AGASA Results and the Status of TA

Details AGASA Results and the Status of TA AGASA Results and the Status of TA

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf....1f&link_type=abstract

Energy Budget in the High Energy Universe: Proceedings of the International Workshop held 22-24 February, 2006, in Kashiwa, Japa

Physics

1

Scientific paper

The Akeno Giant Air Shower Array (AGASA) had observed 11 events of Extremely-High Energy Cosmic Rays (EHECRs) with energies exceeding 1020eV. The energy of these cosmic rays is beyond the Gleisen-Zatsepin-Kuzmin (GZK) cutoff expected by the interaction of EHE protons with the Cosmic Microwave Background (CMB). New experiments with much larger acceptance and improved energy determination, Telescope Array (TA) experiment and Pierre Auger observatory are being built to confirm the existence of EHECRs and to understand their origin.

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