Chemical Composition of Ultra-High Energy Cosmic Rays Observed by AGASA

Physics

Scientific paper

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Scientific paper

We have observed ultra-high energy cosmic rays above the Greisen-ZatsepinKuz'min cut-off energy by Akeno Giant Air Shower Array. Their chemical composition is a key discriminator of origin models. In the present work, we estimate the average composition by an analysis of muons in air showers with AIRES+QGSJET simulation. The data matches the prediction for light hadron primaries and no indication has been found for a gamma-ray dominance.

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