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arxiv: astro-ph/9807193 · v1 · pith:UGVKXE2Hnew · submitted 1998-07-18 · 🌌 astro-ph

Extension of the Cosmic-Ray Energy Spectrum Beyond the Predicted Greisen-Zatsepin-Kuz'min Cutoff

classification 🌌 astro-ph
keywords energyspectrumbeyondcutoffcosmic-rayaboveabsenceagasa
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The cosmic-ray energy spectrum above 10^{18.5} eV is reported using the updated data set of the Akeno Giant Air Shower Array (AGASA) from February 1990 to October 1997. The energy spectrum extends beyond 10^{20} eV and the energy gap between the highest energy event and the others is being filled up with recently observed events. The spectral shape suggests the absence of the 2.7 K cutoff in the energy spectrum or a possible presence of a new component beyond the 2.7 K cutoff.

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