Chemical Composition of Ultrahigh-Energy Cosmic Rays from the Telescope Array Surface Detector Data


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Resumo

Results are presented from investigating the chemical composition of ultrahigh-energy cosmic rays using data from the Telescope Array experiment, obtained at its surface detector array over nine years. The analysis is based on the boosted decision tree approach, which uses 14 observables sensitive to the composition of cosmic rays.

Sobre autores

Ya. Zhezher

Institute for Nuclear Research, Russian Academy of Sciences; Faculty of Physics, Moscow State University

Autor responsável pela correspondência
Email: zhezher.yana@physics.msu.ru
Rússia, Moscow, 142190; Moscow, 119991

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