EPJ Web of Conferences
Volume 120, 2016XLV International Symposium on Multiparticle Dynamics (ISMD 2015)
|Number of page(s)||7|
|Section||4 Astroparticle Physics|
|Published online||04 July 2016|
Measurements of the proton-air cross section with high energy cosmic ray experiments
Department of Physics and Astronomy at the University of Utah
a e-mail: email@example.com
Published online: 4 July 2016
Detecting Ultra High Energy Cosmic Rays (UHECRs) enables us to measure the proton-air inelastic cross section σinel p–air at energies that we are unable to access with particle accelerators. The proton-proton cross section σp–p is subsequently inferred from the proton-air cross section at these energies. UHECR experiments have been reportingon the proton-air inelastic cross section starting with the Fly’s Eye in 1984 at √s =30 TeV and ending with the most recent result of the Telescope Array experiment at √s = 95 TeV in 2015. In this proceeding, I will summarize the most recent experimental results on the σinel p–air measurements from the UHECR experiments.
© Owned by the authors, published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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