Geant4 simulation of production and interaction of muons
Autor: | Helmut Burkhardt, S.R. Kelner, Alexey Bogdanov, M. Maire, L. Urbán, R. P. Kokoulin, Vladimir Ivanchenko, A.M. Rybin |
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Přispěvatelé: | Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), GEANT4 |
Rok vydání: | 2006 |
Předmět: |
Nuclear and High Energy Physics
Particle physics Physics::Instrumentation and Detectors Astrophysics::High Energy Astrophysical Phenomena Cosmic ray 01 natural sciences 7. Clean energy [PHYS.PHYS.PHYS-COMP-PH]Physics [physics]/Physics [physics]/Computational Physics [physics.comp-ph] Nuclear physics Pion 0103 physical sciences Electrical and Electronic Engineering 010306 general physics Particle Physics - Phenomenology Physics Annihilation Muon Large Hadron Collider 010308 nuclear & particles physics Bremsstrahlung Pair production Nuclear Energy and Engineering Muon collider Nuclear Physics - Theory Physics::Accelerator Physics High Energy Physics::Experiment |
Zdroj: | IEEE Transactions on Nuclear Science IEEE Transactions on Nuclear Science, Institute of Electrical and Electronics Engineers, 2006, 53, pp.513-519. ⟨10.1109/TNS.2006.872633⟩ |
ISSN: | 0018-9499 |
DOI: | 10.1109/tns.2006.872633 |
Popis: | A set of models for Monte Carlo simulation of production and interaction of high energy muons is developed in the framework of the Geant4 toolkit. It describes the following physics processes: ionization of high energy muons with radiative corrections, bremsstrahlung, electron-positron pair production, muon induced nuclear reactions, gamma annihilation into muon pair, positron annihilation into muon pair, and into pion pair. These processes are essential for the LHC experiments, for the understanding of the background in underground detectors, for the simulation of effects related with high-energy muons in cosmic ray experiments and for the estimation of backgrounds in future colliders. The applicability area of the models extends to 1 PeV. The major use-cases are discussed. |
Databáze: | OpenAIRE |
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