw]
[16-27]
Neutrini al Gran Sasso, F. Vissani, 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.).
[Vissani-Padova-2002]
[16-28]
Atmospheric neutrino flux calculations, G. Battistoni, Nucl. Phys. Proc. Suppl. 100 (2001) 101-106.
[Battistoni:2001zu]
[16-29]
Uncertainties on atmospheric neutrino flux calculations, G. Battistoni, Nucl. Phys. Proc. Suppl. 100 (2000) 101-106, arXiv:hep-ph/0012268.
[Battistoni:2000mf]
[16-30]
Atmospheric neutrino flux: A review of calculations, T. K. Gaisser, Nucl. Phys. Proc. Suppl. 87 (2000) 145-151, arXiv:hep-ph/0001027.
[Gaisser:1999if]
[16-31]
The primary protons and the atmospheric neutrino fluxes, Paolo Lipari, arXiv:hep-ph/9905506, 1999.
[Lipari:1999rb]
[16-32]
Fluxes of muons and showers with a given energy release from atmospheric neutrinos at energies 10**3-GeV to 10**7- GeV, L. V. Volkova, G. T. Zatsepin, Bull. Russ. Acad. Sci. Phys. 63 (1999) 459-461.
[Volkova:1999pq]
[16-33]
Limits on calculated atmospheric neutrino fluxes at high energies, L. V. Volkova, 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Volkova:1999fm]
[16-34]
Calculation of atmospheric neutrino and the sensitivity of angular dependences to various models, M. Honda, K. Kasahara, S. Midorikawa, 1999. 26th International Cosmic Ray Conference (ICRC 99), Salt Lake City, Utah, 17-25 Aug 1999.
[Honda:1999fd]
[16-35]
A new calculation of atmospheric neutrino flux: The FLUKA approach, G. Battistoni et al., Nucl. Phys. Proc. Suppl. 70 (1999) 358-360.
[Battistoni:1999av]
[16-36]
Uncertainty of the atmospheric neutrino fluxes, M. Honda, Nucl. Phys. Proc. Suppl. 77 (1999) 140-145, arXiv:hep-ph/9811504.
[Honda:1998km]
[16-37]
Fluxes of atmospheric neutrinos and related cosmic rays, T. K. Gaisser, Nucl. Phys. Proc. Suppl. 77 (1999) 133-139, arXiv:hep-ph/9811315.
[Gaisser:1998hb]
[16-38]
Primary cosmic-ray spectrum and the intensity of atmospheric neutrinos, Thomas K. Gaisser, arXiv:hep-ph/9811314, 1998.
[Gaisser:1998ha]
[16-39]
Muon and muon-neutrino fluxes from atmospheric charm, L. Pasquali, M. H. Reno, I. Sarcevic, 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.
[Pasquali:1997kh]
[16-40]
Atmospheric Neutrinos, Morihiro Honda, Takaaki Kajita, Katsuaki Kasahara, Shoichi Midorikawa, Prog. Theor. Phys. Suppl. 123 (1996) 483-490, arXiv:hep-ph/9511223.
[Honda:1995id]
[16-41]
Fluxes of muon-neutrino and electron-neutrino in the atmosphere: Is there an anomaly?, T. K. Gaisser, Nucl. Phys. Proc. Suppl. 35 (1994) 209-215.
[Gaisser:1994jv]
[16-42]
Calculation of low-energy atmospheric neutrino fluxes, M. Honda, 1994.
[Honda:1994qn]
[16-43]
Atmopheric neutrino event rates: The Expectations, T. K. Gaisser, 1993. Neutrino Astronomy Discussion Meeting, London, England, 9-10 June 1993.
[Gaisser:1993jx]
[16-44]
Atmospheric neutrinos, T. Stanev, 1993. 5th International Symposium on Neutrino Telescopes, Venice, Italy, 2-4 Mar 1993.
[Stanev:1993et]
[16-45]
The anomalous atmospheric neutrino flux and the possibility of neutrino oscillation, S. Midorikawa, M. Honda, K. Kasahara, 1991. 5th Workshop on Elementary-Particle Picture of the Universe, Izu, Japan, 19 Nov 1991.
[Midorikawa:1990hc]
[16-46]
Cosmic ray muons and atmospheric neutrinos, L. V. Volkova, 1990. High energy phenomenology, Campinas 1990.
[Volkova:1990pe]
[16-47]
A Comment on electron-neutrino / muon-neutrino ratio in atmospheric neutrino fluxes, L. V. Volkova, 1988. Cosmic gamma rays, neutrinos, and related astrophysics, Erice 1988.
[Volkova:1988qc]
[16-48]
Atmospheric muons and neutrinos of low and medium energies, E. V. Bugaev, Vadim A. Naumov, 1987. 20th International Cosmic Ray Conference, Moscow, USSR, 2-15 Aug 1987.
[Bugaev:1987yy]
[16-49]
Muons and neutrinos, T. Stanev, 1985. 9th Int. Conf. on Cosmic Rays, San Diego, CA, Aug 11-23, 1985.
[Stanev:1985zn]
[16-50]
Atmospheric neutrino fluxes at low-energy, T. Stanev, T. K. Gaisser, 1984. Solar neutrinos and neutrino astronomy, Kyoto 1979.
[Stanev:1984vm]
[16-51]
Interaction rates of atmospheric neutrinos, T. K. Gaisser, Todor Stanev, 1984. ICOBAN '84, Park City, Utah, Jan 4-7, 1984.
[Gaisser:1984mv]
[16-52]
Atmospheric neutrinos in underground detectors, T. K. Gaisser, T. Stanev, 1984. Neutrino Physics and Astrophysics, Nordkirchen 1984.
[Gaisser:1985ri]
[16-53]
High-energy cosmic ray atmospheric neutrinos, L. V. Volkova, 1979. 16th International Cosmic Ray Conference, Muenchen 1975.
[Volkova:1979vb]
16-54.
R. Cowsik, 1963. Eighth International Conference on Cosmic Rays, Jaipur, India, December 1963.
[Cowsik-Berkeley-1963]
16-55.
K. Greisen, 1960. International Conference on Instrumentation for High-Energy Physics, Berkeley, California, September 1960.
[Greisen-Berkeley-1960]

17 - Production Cross Sections

[17-1]
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18 - Production Cross Sections - Conference Proceedings

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19 - Detection Cross Sections

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20 - Detection Cross Sections - Conference Proceedings

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21 - Detector

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22 - Phenomenology

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Probing Lorentz and CPT Violation in a Magnetized Iron Detector using Atmospheric Neutrinos, Animesh Chatterjee, Raj Gandhi, Jyotsna Singh, JHEP 1406 (2014) 045, arXiv:1402.6265.
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Determination of the neutrino mass ordering by combining PINGU and Daya Bay II, Mattias Blennow, Thomas Schwetz, JHEP 1309 (2013) 089, arXiv:1306.3988.
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Comments on the reach of INO experiment: JHEP 1304, 009 (2013) and arXiv:1303.2534 [hep-ph], Abhijit Samanta, arXiv:1305.2819, 2013.
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Probing Non-Standard Interaction of Neutrinos with IceCube and DeepCore, Arman Esmaili, Alexei Yu. Smirnov, JHEP 1306 (2013) 026, arXiv:1304.1042.
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Exploring $\nu_{\tau}-\nu_{s}$ mixing with cascade events in DeepCore, Arman Esmaili, Francis Halzen, O. L. G. Peres, JCAP 1307 (2013) 048, arXiv:1303.3294.
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Constraining Sterile Neutrinos with AMANDA and IceCube Atmospheric Neutrino Data, Arman Esmaili, Francis Halzen, O. L. G. Peres, JCAP 1211 (2012) 041, arXiv:1206.6903.
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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 $\Delta{m}^2$ are either $ 1.2 \times 10^{-3} \, \mathrm{eV}^2 $ or $ > 0.1 \, \mathrm{eV}^2 $.
The smaller value $( 1.2 \times 10^{-3} \, \mathrm{eV}^2 )$ give $P_{\bar\nu_\mu\to\bar\nu_e}=0$ in LSND. Therefore, this case is equivalent to neglect LSND.
The larger values $( > 0.1 \, \mathrm{eV}^2 )$ obviously cannot fit the energy spectra of atmospheric neutrinos, which have been omitted in the analysis.
[C.G.].

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Implications of the $\nu_\mu$ - > $\nu_s$ solution to the atmospheric neutrino anomaly for early universe cosmology, R. Foot, Astropart. Phys. 10 (1999) 253-273, arXiv:hep-ph/9809315.
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Do the Super-Kamiokande atmospheric neutrino results explain electric charge quantisation?, R. Foot, R. R. Volkas, Phys. Rev. D59 (1999) 097301, arXiv:hep-ph/9808388.
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Textures for atmospheric and solar neutrino oscillations, Riccardo Barbieri, Lawrence J. Hall, A. Strumia, Phys. Lett. B445 (1999) 407-411, arXiv:hep-ph/9808333.
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Atmospheric neutrinos at Super-Kamiokande and parametric resonance in neutrino oscillations, E. K. Akhmedov, A. Dighe, P. Lipari, A. Y. Smirnov, Nucl. Phys. B542 (1999) 3-30, arXiv:hep-ph/9808270.
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Super-Kamiokande atmospheric neutrino data, zenith distributions, and three-flavor oscillations, Gian Luigi Fogli, E. Lisi, A. Marrone, G. Scioscia, Phys. Rev. D59 (1999) 033001, arXiv:hep-ph/9808205.
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Dynamical neutrino mass matrix: Large (small) mixing solution to atmospheric (solar) neutrino oscillations, Ernest Ma, Phys. Lett. B442 (1998) 238-242, arXiv:hep-ph/9807386.
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Interpreting the atmospheric neutrino anomaly, R. P. Thun, S. McKee, Phys. Lett. B439 (1998) 123-129, arXiv:hep-ph/9806534.
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Measuring the $\nu_\mu$ to $\bar\nu_\mu$ ratio in a high statistics atmospheric neutrino experiment, J. M. LoSecco, Phys. Rev. D59 (1999) 117302, arXiv:hep-ph/9806318.
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Atmospheric neutrino oscillations in three-flavor neutrinos, T. Teshima, T. Sakai, Prog. Theor. Phys. 101 (1999) 147, arXiv:hep-ph/9805386.
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Parametric resonance of neutrino oscillations and passage of solar and atmospheric neutrinos through the earth, E. K. Akhmedov, Nucl. Phys. B538 (1999) 25-51, arXiv:hep-ph/9805272.
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Three flavor neutrino oscillation analysis of the Super-Kamiokande atmospheric neutrino data, Osamu Yasuda, Phys. Rev. D58 (1998) 091301, arXiv:hep-ph/9804400.
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[22-225]
Comparison of $\nu_\mu$ < - > $\nu_\tau$ and $\nu_\mu$ < - > $\nu_s$ oscillations as solutions of the atmospheric neutrino problem, Paolo Lipari, Maurizio Lusignoli, Phys. Rev. D58 (1998) 073005, arXiv:hep-ph/9803440.
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Parametric resonance in oscillations of atmospheric neutrinos?, Q. Y. Liu, S. P. Mikheyev, A. Yu. Smirnov, Phys. Lett. B440 (1998) 319-326, arXiv:hep-ph/9803415.
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A minimality condition and atmospheric neutrino oscillations, Carl H. Albright, K. S. Babu, Stephen M. Barr, Phys. Rev. Lett. 81 (1998) 1167-1170, arXiv:hep-ph/9802314.
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Confronting solutions to the atmospheric neutrino anomaly involving large angle $\nu_\mu$ - > $\nu_e$ oscillations with Super-Kamiokande and CHOOZ, R. Foot, R. R. Volkas, O. Yasuda, Phys. Lett. B433 (1998) 82-87, arXiv:hep-ph/9802287.
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[22-229]
Comparing and contrasting the $\nu_\mu$ - > $\nu_\tau$ and $\nu_\mu$ - > $\nu_s$ solutions to the atmospheric neutrino problem with Super-Kamiokande data, R. Foot, R. R. Volkas, O. Yasuda, Phys. Rev. D58 (1998) 013006, arXiv:hep-ph/9801431.
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[22-230]
Implications of CHOOZ results for the decoupling of solar and atmospheric neutrino oscillations, Samoil M. Bilenky, C. Giunti, Phys. Lett. B444 (1998) 379-386.
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Examination of neutrino oscillations using high-energy atmospheric neutrino data from Kamiokande, Yuichi Oyama, Phys. Rev. D57 (1998) 6594-6598.
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Mass matrix ansatz for degenerate neutrinos consistent with solar and atmospheric neutrino data, K. Kang, S. K. Kang, J. E. Kim, P. Ko, Phys. Lett. B442 (1998) 249-254.
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Neutrino mass spectrum with $\nu_\mu$ - > $\nu_s$ oscillations of atmospheric neutrinos, Q. Y. Liu, A. Yu. Smirnov, Nucl. Phys. B524 (1998) 505-523, arXiv:hep-ph/9712493.
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A supersymmetric resolution of solar and atmospheric neutrino puzzles, Manuel Drees, S. Pakvasa, X. Tata, T. ter Veldhuis, Phys. Rev. D57 (1998) 5335-5339, arXiv:hep-ph/9712392.
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Zenith distribution of atmospheric neutrino events and electron neutrino mixing, Gian Luigi Fogli, E. Lisi, A. Marrone, D. Montanino, Phys. Lett. B425 (1998) 341-344, arXiv:hep-ph/9711421.
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Atmospheric neutrino oscillation and large lepton flavour violation in the SUSY SU(5) GUT, J. Hisano, Daisuke Nomura, T. Yanagida, Phys. Lett. B437 (1998) 351-358, arXiv:hep-ph/9711348.
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Neutral-to-charged current events ratio in atmospheric neutrinos and neutrino oscillations, Francesco Vissani, Alexei Yu. Smirnov, Phys. Lett. B432 (1998) 376-382, arXiv:hep-ph/9710565.
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Up-down atmospheric neutrino flux asymmetry predictions for various neutrino oscillation scenarios, R. Foot, R. R. Volkas, O. Yasuda, Phys. Lett. B421 (1998) 245-249, arXiv:hep-ph/9710403.
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Unified explanation of the solar and atmospheric neutrino puzzles in a minimal supersymmetric SO(10) model, B. Brahmachari, R. N. Mohapatra, Phys. Rev. D58 (1998) 015001, arXiv:hep-ph/9710371.
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Testing maximal electron and muon neutrino oscillations with sub-GeV Super-Kamiokande atmospheric neutrino data, R. Foot, R. R. Volkas, O. Yasuda, Phys. Rev. D57 (1998) 1345-1349, arXiv:hep-ph/9709483.
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Atmospheric neutrino oscillations with three neutrinos and a mass hierarchy, C. Giunti, C. W. Kim, M. Monteno, Nucl. Phys. B521 (1998) 3-36, arXiv:hep-ph/9709439.
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Up-down asymmetry: A diagnostic for neutrino oscillations, John W. Flanagan, John G. Learned, Sandip Pakvasa, Phys. Rev. D57 (1998) 2649-2652, arXiv:hep-ph/9709438.
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Atmospheric neutrino oscillation and a phenomenological lepton mass matrix, M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Rev. D57 (1998) 4429-4432, arXiv:hep-ph/9709388.
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Bounds on dark matter from the *atmospheric neutrino anomaly*, J. M. LoSecco, Phys. Rev. D56 (1997) 4416-4418, arXiv:hep-ph/9706368.
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Effects for atmospheric neutrino experiments from electron neutrino oscillations, J. Bunn, R. Foot, R. R. Volkas, Phys. Lett. B413 (1997) 109-113, arXiv:hep-ph/9702429.
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Three-flavor atmospheric neutrino anomaly, Gian Luigi Fogli, E. Lisi, D. Montanino, G. Scioscia, Phys. Rev. D55 (1997) 4385-4404, arXiv:hep-ph/9607251.
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Accelerator, reactor, solar and atmospheric neutrino oscillation: Beyond three generations, Srubabati Goswami, Phys. Rev. D55 (1997) 2931-2949, arXiv:hep-ph/9507212.
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Accelerator, reactor and atmospheric neutrino data: A Three flavor oscillation analysis, Srubabati Goswami, Kamales Kar, Amitava Raychaudhuri, Int. J. Mod. Phys. A12 (1997) 781-800, arXiv:hep-ph/9505395.
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Neutrino physics and the mirror world: How exact parity symmetry explains the solar neutrino deficit, the atmospheric neutrino anomaly and the LSND experiment, R. Foot, R. R. Volkas, Phys. Rev. D52 (1995) 6595-6606, arXiv:hep-ph/9505359.
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Atmospheric neutrino oscillations among three neutrino flavors and long baseline experiments, Samoil M. Bilenky, C. Giunti, C. W. Kim, Astropart. Phys. 4 (1996) 241-251, arXiv:hep-ph/9505301.
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Solar and atmospheric neutrino oscillations with three flavors, Mohan Narayan, M. V. N. Murthy, G. Rajasekaran, S. Uma Sankar, Phys. Rev. D53 (1996) 2809-2819, arXiv:hep-ph/9505281.
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Comment on the Kamiokande atmospheric neutrino deficit, David Saltzberg, Phys. Lett. B355 (1995) 499-500, arXiv:hep-ph/9504343.
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On the atmospheric neutrino anomaly and its statistical significance, Gian Luigi Fogli, E. Lisi, Phys. Rev. D52 (1995) 2775-2782, arXiv:hep-ph/9504287.
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Possible implications of the atmospheric, the Bugey, and the Los Alamos neutrino experiments, Hisakazu Minakata, Phys. Rev. D52 (1995) 6630-6633, arXiv:hep-ph/9503417.
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Possible revelation of seesaw mass pattern in solar and atmospheric neutrino data, Ernest Ma, J. Pantaleone, Phys. Rev. D52 (1995) 3763-3767, arXiv:hep-ph/9503312.
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Threefold maximal lepton mixing and the solar and atmospheric neutrino deficits, P. F. Harrison, D. H. Perkins, W. G. Scott, Phys. Lett. B349 (1995) 137-144.
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The Neutrino cross-section and upward going muons, Paolo Lipari, Maurizio Lusignoli, Francesca Sartogo, Phys. Rev. Lett. 74 (1995) 4384-4387, arXiv:hep-ph/9411341.
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Simple radiative neutrino mass matrix for solar and atmospheric oscillations, Ernest Ma, Phys. Rev. D51 (1995) 3145-3148, arXiv:hep-ph/9411315.
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Atmospheric neutrino problem in maximally mixed three generations of neutrinos, C. Giunti, C. W. Kim, J. D. Kim, Phys. Lett. B352 (1995) 357-364, arXiv:hep-ph/9411219.
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Reconciling cold dark matter with COBE / IRAS plus solar and atmospheric neutrino data, Anjan S. Joshipura, J. W. F. Valle, Nucl. Phys. B440 (1995) 647-660, arXiv:hep-ph/9410259.
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Accommodating solar and atmospheric neutrino deficits, hot dark matter, and a double beta decay signal, David O. Caldwell, Rabindra N. Mohapatra, Phys. Rev. D50 (1994) 3477-3483, arXiv:hep-ph/9402231.
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A comprehensive analysis of solar, atmospheric, accelerator and reactor neutrino experiments in a hierarchical three generation scheme, Gian Luigi Fogli, E. Lisi, D. Montanino, Phys. Rev. D49 (1994) 3626-3642.
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Constraints on three neutrino mixing from atmospheric and reactor data, J. Pantaleone, Phys. Rev. D49 (1994) 2152-2155, arXiv:hep-ph/9310363.
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A Common explanation for the atmospheric, solar neutrino and double beta decay anomalies, C. P. Burgess, Oscar Hernandez, Phys. Rev. D48 (1993) 4326-4336, arXiv:hep-ph/9306252.
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Quasielastic neutrino scattering from oxygen and the atmospheric neutrino problem, J. Engel, E. Kolbe, K. Langanke, P. Vogel, Phys. Rev. D48 (1993) 3048-3054, arXiv:nucl-th/9304017.
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The Atmospheric neutrino problem: A Critique, D. H. Perkins, Nucl. Phys. B399 (1993) 3-16.
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Neutrino mass explanations of solar and atmospheric neutrino deficits and hot dark matter, David O. Caldwell, Rabindra N. Mohapatra, Phys. Rev. D48 (1993) 3259-3263.
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A Single solution to the atmospheric and solar neutrino anomalies, A. Acker, J. G. Learned, S. Pakvasa, T. J. Weiler, Phys. Lett. B298 (1993) 149-153.
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Low-energy atmospheric neutrino data interpretations, L. V. Volkova, Phys. Lett. B316 (1993) 178-180.
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Neutrino cross-sections and the small atmospheric muon- neutrino / electron-neutrino ratio, A. K. Mann, Phys. Rev. D48 (1993) 422-424.
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A Neutrino decay model, solar anti-neutrinos and atmospheric neutrinos, A. Acker, A. Joshipura, S. Pakvasa, Phys. Lett. B285 (1992) 371-375.
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23 - Phenomenology - Conference Proceedings

[23-1]
Will atmospheric neutrino experiment at Hyper-Kamiokande see non-standard interaction effects?, Osamu Yasuda, arXiv:1610.09977, 2016. 18th International Workshop on Neutrino Factories, Super beams and Beta beams (NuFact2016), August 21-27 2016, Quy Nhon, Vietnam.
[Yasuda:2016vtk]
[23-2]
Sensitivity of atmospheric neutrino experiments to neutrino non-standard interactions, Shinya Fukasawa, arXiv:1609.07240, 2016. Neutrino 2016, XXVII International Conference on Neutrino Physics and Astrophysics, 4-9 July 2016, London, UK.
[Fukasawa:2016xeq]
[23-3]
Prompt neutrino flux in the atmosphere revisited, M.V. Garzelli, S. Moch, G. Sigl, arXiv:1602.08441, 2016. 17th Lomonosov Conference on Elementary Particle Physics, August 20 - 26 2015, Moscow State University, Moscow, Russia.
[Garzelli:2016yun]
[23-4]
Constraints on the flavor-dependent non-standard interaction in propagation from atmospheric neutrinos, Osamu Yasuda, J. Phys. Conf. Ser. 718 (2016) 062072, arXiv:1601.02369. TAUP2015, International Conference on Topics in Astroparticle and Underground Physics, 7-11 September 2015, Torino, Italy.
[Yasuda:2016svb]
[23-5]
Present theoretical uncertainties on charm hadroproduction in QCD and prompt neutrino fluxes, M.V. Garzelli, S. Moch, G. Sigl, EPJ Web Conf. 116 (2016) 08002, arXiv:1512.09097. VLVNT 2015, Rome, Italy, September 14-16 2015.
[Garzelli:2015tln]
[23-6]
A sterile neutrino at MiniBooNE and IceCube, Manuel Masip, AIP Conf.Proc. 1606 (2014) 59-65, arXiv:1402.0665. II Russian-Spanish Congress: Particle and Nuclear Physics at all Scales, Saint-Petersburg, October 1-4, 2013.
[Masip:2014xna]
[23-7]
Sensitivity of atmospheric neutrinos in Super-Kamiokande to Lorentz violation, Tarek Akiri, arXiv:1308.2210, 2013. Sixth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 17-21, 2013.
[Akiri:2013hca]
[23-8]
PINGU Sensitivity to the Neutrino Mass Hierarchy, M. G. Aartsen et al. (IceCube), arXiv:1306.5846, 2013. Snowmass 2013.
[Aartsen:2013aaa]
[23-9]
Sterile Neutrinos and IceCube, Francis Halzen, J. Phys. Conf. Ser. 408 (2013) 012023, arXiv:1111.0918. NUFACT 11, the XIIIth Intl. Workshop on Neutrino Factories, Super beams and Beta beams, 1-6 August 2011 at CERN and the University of Geneva, Switzerland.
[Halzen:2011yq]
[23-10]
Sibyll with charm, Eun-Joo Ahn, Ralph Engel, Thomas K. Gaisser, Paolo Lipari, Todor Stanev, arXiv:1102.5705, 2011. ISVHECRI 2010.
[Ahn:2011wt]
[23-11]
Some constraints on new physics by atmospheric neutrinos, Osamu Yasuda, Nucl. Phys. Proc. Suppl. 229-232 (2012) 543, arXiv:1010.5962. 24th International Conference on Neutrino Physics and Astrophysics (Neutrino 2010), Athens, Greece, 14-19 Jun 2010.
[Yasuda:2010eq]
[23-12]
High-energy atmospheric neutrinos, S. I. Sinegovsky, A. A. Kochanov, T. S. Sinegovskaya, arXiv:1010.2336, 2010. XVI International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2010), Batavia, IL, USA (28 June - 2 July 2010).
[Sinegovsky:2010dq]
[23-13]
The Physics Role and Potential of future Atmospheric Detectors, Raj Gandhi, AIP Conf. Proc. 1222 (2010) 26-30, arXiv:1004.5396. NUFACT 09, Chicago.
[Gandhi:2010iz]
[23-14]
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.
[Gaisser:2009gn]
[23-15]
Three-flavour neutrino oscillation update and comments on possible hints for a non-zero $\theta_{13}$, Michele Maltoni, Thomas Schwetz, PoS IDM2008 (2008) 072, arXiv:0812.3161. IDM2008, Aug. 18-22, 2008, Stockholm, Sweden.
[Maltoni:2008ka]
[23-16]
Physics Potential of Future Atmospheric Neutrino Searches, Thomas Schwetz, Nucl. Phys. Proc. Suppl. 188 (2009) 158-163, arXiv:0812.2392. NOW2008, Conca Specchiulla, Otranto, Italy, September 6-13, 2008.
[Schwetz:2008tc]
[23-17]
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.
[Maltoni:2008ie]
[23-18]
Modeling Atmospheric Neutrino Interactions: Duality Constrained Parameterization of Vector and Axial Nucleon Form Factors, A. Bodek, S. Avvakumov, R. Bradford, H. Budd, arXiv:0708.1827, 2007. 30th International Cosmic Ray Conference (ICRC 2007), Merida, Yucatan, Mexico, 3-11 Jul 2007.
[Bodek:2007wz]
[23-19]
Potentialities of atmospheric neutrinos, Michele Maltoni, arXiv:0707.1218, 2007. Rencontres de Moriond EW 2007, La Thuile, Italy, March 10-17, 2007.
[Maltoni:2007zz]
[23-20]
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.
[GonzalezGarcia:2006mh]
[23-21]
Can we learn something more on oscillations from atmospheric neutrinos?, Thomas Schwetz, Conf.Proc. C060726 (2006) 288-291, arXiv:hep-ph/0610053. ICHEP06, July 26-August 2, 2006, Moscow.
[Schwetz:2006he]
[23-22]
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.
[GonzalezGarcia:2006ji]
[23-23]
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.
[GonzalezGarcia:2006wm]
[23-24]
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.
[Battistoni:2006nz]
[23-25]
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.
[Minakata:2006fe]
[23-26]
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.
[Roy:2006dw]
[23-27]
The measurement of theta(13) and delta: The role of the uncertainties on the solar and atmospheric parameters, D. Meloni, Nucl. Phys. Proc. Suppl. 155 (2006) 178, arXiv:hep-ph/0509370. NUFACT'05, 21-26 June 2005, Frascati.
[Meloni:2005mv]
[23-28]
Search for exotic contributions to atmospheric neutrino oscillations, G. Battistoni et al., Phys. Atom. Nucl. 69 (2006) 1842-1846, arXiv:hep-ex/0508041. 29th I.C.R.C., Pune, India (2005).
[Battistoni:2005in]
[23-29]
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.
[Seki:2005yk]
[23-30]
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.
[Goswami:2004ya]
[23-31]
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.
[Petcov:2004bd]
[23-32]
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.
[Athar:2004pb]
[23-33]
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.
[Fogli:2003kp]
[23-34]
Inconsistencies in Interpreting the Atmospheric Neutrino Anomaly, John M. LoSecco, Pramana 62 (2004) 635, arXiv:hep-ph/0305022. PASCOS-2003.
[LoSecco:2003dg]
[23-35]
Neutrino Oscillations: Global Fits, T. Schwetz, 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.
[Schwetz:MPI2003]
[23-36]
Standard and Non-Standard Physics in Neutrino Oscillations, M. Maltoni, 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).
[Maltoni:2002kq]
[23-37]
Standard and non-standard neutrino properties, J. W. F. Valle, 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.
[Valle:2002tm]
[23-38]
LMA parameters and non-zero U(e3) effects on atmospheric nu data?, O. L. G. Peres, A. Yu. Smirnov, 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.
[Peres:2002ri]
[23-39]
From Atmospheric Neutrinos to Accelerator Neutrinos, P. Lipari, 2002. Workshop Neutrini al Gran Sasso - 25 March 2002, Padova, Italy. http://www.pd.infn.it/~laveder/cngspd/trasparenze/Lipari.pdf.
[Lipari-Padova2002]
[23-40]
(Mis)understanding the atmospheric neutrino anomaly, J. M. LoSecco, Nucl. Phys. Proc. Suppl. 98 (2001) 182-188, arXiv:hep-ph/0011117.
[LoSecco:2000xf]
[23-41]
Statistical tests for zenith angle dependences of up-going mu-like neutrino events for multi-GeV region, T. Kitamura et al., Nucl. Phys. Proc. Suppl. 75A (1999) 403-405.
[Kitamura:1999yr]

24 - Phenomenology - Muons

[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.
[Panda:2007fa]
[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.
[Kochanov:2007kc]
[24-3]
On the deficit of calculated muon flux at sea level for energies $ > 100$ GeV, A. A. Lagutin, A. G. Tyumentsev, A. V. Yushkov, Int. J. Mod. Phys. A20 (2005) 6959, arXiv:astro-ph/0503092.
[Lagutin:2005uj]
[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.
[Hansen:2004kf]
[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.
[Misaki:2003ga]

25 - Phenomenology - Muons - Conference Proceedings

[25-1]
Calculation of muon fluxes at the small atmospheric depths, Koh Abe et al., arXiv:astro-ph/0312632, 2003. 28th International Cosmic Ray Conferences (ICRC 2003), Tsukuba, Japan, 31 Jul - 7 Aug 2003.
[Abe:2003ah]

26 - Phenomenology - Models

[26-1]
Near Maximal Atmospheric Neutrino Mixing in Neutrino Mass Models with Two Texture Zeros, S. Dev, Radha Raman Gautam, Lal Singh, Manmohan Gupta, Phys. Rev. D90 (2014) 013021, arXiv:1405.0566.
[Dev:2014dla]
[26-2]
Relating large $U_{e3}$ to the ratio of neutrino mass-squared differences, Werner Rodejohann, Morimitsu Tanimoto, Atsushi Watanabe, Phys. Lett. B710 (2012) 636-640, arXiv:1201.4936.
[Rodejohann:2012jz]
[26-3]
Maximal atmospheric neutrino mixing from texture zeros and quasi-degenerate neutrino masses, W. Grimus, P.O. Ludl, Phys. Lett. B700 (2011) 356-361, arXiv:1104.4340.
[Grimus:2011sf]
[26-4]
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.
[Ji:2006qs]
[26-5]
Linking solar and long baseline terrestrial neutrino experiments, E. K. Akhmedov, G. C. Branco, M. N. Rebelo, Phys. Rev. Lett. 84 (2000) 3535, arXiv:hep-ph/9912205.
[Akhmedov:1999uw]

27 - Phenomenology - Critics

[27-1]
On the Relation between the True Directions of Neutrinos and the Reconstructed Directions of Neutrinos in L/E Analysis Performed by Super-Kamiokande Collaboration Part1, E.Konishi et al., arXiv:1108.1064, 2011.
[Konishi:2013zoa]
[27-2]
On the Sensitivity of L/E Analysis of Super-Kamiokande Atmospheric Neutrino Data to Neutrino Oscillation Part~2 -- Four Possible L/E Analyses for the Maximum Oscillation by the Numerical Computer Experiment --, E. Konishi et al., arXiv:1007.4921, 2010.
[Konishi:2010my]
[27-3]
Comprehensive Analysis of Neutrinos in SK part 3 - L/E Analysis for Single Ring Muon Events II -, E. Konishi et al., arXiv:0808.3508, 2008.
[Konishi:2008cn]
[27-4]
Comprehensive Analysis of Neutrinos in SK part II - L/E Analysis for Single Ring Muon Events I -, E. Konishi et al., arXiv:0808.3313, 2008.
[Konishi:2008wa]
[27-5]
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.
[Galkin:2008qe]
[27-6]
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.
[Konishi:2008gc]
[27-7]
The numerical computer experiment for the neutrino events with the SK neutrino oscillation parameters occurring outside the Superkamiokande detector, N. Takahashi, E. Konishi, A. Misaki, arXiv:0802.2422, 2008.
[Takahashi:2008ic]
[27-8]
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.
[Konishi:2007uk]
[27-9]
Can One Extract the Neutrino Oscillation Signature from the SuperKamiokande Experiment? An Analysis of Neutrino Events Occurring outside the Detector, N. Takahashi, A. Misaki, arXiv:hep-ex/0505020, 2005.
[Takahashi:2005sx]
[27-10]
A discrimination procedure between muon and electron in Superkamiokande experiment based on the angular distribution function method, V. I. Galkin, A. M. Anokhina, E. Konishi, A. Misaki, arXiv:hep-ex/0501058, 2005.
[Galkin:2005vt]
[27-11]
A theory of pattern recognition for the discrimination between muon and electron in the Super-Kamiokande, V. I. Galkin, A. M. Anokhina, E. Konishi, A. Misaki, arXiv:hep-ex/0412059, 2004.
[Galkin:2004gv]
[27-12]
Have Superkamiokande really measured the direction of the atmospheric neutrinos which produce fully contained events and partially contained events?, E. Konishi, Y. Minorikawa, V. I. Galkin, M. Ishiwata, A. Misaki, arXiv:hep-ex/0407015, 2004.
[Konishi:2004us]
[27-13]
The Zenith Angle Distribution of Fully Contained Events in SuperKamiokande and the Impact of Quasi Elastic Scattering on their Direction, Eiichi Konishi, Y. Minorikawa, V. I. Galkin, M. Ishiwata, A. Misaki, arXiv:astro-ph/0406497, 2004.
[Konishi:2004fa]

28 - Phenomenology - Critics - Conference Proceedings

[28-1]
Examination on SK atmospheric neutrino experiment by the computer experiment, A Misaki et al., arXiv:hep-ex/0605020, 2006. TAUP2005.
[Misaki:2006da]

29 - Theory - Neutrino Oscillations

[29-1]
Oscillations of high energy neutrinos in matter: Precise formalism and parametric resonance, E. Kh. Akhmedov, M. Maltoni, A. Yu. Smirnov, Phys. Rev. Lett. 95 (2005) 211801, arXiv:hep-ph/0506064.
[Akhmedov:2005yj]

30 - Theory - Models

[30-1]
The Elements of the Neutrino Mass Matrix: Allowed Ranges and Implications of Texture Zeros, A. Merle, W. Rodejohann, Phys. Rev. D73 (2006) 073012, arXiv:hep-ph/0603111.
[Merle:2006du]
[30-2]
A maximal atmospheric mixing from a maximal CP violating phase, Isabella Masina, Phys. Lett. B633 (2006) 134-140, arXiv:hep-ph/0508031.
[Masina:2005hf]

31 - Future Experiments

[31-1]
PINGU: A Vision for Neutrino and Particle Physics at the South Pole, M. G. Aartsen et al. (IceCube-Gen2), arXiv:1607.02671, 2016.
[TheIceCube-Gen2:2016cap]
[31-2]
Letter of Intent for KM3NeT2.0, S. Adrian-Martinez et al. (KM3Net), J. Phys. G43 (2016) 084001, arXiv:1601.07459.
[Adrian-Martinez:2016fdl]
[31-3]
Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO), Shakeel Ahmed et al. (ICAL), arXiv:1505.07380, 2015.
[Ahmed:2015jtv]
[31-4]
Letter of Intent: The Atmospheric Neutrino Neutron Interaction Experiment (ANNIE), I. Anghel et al. (ANNIE), arXiv:1504.01480, 2015.
[Anghel:2015xxt]
[31-5]
A Simulations Study of the Muon Response of the Iron Calorimeter Detector at the India-based Neutrino Observatory, Animesh Chatterjee et al., JINST 9 (2014) P07001, arXiv:1405.7243.
[Chatterjee:2014vta]
[31-6]
Expression of Interest: The Atmospheric Neutrino Neutron Interaction Experiment (ANNIE), I. Anghel et al. (ANNIE), arXiv:1402.6411, 2014.
[Anghel:2014ynd]
[31-7]
Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU), M. G. Aartsen et al. (IceCube-PINGU), arXiv:1401.2046, 2014.
[Aartsen:2014oha]
[31-8]
Hyper-Kamiokande Physics Opportunities, E. Kearns et al. (Hyper-Kamiokande Working Group), arXiv:1309.0184, 2013.
[Kearns:2013lea]
[31-9]
Future large-scale water-Cherenkov detector, L. Agostino et al. (MEMPHYS), Phys. Rev. ST Accel. Beams 16, 061001 (2013) 061001, arXiv:1306.6865.
[Agostino:2013ilw]
[31-10]
Hadron energy response of the ICAL detector at INO, Moon Moon Devi et al., JINST 8 (2013) P11003, arXiv:1304.5115.
[Devi:2013wxa]
[31-11]
Study of the performance of a large scale water-Cherenkov detector (MEMPHYS), L. Agostino et al. (MEMPHYS), JCAP JCAP1301 (2013) 024, arXiv:1206.6665.
[Agostino:2012fd]
[31-12]
Letter of Intent: The Hyper-Kamiokande Experiment - Detector Design and Physics Potential, K. Abe et al., arXiv:1109.3262, 2011.
[Abe:2011ts]
[31-13]
On the possibility to use ATLAS and CMS detectors for neutrino physics, A. Guskov, arXiv:0909.2513, 2009.
[Guskov:2009qb]
[31-14]
Large underground, liquid based detectors for astro-particle physics in Europe: scientific case and prospects, J. Aysto et al., JCAP 0711 (2007) 011, arXiv:0705.0116.
[Autiero:2007zj]
[31-15]
MEMPHYS: A large scale water Cerenkov detector at Frejus, A. de Bellefon et al., arXiv:hep-ex/0607026, 2006.
[deBellefon:2006vq]
[31-16]
A design outline for a Cherenkoff neutrino observatory, E. P. Bonvin, S. T. Hatamian, arXiv:physics/0310160, 2003.
[Bonvin:1991hz]
[31-17]
Physics Chapter: NUSEL-Homestake Science Book, C. Aalseth et al. (Homestake), arXiv:nucl-ex/0308018, 2003.
[Homestake:2003aa]
[31-18]
Multi-ring signatures of the oscillation $\nu_\mu \to \nu_e$ in a water Cherenkov detector, A. Asratyan et al., Eur. Phys. J. C31 (2003) 31, arXiv:hep-ex/0302013.
[Asratyan:2003ci]

32 - Future Experiments - Conference Proceedings

[32-1]
Probing new physics with atmospheric neutrinos at KM3NeT-ORCA, Joao A. B. Coelho (KM3NeT), arXiv:1702.04508, 2017. 27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016).
[Coelho:2017cwp]
[32-2]
Prospects for measuring the neutrino mass hierarchy with KM3NeT/ORCA, Jannik Hofestadt (KM3NeT), arXiv:1701.04078, 2017. 25th European Cosmic Ray Symposium (ECRS 2016) Turin, Italy, September 04-09, 2016.
[Hofestadt:2017jfu]
[32-3]
KM3NeT-ORCA: Oscillation Research with Cosmics in the Abyss, Paschal Coyle, arXiv:1701.01382, 2017. 27th International Conference on Neutrino Physics and Astrophysics (Neutrino 2016).
[Coyle:2017szp]
[32-4]
Neutrino Mass Ordering Studies with PINGU and IceCube/DeepCore, Steven Wren, arXiv:1604.08807, 2016. NuPhys2015 (London, 16-18 December 2015).
[Wren:2016phy]
[32-5]
From DeepCore to PINGU: Measuring atmospheric neutrino oscillations at the South Pole, J. P. Yanez (IceCube-Gen2), EPJ Web Conf. 116 (2016) 11009, arXiv:1601.05245. VLVnT Workshop 2015.
[Yanez:2016ojt]
[32-6]
Measuring the Neutrino Mass Hierarchy with Atmospheric Neutrinos, D. F. Cowen et al. (IceCube/PINGU), arXiv:1409.5755, 2014. Fundamental Symmetries, Neutrinos, Neutrons and related Nuclear Astrophysics Long-Range Plan Town Meeting, Sept. 28-29, 2014, Chicago, IL.
[Cowen:2014rga]
[32-7]
The LAGUNA design study- towards giant liquid based underground detectors for neutrino physics and astrophysics and proton decay searches, D. Angus et al. (LAGUNA), arXiv:1001.0077, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
[Angus:2010sz]
[32-8]
Giant Liquid Argon Observatory for Proton Decay, Neutrino Astrophysics and CP-violation in the Lepton Sector (GLACIER), A. Badertscher et al., arXiv:1001.0076, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, Oct. 2009.
[Badertscher:2010sy]
[32-9]
R&D for Future 100 kton Scale Liquid Argon Detectors, A. Marchionni, arXiv:0912.4417, 2009. European Strategy for Future Neutrino Physics, CERN, Oct. 2009.
[Marchionni:2009tj]
[32-10]
Underground Neutrino Detectors for Particle and Astroparticle Science: the Giant Liquid Argon Charge Imaging ExpeRiment (GLACIER), A. Rubbia, J. Phys. Conf. Ser. 171 (2009) 012020, arXiv:0908.1286.
[Rubbia:2009md]
[32-11]
Development of Glass Resistive Plate Chambers for INO, Satyanarayana Bheesette et al. (INO), arXiv:0810.4693, 2008. ICHEP08.
[Bheesette:2008rb]
[32-12]
India-based Neutrino Observatory, G.Rajasekaran, Aip Conf. Proc. 721 (2004) 243, arXiv:hep-ph/0402246. NuFact 03, 5th International Workshop on Neutrino Factories and Superbeams, 5-11, June 2003, Columbia University, New York.
[Rajasekaran:2004wi]
[32-13]
Future projects on atmospheric neutrinos, T. Tabarelli de Fatis, Nucl. Phys. Proc. Suppl. 118 (2003) 118, arXiv:hep-ex/0209053. XXth Internat. Conf. on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, May 25-30, 2002.
[TabarellideFatis:2002by]
[32-14]
UNO: Underground Nucleon Decay and Neutrino Observatory, C. McGrew, 2002. International Workshop on Neutrinos and Subterranean Science - NeSS 02, Washington, DC, September 19-21, 2002. http://mocha.phys.washington.edu/~int_talk/WorkShops/Neutrino02/Working_Groups/People/McGrew_C/mcgrew_thurs_protondecaywg.pdf.
[McGrew-talk:2002b]

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Last Update: Fri 17 Mar 2017, 09:07:34 UTC