6th School on Cosmic Rays and Astrophysics | |
Cosmic-ray physics at CERN | |
Rodríguez Cahuantzi, M.^1 | |
Faculty of Physics and Mathematics, Autonomous University of Puebla, Ciudad Universitaria, Av. San Claudio y 18 Sur, Edif. EMA3-231, Puebla | |
72570, Mexico^1 | |
关键词: Atmospheric muons; Collider detectors; Large amounts; Large Hadron collider LHC; LHC experiments; Me-xico; Theoretical physics; | |
Others : https://iopscience.iop.org/article/10.1088/1742-6596/866/1/012013/pdf DOI : 10.1088/1742-6596/866/1/012013 |
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来源: IOP | |
【 摘 要 】
Accelerator experiments located underground are suitable for the study of atmospheric muons. The use of high-energy collider detectors for cosmic-ray physics was pioneered during the era of the Large Electron-Positron (LEP) collider at CERN by ALEPH, DELPHI and L3 collaborations. A development of these programs is possible at the Large Hadron Collider (LHC), where experiments like ALICE and CMS will operate for many years, with the possibility of recording a large amount of cosmic-ray data. In this proceedings, a review of the results obtained by LEP and LHC experiments is presented. This material was discussed along two sessions during the VI School on Cosmic-ray Physics and Astrophysics held at the Mesoamerican Center for Theoretical Physics (MCTP) located in Tuxtla Gutierrez, Chiapas, Mexico.
【 预 览 】
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Cosmic-ray physics at CERN | 1362KB | download |