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Competition between decay and re-interaction of charged pions and kaons depends on the temperature/density profile of the upper atmosphere. The amplitude and phase of the variations depend on the minimum muon energy required to reach the…

High Energy Astrophysical Phenomena · Physics 2021-07-28 Thomas Gaisser , Stef Verpoest

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…

Quantum - or classically correlated - light can be employed in various ways to improve resolution and measurement sensitivity. In an "interaction-free" measurement, a single photon can be used to reveal the presence of an object placed…

We present a cosmic ray muon tomographic experiment for measuring the muon flux and imaging the tunnel overburden structures in Changshu, China. The device used in this study is a tracking detector based on the plastic scintillator with…

Instrumentation and Detectors · Physics 2020-07-28 Ran Han , Qian Yu , Zhiwei Li , Jingtai Li , Yaping Cheng , Bin Liao , Lixiang Jiang , Sidao Ni , Tianfang Liu , Zheng Wang

CosmicWatch-based muon detectors are inexpensive, handheld, battery-powered, portable instruments designed to measure the flux of secondary muons produced when primary cosmic rays continuously strike the Earth's atmosphere. As these muons…

Instrumentation and Detectors · Physics 2026-05-07 Ishannita Banerjee , Swagato Banerjee , Douglas Jackson , John Naber

The underground muon detector of the Pierre Auger Observatory is aimed at attaining direct measurements of the muonic component of extensive air showers produced by cosmic rays with energy from $10^{16.5}$ eV up to the region of the ankle…

Instrumentation and Methods for Astrophysics · Physics 2021-09-01 A. M. Botti , F. Sánchez , M. Roth , A. Etchegoyen

Numerical weather prediction requires initial estimates of the atmospheric state. Since the atmospheric density field is intricately woven into the atmosphere's governing equations, advancing atmospheric density estimation will improve…

Atmospheric and Oceanic Physics · Physics 2025-09-08 William Luszczak , Man-Yau Chan

We demonstrate a scheme for direct absorption imaging of an ultracold ground-state polar molecular gas near quantum degeneracy. A challenge in imaging molecules is the lack of closed optical cycling transitions. Our technique relies on…

Quantum Gases · Physics 2015-05-18 D. Wang , B. Neyenhuis , M. H. G. de Miranda , K. -K. Ni , S. Ospelkaus , D. S. Jin , J. Ye

Muons serve as the best probes of the physics of hadronic interactions in the upper atmosphere because of their simple physics. All the properties of detected muons, such as their energy and angle of incidence, are governed by the…

High Energy Astrophysical Phenomena · Physics 2013-09-24 Dimitra Atri

Atmospheric muons play an important role in underwater/ice neutrino detectors. In this paper, a parameterisation of the flux of single and multiple muon events, their lateral distribution and of their energy spectrum is presented. The…

High Energy Physics - Phenomenology · Physics 2014-11-18 Y. Becherini , A. Margiotta , M. Sioli , M. Spurio

The characteristics of the partial nuclear muon capture with massive left-handed Dirac neutrino and relativistic component of the muon wave function have been derived. The multipole amplitudes are given as a function of neutrino mass…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Ciechanowicz , Z. Oziewicz , N. Popov

Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event yield in large-volume underground particle detectors. The IceCube detector, with an instrumented volume of about a cubic kilometer, has the…

High Energy Astrophysical Phenomena · Physics 2016-03-17 IceCube Collaboration , M. G. Aartsen , K. Abraham , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , T. Anderson , M. Archinger , C. Arguelles , T. C. Arlen , J. Auffenberg , X. Bai , S. W. Barwick , V. Baum , R. Bay , J. J. Beatty , J. Becker Tjus , K. -H. Becker , E. Beiser , S. BenZvi , P. Berghaus , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , M. Börner , F. Bos , D. Bose , S. Böser , O. Botner , J. Braun , L. Brayeur , H. -P. Bretz , N. Buzinsky , J. Casey , M. Casier , E. Cheung , D. Chirkin , A. Christov , B. Christy , K. Clark , L. Classen , S. Coenders , D. F. Cowen , A. H. Cruz Silva , J. Daughhetee , J. C. Davis , M. Day , J. P. A. M. de André , C. De Clercq , E. del Pino Rosendo , H. Dembinski , S. De Ridder , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , J. C. Díaz-Vélez , V. di Lorenzo , J. P. Dumm , M. Dunkman , R. Eagan , B. Eberhardt , T. Ehrhardt , B. Eichmann , S. Euler , P. A. Evenson , O. Fadiran , S. Fahey , A. R. Fazely , A. Fedynitch , J. Feintzeig , J. Felde , K. Filimonov , C. Finley , T. Fischer-Wasels , S. Flis , C. -C. Fösig , T. Fuchs , M. Glagla , T. K. Gaisser , R. Gaior , J. Gallagher , L. Gerhardt , K. Ghorbani , D. Gier , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , G. Golup , J. G. Gonzalez , D. Góra , D. Grant , P. Gretskov , J. C. Groh , A. Groß , C. Ha , C. Haack , A. Haj Ismail , A. Hallgren , F. Halzen , B. Hansmann , K. Hanson , D. Hebecker , D. Heereman , K. Helbing , R. Hellauer , D. Hellwig , S. Hickford , J. Hignight , G. C. Hill , K. D. Hoffman , R. Hoffmann , K. Holzapfe , A. Homeier , K. Hoshina , F. Huang , M. Huber , W. Huelsnitz , P. O. Hulth , K. Hultqvist , S. In , A. Ishihara , E. Jacobi , G. S. Japaridze , K. Jero , M. Jurkovic , B. Kaminsky , A. Kappes , T. Karg , A. Karle , M. Kauer , A. Keivani , J. L. Kelley , J. Kemp , A. Kheirandish , J. Kiryluk , J. Kläs , S. R. Klein , G. Kohnen , R. Koirala , H. Kolanoski , R. Konietz , A. Koob , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , K. Krings , G. Kroll , M. Kroll , J. Kunnen , N. Kurahashi , T. Kuwabara , M. Labare , J. L. Lanfranchi , M. J. Larson , M. Lesiak-Bzdak , M. Leuermann , J. Leuner , J. Lünemann , J. Madsen , G. Maggi , K. B. M. Mahn , R. Maruyama , K. Mase , H. S. Matis , R. Maunu , F. McNally , K. Meagher , M. Medici , A. Meli , T. Menne , G. Merino , T. Meures , S. Miarecki , E. Middell , E. Middlemas , J. Miller , L. Mohrmann , T. Montaruli , R. Morse , R. Nahnhauer , U. Naumann , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke , A. Olivas , A. Omairat , A. O'Murchadha , T. Palczewski , H. Pandya , L. Paul , J. A. Pepper , C. Pérez de los Heros , C. Pfendner , D. Pieloth , E. Pinat , J. Posselt , P. B. Price , G. T. Przybylski , J. Pütz , M. Quinnan , L. Rädel , M. Rameez , K. Rawlins , P. Redl , R. Reimann , M. Relich , E. Resconi , W. Rhode , M. Richman , S. Richter , B. Riedel , S. Robertson , M. Rongen , C. Rott , T. Ruhe , D. Ryckbosch , S. M. Saba , L. Sabbatini , H. -G. Sander , A. Sandrock , J. Sandroos , S. Sarkar , K. Schatto , F. Scheriau , M. Schimp , T. Schmidt , M. Schmitz , S. Schoenen , S. Schöneberg , A. Schönwald , A. Schukraft , L. Schulte , D. Seckel , S. Seunarine , R. Shanidze , M. W. E. Smith , D. Soldin , G. M. Spiczak , C. Spiering , M. Stahlberg , M. Stamatikos , T. Stanev , N. A. Stanisha , A. Stasik , T. Stezelberger , R. G. Stokstad , A. Stößl , E. A. Strahler , R. Ström , N. L. Strotjohann , G. W. Sullivan , M. Sutherland , H. Taavola , I. Taboada , S. Ter-Antonyan , A. Terliuk , G. Tešić , S. Tilav , P. A. Toale , M. N. Tobin , D. Tosi , M. Tselengidou , A. Turcati , E. Unger , M. Usner , S. Vallecorsa , N. van Eijndhoven , J. Vandenbroucke , J. van Santen , S. Vanheule , J. Veenkamp , M. Vehring , M. Voge , M. Vraeghe , C. Walck , M. Wallraff , N. Wandkowsky , Ch. Weaver , C. Wendt , S. Westerhoff , B. J. Whelan , N. Whitehorn , C. Wichary , K. Wiebe , C. H. Wiebusch , L. Wille , D. R. Williams , H. Wissing , M. Wolf , T. R. Wood , K. Woschnagg , D. L. Xu , X. W. Xu , Y. Xu , J. P. Yanez , G. Yodh , S. Yoshida , P. Zarzhitsky , M. Zoll

Measurements at 100 TeV and above are an important goal for the next generation of high energy gamma-ray astronomy experiments to solve the still open problem of the origin of galactic cosmic rays. The most natural experimental solution to…

Astrophysics · Physics 2007-10-11 G. Di Sciascio , T. Di Girolamo , E. Rossi , L. Saggese

Since its discovery in the 1930s, the muon has played an important role in our quest to understand the sub-atomic theory of matter. The muon was the first second-generation standard-model particle to be discovered, and its decay has…

High Energy Physics - Experiment · Physics 2008-11-26 B. Lee Roberts

Ghost imaging is an unconventional imaging technique that generates high resolution images by correlating the intensity of two light beams, neither of which independently contains useful information about the shape of the object. Ghost…

We present a novel underground imaging system that utilizes cosmic-ray muons to explore the subsurface environment at the City of David archaeological site in ancient Jerusalem. This report details the initial findings from measurements…

Traditional ghost imaging acquires images via the correlation of the intensity fluctuations of reference patterns and bucket values, and can even generate positive-negative images by conditionally averaging partial patterns. Here, we…

Image and Video Processing · Electrical Eng. & Systems 2019-11-19 Ya-Xin Li , Wen-Kai Yu , Shuo-Fei Wang

Muons from cosmic-ray interactions in the atmosphere provide a high-statistics source of particles that can be used to study the performance and calibration of the ATLAS detector. Cosmic-ray muons can penetrate to the cavern and deposit…

Instrumentation and Detectors · Physics 2012-08-27 The ATLAS Collaboration

In the previous part I, we have developed the generalized theory of the probability tomography method to image polar and dipolar sources of a vector or scalar geophysical anomaly field. The purpose of the new method was to improve the…

Geophysics · Physics 2011-12-30 Paolo Mauriello , Domenico Patella

Cosmic rays interact with nuclei in the Earth's atmosphere to produce extensive air showers, which give rise to the atmospheric muon flux. Temperature fluctuations in the atmosphere influence the rate of muons measured in deep underground…

High Energy Physics - Phenomenology · Physics 2025-09-23 Amanda Alves , Lilly Pyras , Dennis Soldin , Stef Verpoest
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