会议论文详细信息
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
来源: IOP
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【 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.

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