17–24 Jul 2024
Prague
Europe/Prague timezone

Cosmic Anti-Protons and Properties of Elementary Particle Fluxes

19 Jul 2024, 08:30
20m
South Hall 2B

South Hall 2B

Parallel session talk 08. Astro-particle Physics and Cosmology Astro-particle Physics and Cosmology

Speaker

Cheng Zhang (Institute of High Energy Physics,Chinese Academy of Sciences(CN))

Description

Precision measurements by AMS reveal unique properties of cosmic charged elementary particles. In the absolute rigidity range ~60 to ~500 GV, the antiproton flux and proton flux have nearly identical rigidity dependence. This behavior indicates an excess of high energy antiprotons compared with secondary antiprotons produced from the collision of cosmic rays. More importantly, from ~60 to ~500 GV the antiproton flux and positron flux show identical rigidity dependence. The positron-to-antiproton flux ratio is independent of energy and its value is determined to be a factor of 2 with percent accuracy. This unexpected observation indicates a common origin of high energy antiprotons and positrons in the cosmos.

Alternate track 09. Dark Matter Detection
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Author

Cheng Zhang (Institute of High Energy Physics,Chinese Academy of Sciences(CN))

Presentation materials