Unique Properties of the 3rd group of cosmic rays: Results from the Alpha Magnetic Spectrometer

26 Aug 2025, 17:30
20m
Conference Room F1-R2

Conference Room F1-R2

Oral High-Energy Astrophysics and Cosmic Rays High-Energy Astrophysics and Cosmic Rays

Speaker

诚 张 (中国科学院高能物理研究所)

Description

We report the latest results on the properties of C, N, Ne, Na,Mg, Al, S, Cl, Ar, K, and Ca cosmic rays fluxes in the rigidity range 2.5 GV to 3 TV collected by the AMS furing first 13.5 years of operation. We observe that fluxes are well described by the sums of a primary cosmic ray component and a secondary cosmic ray component. With our measurements, the abundance ratios at the source C/O, N/O, Ne/Si, Na/Si, Mg/Si, Al/Si, S/Si, Cl/Si, Ar/Si, K/Si, and Ca/Si are determined independent of cosmic ray propagation.

Collaboration you are representing AMS collaboration

Author

诚 张 (中国科学院高能物理研究所)

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