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On the measurement of the proton-air cross section using longitudinal shower profiles

Ralf Ulrich, Johannes Blümer, Ralph Engel, Fabian Schüssler, Michael Unger

astro-pharXiv:astro-ph/0612205

Abstract

In this paper, we will discuss the prospects of deducing the proton-air cross section from fluorescence telescope measurements of extensive air showers. As it is not possible to observe the point of first interaction X 1 directly, other observables closely linked to X 1 must be inferred from the longitudinal profiles. This introduces a dependence on the models used to describe the shower development. The most straightforward candidate for a good correlation to X 1 is the depth of shower maximum X max. We will discuss the sensitivity of an X max-based analysis on σ p-air and quantify the systematic uncertainties arising from the model dependence, parameters of the reconstruction method itself and a possible non-proton contamination of the selected shower sample.

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