Measurements of the proton-air cross section with high energy cosmic ray experiments

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 ener...

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Main Author: Abbasi Rasha
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201612004005
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author Abbasi Rasha
author_facet Abbasi Rasha
author_sort Abbasi Rasha
collection DOAJ
description 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.
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spelling doaj.art-b788ae3c663d44f1a15844d11bbfea9e2022-12-21T18:40:30ZengEDP SciencesEPJ Web of Conferences2100-014X2016-01-011200400510.1051/epjconf/201612004005epjconf_ismd2016_04005Measurements of the proton-air cross section with high energy cosmic ray experimentsAbbasi Rasha0Department of Physics and Astronomy at the University of UtahDetecting 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.http://dx.doi.org/10.1051/epjconf/201612004005
spellingShingle Abbasi Rasha
Measurements of the proton-air cross section with high energy cosmic ray experiments
EPJ Web of Conferences
title Measurements of the proton-air cross section with high energy cosmic ray experiments
title_full Measurements of the proton-air cross section with high energy cosmic ray experiments
title_fullStr Measurements of the proton-air cross section with high energy cosmic ray experiments
title_full_unstemmed Measurements of the proton-air cross section with high energy cosmic ray experiments
title_short Measurements of the proton-air cross section with high energy cosmic ray experiments
title_sort measurements of the proton air cross section with high energy cosmic ray experiments
url http://dx.doi.org/10.1051/epjconf/201612004005
work_keys_str_mv AT abbasirasha measurementsoftheprotonaircrosssectionwithhighenergycosmicrayexperiments