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Related papers: Cosmic Ray Muons in Laboratories Deep Underground

200 papers

The Deep Underground Neutrino Experiment (DUNE) is a project to design, construct and operate a next-generation long-baseline neutrino detector with a liquid argon (LAr) target capable also of searching for proton decay and supernova…

Instrumentation and Detectors · Physics 2016-06-22 Vitaly A. Kudryavtsev

We present the result of a search for correlations in the arrival times of high energy muons collected from 1995 till 2000 with the streamer tube system of the complete MACRO detector at the underground Gran Sasso Lab. Large samples of…

The results presented at the 28th International Cosmic Ray Conference on neutrino and muon physics are summarized. Neutrinos and muons provide a huge amount of information on particle interactions up to very high energies and on fundamental…

High Energy Physics - Phenomenology · Physics 2007-05-23 Teresa Montaruli

X-ray computed tomography (CT) has an indispensable role in constructing 3D images of objects made from light materials. However, limited by absorption coefficients, X-rays cannot deeply penetrate materials such as copper and lead. Here we…

Instrumentation and Detectors · Physics 2015-01-29 Burkhant Suerfu , Christopher G. Tully

The MUon RAdiography of VESuvius (MURAVES) project aims at the study of the summital cone of Mt. Vesuvius, an active volcano near Naples (Italy), by measuring its density profile through muon flux attenuation. Its data, combined with those…

Upward throughgoing muons in underground detectors are induced by atmospheric $\nu_\mu$ with energies in the $1-10^4 GeV$ range. The oscillations of atmospheric muon neutrinos should affect mainly those with energy smaller than $E_\nu \sim…

High Energy Physics - Experiment · Physics 2007-05-23 D. Bakari , Y. Becherini , M. Spurio

KM3NeT is a research infrastructure located in the Mediterranean Sea, that will consist of two deep-sea Cherenkov neutrino detectors. With one detector (ARCA), the KM3NeT Collaboration aims at identifying and studying TeV-PeV astrophysical…

Instrumentation and Detectors · Physics 2020-02-28 KM3NeT Collaboration , M. Ageron , S. Aiello , F. Ameli , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , J. Aublin , C. Bagatelas , G. Barbarino , B. Baret , S. Basegmez du Pree , A. Belias , E. Berbee , A. M. van den Berg , V. Bertin , V. van Beveren , S. Biagi , A. Biagioni , S. Bianucci , M. Billault , M. Bissinger , R. de Boer , J. Boumaaza , S. Bourret , M. Bouta , M. Bouwhuis , C. Bozza , H. Brânzaş , M. Briel , M. Bruchner , R. Bruijn , J. Brunner , E. Buis , R. Buompane , J. Busto , G. Cacopardo , L. Caillat , C. Calì , D. Calvo , A. Capone , S. Celli , M. Chabab , N. Chau , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , S. Colonges , R. Coniglione , A. Cosquer , P. Coyle , A. Creusot , G. Cuttone , C. D'Amato , A. D'Amico , A. D'Onofrio , R. Dallier , M. De Palma , C. De Sio , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , R. Donà , C. Donzaud , L. van Dooren , D. Dornic , M. Dörr , M. Durocher , T. Eberl , T. van Eeden , I. El Bojaddaini , H. Eljarrari , D. Elsaesser , A. Enzenhöfer , P. Fermani , G. Ferrara , M. D. Filipović , L. A. Fusco , D. Gajanana , T. Gal , A. Garcia Soto , F. Garufi , L. Gialanella , E. Giorgio , A. Giuliante , S. R. Gozzini , R. Gracia , K. Graf , D. Grasso , T. Grégoire , G. Grella , A. Grimaldi , A. Grmek , D. Guderian , M. Guerzoni , C. Guidi , S. Hallmann , H. Hamdaoui , H. van Haren , A. Heijboer , A. Hekalo , S. Henry , J. J. Hernández-Rey , J. Hofestädt , F. Huang , E. Huesca Santiago , G. Illuminati , C. W. James , P. Jansweijer , M. Jongen , M. de Jong , P. de Jong , M. Kadler , P. Kalaczyński , O. Kalekin , U. F. Katz , F. Kayzel , P. Keller , N. R. Khan Chowdhury , F. van der Knaap , E. N. Koffeman , P. Kooijman , J. Koopstra , A. Kouchner , M. Kreter , V. Kulikovskiy , Meghna K. K. , R. Lahmann , P. Lamare , G. Larosa , J. Laurence , R. Le Breton , F. Leone , E. Leonora , G. Levi , F. Librizzi , M. Lincetto , P. Litrico , C. D. Llorens Alvarez , A. Lonardo , F. Longhitano , D. Lopez-Coto , G. Maggi , J. Mańczak , K. Mannheim , A. Margiotta , A. Marinelli , C. Markou , L. Martin , J. A. Martínez-Mora , A. Martini , F. Marzaioli , R. Mele , K. W. Melis , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Mongelli , M. Morganti , M. Moser , A. Moussa , R. Muller , P. Musico , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , C. Nielsen , B. Ó Fearraigh , M. Organokov , A. Orlando , V. Panagopoulos , G. Pancaldi , G. Papalashvili , R. Papaleo , C. Pastore , G. E. Păvălaş , G. Pellegrini , C. Pellegrino , M. Perrin-Terrin , P. Piattelli , K. Pikounis , O. Pisanti , C. Poirè , G. Polydefki , V. Popa , M. Post , T. Pradier , G. Pühlhofer , S. Pulvirenti , L. Quinn , F. Raffaelli , N. Randazzo , A. Rapicavoli , S. Razzaque , D. Real , S. Reck , J. Reubelt , G. Riccobene , L. Rigalleau , G. Rizza , R. Rocco , A. Rovelli , J. Royon , M. Salemi , I. Salvadori , D. F. E. Samtleben , A. Sánchez Losa , M. Sanguineti , A. Santangelo , D. Santonocito , P. Sapienza , J. Schmelling , V. Sciacca , D. Sciliberto , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , F. Simeone , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , J. Steijger , S. M. Stellacci , B. Strandberg , D. Stransky , T. Stüven , M. Taiuti , Y. Tayalati , E. Tenllado , D. Tézier , T. Thakore , S. Theraube , P. Timmer , S. Tingay , A. Trovato , S. Tsagkli , E. Tzamariudaki , D. Tzanetatos , C. Valieri , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , G. de Wasseige , J. Wilms , R. Wojaczyński , E. de Wolf , D. Zaborov , A. Zegarelli , J. D. Zornoza , J. Zúñiga

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…

Neutrons produced by cosmic muon interactions are important contributors to backgrounds in underground detectors when searching for rare events. Typically such neutrons can dominate the background, as they are particularly difficult to…

Instrumentation and Methods for Astrophysics · Physics 2015-06-22 A Empl , E. V. Hungerford , R. Jasim , P. Mosteiro

The flux of muons induced by atmospheric neutrinos has been measured with the MACRO detector. Different event topologies have been detected, due to neutrino interactions in the apparatus and in the rock below it. The upward-throughgoing…

High Energy Physics - Experiment · Physics 2007-05-23 Paolo Bernardini

Muography is an imaging tool based on the attenuation of cosmic muons to observe the density distribution of large objects, such as underground caves or fractured zones. Tomography based on muography measurements -- that is, three…

In this work, we describe the calibration and first measurements in the commissioning of MuTe, a hybrid Muon Telescope with two subdetectors --a scintillator hodoscope and a Water Cherenkov Detector (WCD)-- for imaging the inner structures…

Deep neural networks are a powerful technique that have found ample applications in several branches of Physics. In this work, we apply machine learning algorithms to a specific problem of Cosmic Ray Physics: the estimation of the muon…

Instrumentation and Methods for Astrophysics · Physics 2019-04-10 A. Guillen , A. Bueno , J. M. Carceller , J. C. Martinez-Velazquez , G. Rubio , C. J. Todero Peixoto , P. Sanchez-Lucas

In this paper, we present a refined calculation of the atmospheric neutrino flux spanning from GeV to PeV energies. Our method, Daemonflux, utilizes data-driven inputs and incorporates adjustable parameters to take their uncertainties into…

High Energy Physics - Phenomenology · Physics 2023-08-29 Juan Pablo Yañez , Anatoli Fedynitch

High-energy muons from air shower events detected in IceCube are selected using state of the art machine learning algorithms. Attributes to distinguish a HE-muon event from the background of low-energy muon bundles are selected using the…

Instrumentation and Methods for Astrophysics · Physics 2017-01-17 Tomasz Fuchs

In this paper we study the sensitivity of the flux of atmospheric muons to uncertainties in the primary cosmic ray spectrum and to the treatment of the geomagnetic field in a calculation. We use the air shower simulation program AIRES to…

Astrophysics · Physics 2008-11-26 P. Hansen , T. K. Gaisser , T. Stanev , S. J. Sciutto

The IceCube detector allows for the first time a measurement of atmospheric muon and neutrino energy spectra from tens of GeV up to the PeV range. The lepton flux in the highest energy region depends on both the primary cosmic ray…

High Energy Astrophysical Phenomena · Physics 2019-08-13 P. Berghaus

The results obtained by studying the background of neutrons produced by cosmic-ray muons in underground experimental facilities intended for rare-event searches and in surrounding rock are presented. The types of this rock may include…

Instrumentation and Detectors · Physics 2017-03-21 K. V. Manukovsky , O. G. Ryazhskaya , N. M. Sobolevsky , A. V. Yudin

We evaluated rates of transversing muons, muon-induced fast neutrons, and production of $^{40}$Cl and other cosmogenically produced nuclei that pose as potential sources of background to the physics program proposed for an argon-based long…

Instrumentation and Detectors · Physics 2013-05-30 D. Barker , D. -M. Mei , C. Zhang

The proposed ICAL detector at INO is a large sized underground magnetized iron detector. ICAL is designed to reconstruct muon momentum using magnetic spectrometers. Energy measurement using magnets fail for muons in TeV range, since the…

Instrumentation and Detectors · Physics 2019-05-21 Jaydip Singh , Srishti Nagu , Jyotsna Singh