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We present a review of atmospheric muon flux and energy spectrum measurements over almost six decades of muon momentum. Sea-level and underground/water/ice experiments are considered. Possible sources of systematic errors in the…

Earth and Planetary Astrophysics · Physics 2012-08-16 Stefano Cecchini , Maurizio Spurio

An instructional laboratory experiment to measure the muon mass is described. Using coincidence-anticoincidence detection, the decay of a cosmic-ray muon into an electron (or positron) is observed in a multiplate spark chamber, and recorded…

Physics Education · Physics 2010-02-05 Benjamin Brau , Christopher May , Robert Ormond , John Essick

The Daya Bay Experiment consists of eight identically designed detectors located in three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 meters of water equivalent vertical overburden, respectively. Cosmic muon…

Instrumentation and Detectors · Physics 2018-01-09 F. P. An , A. B. Balantekin , H. R. Band , M. Bishai , S. Blyth , D. Cao , G. F. Cao , J. Cao , Y. L. Chan , J. F. Chang , Y. Chang , H. S. Chen , Q. Y. Chen , S. M. Chen , Y. X. Chen , Y. Chen , J. Cheng , Z. K. Cheng , J. J. Cherwinka , M. C. Chu , A. Chukanov , J. P. Cummings , Y. Y. Ding , M. V. Diwan , M. Dolgareva , J. Dove , D. A. Dwyer , W. R. Edwards , R. Gill , M. Gonchar , G. H. Gong , H. Gong , M. Grassi , W. Q. Gu , L. Guo , X. H. Guo , Y. H. Guo , Z. Guo , R. W. Hackenburg , S. Hans , M. He , K. M. Heeger , Y. K. Heng , A. Higuera , Y. B. Hsiung , B. Z. Hu , T. Hu , E. C. Huang , H. X. Huang , X. T. Huang , P. Huber , W. Huo , G. Hussain , D. E. Jaffe , K. L. Jen , S. Jetter , X. P. Ji , X. L. Ji , J. B. Jiao , R. A. Johnson , D. Jones , L. Kang , S. H. Kettell , A. Khan , S. Kohn , M. Kramer , K. K. Kwan , M. W. Kwok , T. Kwok , T. J. Langford , K. Lau , L. Lebanowski , J. Lee , J. H. C. Lee , R. T. Lei , R. Leitner , C. Li , D. J. Li , F. Li , G. S. Li , Q. J. Li , S. Li , S. C. Li , W. D. Li , X. N. Li , X. Q. Li , Y. F. Li , Z. B. Li , H. Liang , C. J. Lin , G. L. Lin , S. Lin , S. K. Lin , Y. -C. Lin , J. J. Ling , J. M. Link , L. Littenberg , B. R. Littlejohn , J. L. Liu , J. C. Liu , C. W. Loh , C. Lu , H. Q. Lu , J. S. Lu , K. B. Luk , X. Y. Ma , X. B. Ma , Y. Q. Ma , Y. Malyshkin , D. A. Martinez Caicedo , K. T. McDonald , R. D. McKeown , I. Mitchell , Y. Nakajima , J. Napolitano , D. Naumov , E. Naumova , H. Y. Ngai , J. P. Ochoa-Ricoux , A. Olshevskiy , H. -R. Pan , J. Park , S. Patton , V. Pec , J. C. Peng , L. Pinsky , C. S. J. Pun , F. Z. Qi , M. Qi , X. Qian , R. M. Qiu , N. Raper , J. Ren , R. Rosero , B. Roskovec , X. C. Ruan , C. Sebastiani , H. Steiner , J. L. Sun , W. Tang , D. Taychenachev , K. Treskov , K. V. Tsang , C. E. Tull , N. Viaux , B. Viren , V. Vorobel , C. H. Wang , M. Wang , N. Y. Wang , R. G. Wang , W. Wang , X. Wang , Y. F. Wang , Z. Wang , Z. Wang , Z. M. Wang , H. Y. Wei , L. J. Wen , K. Whisnant , C. G. White , L. Whitehead , T. Wise , H. L. H. Wong , S. C. F. Wong , E. Worcester , C. -H. Wu , Q. Wu , W. J. Wu , D. M. Xia , J. K. Xia , Z. Z. Xing , J. L. Xu , Y. Xu , T. Xue , C. G. Yang , H. Yang , L. Yang , M. S. Yang , M. T. Yang , Y. Z. Yang , M. Ye , Z. Ye , M. Yeh , B. L. Young , Z. Y. Yu , S. Zeng , L. Zhan , C. Zhang , C. C. Zhang , H. H. Zhang , J. W. Zhang , Q. M. Zhang , X. T. Zhang , Y. M. Zhang , Y. X. Zhang , Y. M. Zhang , Z. J. Zhang , Z. Y. Zhang , Z. P. Zhang , J. Zhao , L. Zhou , H. L. Zhuang , J. H. Zou

The Scattering and Neutrino Detector at the LHC (\SND) started taking data at the beginning of Run 3 of the LHC. The experiment is designed to perform measurements with neutrinos produced in proton-proton collisions at the LHC in an energy…

High Energy Physics - Experiment · Physics 2023-11-17 LHC Collaboration

The atmospheric neutrino flux includes a component from the prompt decay of charmed hadrons that becomes significant only at $E\ge 10$ TeV. At these energies, however, the diffuse flux of cosmic neutrinos discovered by IceCube seems to be…

High Energy Physics - Phenomenology · Physics 2021-09-15 Miguel Gutiérrez , Gerardo Hernández-Tomé , José I. Illana , Manuel Masip

High-energy cosmic rays are observed indirectly by detecting the extensive air showers initiated in Earth's atmosphere. The interpretation of these observations relies on accurate models of air shower physics, which is a challenge and an…

The temperature of the upper atmosphere affects the height of primary cosmic ray interactions and the production of high-energy cosmic ray muons which can be detected deep underground. The MINOS far detector at Soudan MN, USA, has collected…

High Energy Physics - Experiment · Physics 2012-08-27 The MINOS Collaboration

The Large Volume Detector (LVD), hosted in the INFN Laboratori Nazionali del Gran Sasso, is triggered by atmospheric muons at a rate of $\sim 0.1$~Hz. The data collected over almost a quarter of century are used to study the muon intensity…

Extensive air showers produce high-energy muons that can be utilized to probe hadronic interaction models in cosmic ray interactions. Most muons originate from pion and kaon decays, called $\textit{conventional}$ muons, while a smaller…

It has been shown that muon flux intensities calculated in terms of the EPOS LHC and EPOS 1.99 models at the energy of 10^4 GeV exceed the data of the classical experiments L3+Cosmic, MACRO and LVD on the spectra of atmospheric muons by a…

High Energy Astrophysical Phenomena · Physics 2015-04-28 L. G. Dedenko , G. F. Fedorova , T. M. Roganova

The seasonal variation of single muons is a well-understood phenomenon, mainly driven by a positive correlation with temperature fluctuations in the atmospheric profiles. However, the rate of multi-muon events recorded by various…

High Energy Astrophysical Phenomena · Physics 2025-09-23 Jordi Tuneu , Eva Santos , Peter Filip

High-energy cosmic-ray muons reaching deep underground laboratories can cause events in detectors that mimic signals expected from dark matter particles, neutrinos, or rare decays. Knowledge of the muon flux and energy spectrum is important…

High Energy Physics - Experiment · Physics 2026-02-20 D. S. Akerib , A. K. Al Musalhi , F. Alder , B. J. Almquist , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , A. Baker , S. Balashov , J. Bang , J. W. Bargemann , E. E. Barillier , K. Beattie , A. Bhatti , T. P. Biesiadzinski , H. J. Birch , E. Bishop , G. M. Blockinger , C. A. J. Brew , P. Brás , S. Burdin , M. C. Carmona-Benitez , M. Carter , A. Chawla , H. Chen , Y. T. Chin , N. I. Chott , S. Contreras , M. V. Converse , R. Coronel , A. Cottle , G. Cox , D. Curran , C. E. Dahl , I. Darlington , S. Dave , A. David , J. Delgaudio , S. Dey , L. de Viveiros , L. Di Felice , C. Ding , J. E. Y. Dobson , E. Druszkiewicz , S. Dubey , C. L. Dunbar , S. R. Eriksen , N. M. Fearon , N. Fieldhouse , S. Fiorucci , H. Flaecher , E. D. Fraser , T. M. A. Fruth , P. W. Gaemers , R. J. Gaitskell , A. Geffre , J. Genovesi , C. Ghag , J. Ghamsari , A. Ghosh , R. Gibbons , S. Gokhale , J. Green , M. G. D. van der Grinten , J. J. Haiston , C. R. Hall , T. Hall , R. H. Hampp , S. J. Haselschwardt , M. A. Hernandez , S. A. Hertel , G. J. Homenides , M. Horn , D. Q. Huang , D. Hunt , R. S. James , E. Jacquet , K. Jenkins , A. C. Kaboth , A. C. Kamaha , M. K. Kannichankandy , D. Khaitan , A. Khazov , J. Kim , Y. D. Kim , D. Kodroff , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , C. Lawes , D. S. Leonard , K. T. Lesko , C. Levy , J. Lin , A. Lindote , W. H. Lippincott , J. Long , M. I. Lopes , W. Lorenzon , C. Lu , S. Luitz , V. Mahajan , P. A. Majewski , A. Manalaysay , R. L. Mannino , R. J. Matheson , C. Maupin , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , J. B. Mclaughlin , R. McMonigle , B. Mitra , E. Mizrachi , M. E. Monzani , K. Morå , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , H. N. Nelson , F. Neves , A. Nguyen , C. L. O'Brien , F. H. O'Shea , I. Olcina , K. C. Oliver-Mallory , J. Orpwood , K. Y. Oyulmaz , K. J. Palladino , N. J. Pannifer , N. Parveen , S. J. Patton , B. Penning , G. Pereira , E. Perry , T. Pershing , A. Piepke , S. S. Poudel , Y. Qie , J. Reichenbacher , C. A. Rhyne , G. R. C. Rischbieter , E. Ritchey , H. S. Riyat , R. Rosero , N. J. Rowe , T. Rushton , D. Rynders , S. Saltão , D. Santone , I. Sargeant , A. B. M. R. Sazzad , R. W. Schnee , G. Sehr , B. Shafer , S. Shaw , W. Sherman , K. Shi , T. Shutt , C. Silva , G. Sinev , J. Siniscalco , A. M. Slivar , R. Smith , V. N. Solovov , P. Sorensen , J. Soria , T. Stenhouse , T. J. Sumner , A. Swain , M. Szydagis , D. R. Tiedt , M. Timalsina , D. R. Tovey , J. Tranter , M. Trask , K. Trengove , M. Tripathi , A. Usón , A. C. Vaitkus , O. Valentino , V. Velan , A. Wang , J. J. Wang , Y. Wang , L. Weeldreyer , T. J. Whitis , K. Wild , M. Williams , J. Winnicki , L. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , J. Xu , Y. Xu , M. Yeh , D. Yeum , J. Young , W. Zha , H. Zhang , T. Zhang , Y. Zhou

In this paper parametric formulas are presented to evaluate the flux of atmospheric muons in the range of vertical depth between 1.5 to 5 km of water equivalent (km w.e.) and up to 85^o for the zenith angle. We take into account their…

High Energy Physics - Phenomenology · Physics 2009-10-23 M. Bazzotti , S. Biagi , G. Carminati , S. Cecchini , T. Chiarusi , G. Giacomelli , A. Margiotta , M. Sioli , M. Spurio

Inclusive distributions of charged particles in hadronic W decays are experimentally investigated using the statistics collected by the DELPHI experiment at LEP during 1997, 1998 and 1999, at centre-of-mass energies from 183 to around 200…

High Energy Physics - Experiment · Physics 2010-04-08 P. Abreu

The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008…

High Energy Physics - Experiment · Physics 2010-03-10 OPERA Collaboration , N. Agafonova , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , D. Autiero , A. Badertscher , A. Bagulya , A. Bertolin , M. Besnier , D. Bick , V. Boyarkin , C. Bozza , T. Brugière , R. Brugnera , G. Brunetti , S. Buontempo , A. Cazes , L. Chaussard , M. Chernyavsky , V. Chiarella , N. Chon-Sen , A. Chukanov , M. Cozzi , G. D'Amato , F. Dal Corso , N. D'Ambrosio , G. De Lellis , Y. D'eclais , M. De Serio , F. Di Capua , D. Di Ferdinando , A. Di Giovanni , N. Di Marco , S. Dmitrievski , M. Dracos , D. Duchesneau , S. Dusini , J. Ebert , O. Egorov , R. Enikeev , A. Ereditato , L. S. Esposito , J. Favier , G. Felici , T. Ferber , R. Fini , D. Frekers , T. Fukuda , C. Fukushima , V. I. Galkin , A. Garfagnini , G. Giacomelli , M. Giorgini , C. Goellnitz , J. Goldberg , D. Golubkov , L. Goncharova , Y. Gornushkin , G. Grella , F. Grianti , M. Guler , C. Gustavino , C. Hagner , K. Hamada , T. Hara , M. Hierholzer , K. Hoshino , M. Ieva , K. Jakovcic , C. Jollet , F. Juget , M. Kazuyama , S. H. Kim , M. Kimura , B. Klicek , J. Knuesel , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , H. Kubota , C. Lazzaro , J. Lenkeit , A. Ljubicic , A. Longhin , G. Lutter , A. Malgin , G. Mandrioli , A. Marotta , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , F. Meisel , A. Meregaglia , P. Migliozzi , S. Mikado , S. Miyamoto , P. Monacelli , K. Morishima , U. Moser , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , D. Naumov , V. Nikitina , K. Niwa , Y. Nonoyama , S. Ogawa , A. Olchevski , C. Oldorf , G. Orlova , V. Osedlo , M. Paniccia , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , V. Pilipenko , C. Pistillo , G. Policastro , N. Polukhina , M. Pozzato , K. Pretzl , P. Publichenko , F. Pupilli , R. Rescigno , T. Roganova , H. Rokujo , G. Romano , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , V. Ryasny , O. Ryazhskaya , O. Sato , Y. Sato , A. Schembri , W. Schmidt Parzefall , H. Schroeder , L. Scotto Lavina , A. Sheshukov , H. Shibuya , S. Simone , M. Sioli , C. Sirignano , G. Sirri , J. S. Song , M. Spinetti , L. Stanco , N. Starkov , M. Stipcevic , T. Strauss , P. Strolin , S. Takahashi , M. Tenti , F. Terranova , I. Tezuka , V. Tioukov , P. Tolun , T. Tran , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , V. Yakushev , C. S. Yoon , T. Yoshioka , J. Yoshida , Y. Zaitsev , S. Zemskova , A. Zghiche , R. Zimmermann

If produced at the LHC, long-lived charged particles (LLCPs) would leave tracks in the muon detector. Time-of-Flight based methods for detecting these particles become less efficient if the LLCPs are fast, which would typically be the case…

High Energy Physics - Phenomenology · Physics 2015-06-03 Iftah Galon , Yael Shadmi , Shahrazad Tarboush , Shlomit Tarem

An inclusive search for long-lived exotic particles (LLPs) decaying to final states with a pair of muons is presented. The search uses data corresponding to an integrated luminosity of 36.6 fb$^{-1}$ collected by the CMS experiment from the…

High Energy Physics - Experiment · Physics 2024-05-21 CMS Collaboration

Over the last two decades, various experiments have measured muon densities in extensive air showers over several orders of magnitude in primary energy. While some experiments observed differences in the muon densities between simulated and…

High Energy Astrophysical Phenomena · Physics 2021-08-24 Dennis Soldin

The CMS detector at the LHC has recorded events from proton-proton collisions, with muon momenta reaching up to 1.8 TeV in the collected dimuon samples. These high-momentum muons allow direct access to new regimes in physics beyond the…

Instrumentation and Detectors · Physics 2020-03-04 CMS Collaboration