English
Related papers

Related papers: COME: Cylindrical oriented muon emission in GEANT4…

200 papers

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

The Muon Ionization Cooling Experiment (MICE) collaboration seeks to demonstrate the feasibility of ionization cooling, the technique by which it is proposed to cool the muon beam at a future neutrino factory or muon collider. The emittance…

Accelerator Physics · Physics 2019-03-27 The MICE Collaboration , D. Adams , D. Adey , R. Asfandiyarov , G. Barber , A. de Bari , R. Bayes , V. Bayliss , R. Bertoni , V. Blackmore , A. Blondel , J. Boehm , M. Bogomilov , M. Bonesini , C. N. Booth , D. Bowring , S. Boyd , T. W. Bradshaw , A. D. Bross , C. Brown , L. Coney , G. Charnley , G. T. Chatzitheodoridis , F. Chignoli , M. Chung , D. Cline , J. H. Cobb , D. Colling , N. Collomb , P. Cooke , M. Courthold , L. M. Cremaldi , A. DeMello , A. J. Dick , A. Dobbs , P. Dornan , F. Drielsma , K. Dumbell , M. Ellis , F. Filthaut , P. Franchini , B. Freemire , A. Gallagher , R. Gamet , R. B. S. Gardener , S. Gourlay , A. Grant , J. R. Greis , S. Griffiths , P. Hanlet , G. G. Hanson , T. Hartnett , C. Heidt , P. Hodgson , C. Hunt , S. Ishimoto , D. Jokovic , P. B. Jurj , D. M. Kaplan , Y. Karadzhov , A. Klier , Y. Kuno , A. Kurup , P. Kyberd , J-B. Lagrange , J. Langlands , W. Lau , D. Li , Z. Li , A. Liu , K. Long , T. Lord , C. Macwaters , D. Maletic , B. Martlew , J. Martyniak , R. Mazza , S. Middleton , T. A. Mohayai , A. Moss , A. Muir , I. Mullacrane , J. J. Nebrensky , D. Neuffer , A. Nichols , J. C. Nugent , A. Oates , D. Orestano , E. Overton , P. Owens , V. Palladino , M. Palmer , J. Pasternak , V. Pec , C. Pidcott , M. Popovic , R. Preece , S. Prestemon , D. Rajaram , S. Ricciardi , M. Robinson , C. Rogers , K. Ronald , P. Rubinov , H. Sakamoto , D. A. Sanders , A. Sato , M. Savic , P. Snopok , P. J. Smith , F. J. P. Soler , Y. Song , T. Stanley , G. Stokes , V. Suezaki , D. J. Summers , C. K. Sung , J. Tang , J. Tarrant , I. Taylor , L. Tortora , Y. Torun , R. Tsenov , M. Tucker , M. A. Uchida , S. Virostek , G. Vankova-Kirilova , P. Warburton , S. Wilbur , A. Wilson , H. Witte , C. White , C. G. Whyte , X. Yang , A. R. Young , M. Zisman

An intense beam of muons is needed to provide a luminosity on the order of 10$^{34}$ cm$^{-2}$s$^{-1}$ for a multi-TeV collider. Because muons produced by colliding a multi-MW proton beam with a target made of carbon or mercury have a large…

We follow a model based on the SU(8) symmetry for the interaction of mesons with baryons. The model treats on an equal footing the pseudo-scalars and the vector mesons, as required by heavy quark symmetry. The T-matrix calculated within an…

High Energy Physics - Phenomenology · Physics 2011-03-17 D. Gamermann , C. García-Recio , J. Nieves , L. L. Salcedo , L. Tolos

We present low energy recoil detection results in the keV energy region, from measurements performed with the Spherical Proportional Counter (SPC). An ${}^{241}Am-{}^{9}{Be}$ fast neutron source is used in order to obtain neutron-nucleus…

Instrumentation and Detectors · Physics 2017-09-20 I. Savvidis , I. Katsioulas , C. Eleftheriadis , I. Giomataris , T. Papaevangellou

We compute deep-sea energy spectra and zenith-angle distributions of the atmospheric muons, both conventional and prompt. The prompt muon contribution to the muon flux underwater is calculated taking into consideration predictions of recent…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Misaki , T. S. Sinegovskaya , S. I. Sinegovsky , N. Takahashi

A new physics-based compact model, which makes it possible to simulate in a unified way the neutron and proton of cosmic ray induced SEU cross sections, including effects from nuclear reaction products and from direct ionization by…

Muons are copiously produced within hadronic extensive air showers (EAS) occurring in the Earth's atmosphere, and are used by particle air shower detectors as a means of identifying the primary cosmic ray which initiated the EAS. Imaging…

Instrumentation and Methods for Astrophysics · Physics 2019-04-10 A. M. W. Mitchell , H. P. Dembinski , R. D. Parsons

A model to describe the output particle distribution generated by particles impinging on a planar target has been developed. This model was developed to simulate positron production in the Cornell CESR Linac but can be applied to targets…

Accelerator Physics · Physics 2022-01-03 John Mastroberti , David Sagan , Jim Shanks

Neutrino telescopes are opening new opportunities in observational high energy astrophysics. In these detectors, atmospheric muons from primary cosmic ray interactions in the atmosphere play an important role. They provide the most abundant…

Instrumentation and Methods for Astrophysics · Physics 2009-08-03 G. Carminati , M. Bazzotti , S. Biagi , S. Cecchini , T. Chiarusi , A. Margiotta , M. Sioli , M. Spurio

The proposed work demonstrates the results of creating and investigating the mathematical model of the source of fast neutrons. The model carrier is a computer program developed in the C++ programming language in the Linux operating system…

Computational Physics · Physics 2020-01-30 Tetiana Malykhina , Viktoriia Lisovska , Valentina Shpagina , Ruslan Timchenko

Neutrino telescopes will open, in the next years, new opportunities in observational high energy astrophysics. For these experiments, atmospheric muons from primary cosmic ray interactions in the atmosphere play an important role, because…

Instrumentation and Detectors · Physics 2009-01-01 G. Carminati , A. Margiotta , M. Spurio

The FASER experiment was designed to study long-lived dark sector particles and neutrinos traveling in the forward direction at the LHC. Neutrinos are predominantly produced from meson decays, which also result in an intense energetic flux…

High Energy Physics - Phenomenology · Physics 2025-07-29 Roshan Mammen Abraham , Max Fieg

Due to the high penetrating power of cosmic ray muons, they can be used to probe very thick and dense objects. As charged particles, they can be tracked by ionization detectors, determining the position and direction of the muons. With…

Image and Video Processing · Electrical Eng. & Systems 2024-10-11 Jesus J. Valencia , Adam A. Hecht , C. L. Morris , E. Guardincerri , D. Poulson , J. Bacon , J. M. Durham

We present a search for the production of excited or exotic muons (mu*) via the reaction pbar + p -> mu* + mu -> mu gamma + mu using 371/pb of data collected with the Run II CDF detector. In this signature-based search, we look for a…

High Energy Physics - Experiment · Physics 2007-05-23 Heather Gerberich , Christopher Hays , Ashutosh Kotwal

In extensive air shower experiments, the number of muons crossing a detector at a given position, as well as their arrival time, arrival direction, and energy, are determined by a more fundamental 3-dimensional distribution linked to the…

High Energy Physics - Phenomenology · Physics 2023-03-15 Lorenzo Cazon , Rúben Conceição , Felix Riehn

The international Muon Ionization Cooling Experiment (MICE) aims to demonstrate muon beam ionization cooling for the first time and constitutes a key part of the R&D towards a future neutrino factory or muon collider. Beam cooling reduces…

Accelerator Physics · Physics 2019-08-15 Tanaz Angelina Mohayai , Pavel Snopok , David Neuffer , Chris Rogers

Muon beams of low emittance provide the basis for the intense, well-characterised neutrino beams of a neutrino factory and for multi-TeV lepton-antilepton collisions at a muon collider. The international Muon Ionization Cooling Experiment…

Accelerator Physics · Physics 2021-08-18 The MICE collaboration , M. Bogomilov , R. Tsenov , G. Vankova-Kirilova , Y. P. Song , J. Y. Tang , Z. H. Li , R. Bertoni , M. Bonesini , F. Chignoli , R. Mazza , V. Palladino , A. de Bari , D. Orestano , L. Tortora , Y. Kuno , H. Sakamoto , A. Sato , S. Ishimoto , M. Chung , C. K. Sung , F. Filthaut , M. Fedorov , D. Jokovic , D. Maletic , M. Savic , N. Jovancevic , J. Nikolov , M. Vretenar , S. Ramberger , R. Asfandiyarov , A. Blondel , F. Drielsma , Y. Karadzhov , G. Charnley , N. Collomb , K. Dumbell , A. Gallagher , A. Grant , S. Griffiths , T. Hartnett , B. Martlew , A. Moss , A. Muir , I. Mullacrane , A. Oates , P. Owens , G. Stokes , P. Warburton , C. White , D. Adams , V. Bayliss , J. Boehm , T. W. Bradshaw , C. Brown , M. Courthold , J. Govans , M. Hills , J. -B. Lagrange , C. Macwaters , A. Nichols , R. Preece , S. Ricciardi , C. Rogers , T. Stanley , J. Tarrant , M. Tucker , S. Watson , A. Wilson , R. Bayes , J. C. Nugent , F. J. P. Soler , R. Gamet , P. Cooke , V. J. Blackmore , D. Colling , A. Dobbs , P. Dornan , P. Franchini , C. Hunt , P. B. Jurj , A. Kurup , K. Long , J. Martyniak , S. Middleton , J. Pasternak , M. A. Uchida , J. H. Cobb , C. N. Booth , P. Hodgson , J. Langlands , E. Overton , V. Pec , P. J. Smith , S. Wilbur , G. T. Chatzitheodoridis , A. J. Dick , K. Ronald , C. G. Whyte , A. R. Young , S. Boyd , J. R. Greis , T. Lord , C. Pidcott , I. Taylor , M. Ellis , R. B. S. Gardener , P. Kyberd , J. J. Nebrensky , M. Palmer , H. Witte , D. Adey , A. D. Bross , D. Bowring , P. Hanlet , A. Liu , D. Neuffer , M. Popovic , P. Rubinov , A. DeMello , S. Gourlay , A. Lambert , D. Li , T. Luo , S. Prestemon , S. Virostek , B. Freemire , D. M. Kaplan , T. A. Mohayai , D. Rajaram , P. Snopok , Y. Torun , L. M. Cremaldi , D. A. Sanders , D. J. Summers , L. R. Coney , G. G. Hanson , C. Heidt

Precision spectroscopy of the Muonium Lamb shift and fine structure requires a robust source of 2S Muonium. To date, the beam-foil technique is the only demonstrated method for creating such a beam in vacuum. Previous experiments using this…

High Energy Physics - Experiment · Physics 2020-09-07 G. Janka , B. Ohayon , Z. Burkley , L. Gerchow , N. Kuroda , X. Ni , R. Nishi , Z. Salman , A. Suter , M. Tuzi , C. Vigo , T. Prokscha , P. Crivelli