arXiv · hep-ph/9802384
Proton-proton Cross Section at sqrt(s) \sim 30 TeV
Abstract
There are both theoretical and experimental uncertainties in using data from cosmic-ray air showers to estimate hadronic cross sections above accelerator energies. We outline these problems and compare the physics used to extract σ_{pp}^{tot} from air shower data to the widely used parameterization of the proton-proton cross section of Donnachie and Landshoff and other contemporary models. We conclude that the published cosmic-ray cross section values do not strongly constrain σ_{pp}^{tot} fits from lower energy accelerator data.
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Ralph Engel, T. K. Gaisser, Paolo Lipari, Todor Stanev. 1998-02-20. Proton-proton Cross Section at sqrt(s) \sim 30 TeV. https://doi.org/10.1103/physrevd.58.014019
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