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Status and prospects of the ultrahigh energy cosmic rays

Maria Giller

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This paper summarizes measurement results of the UHECR energy spectrum and arrival directions. Various scenarios trying to explain the flat AGASA spectrum (no GZK cutoff) are recalled. Recent HiRes data are, however, consistent with the expected GZK cutoff, so that for E > 1020 eV the fluxes measured by the two experiments diverge by more than one order of magnitude. The multiple events, observed by AGASA, seem not to be statistical fluctuations and we analyse the information contained in them. The Pierre Auger Observatory (in construction) is expected to dispel the doubts about existence of the GZK cutoff as well as those about the nature of the multiplets.


PACS

96.50.sb Composition, energy spectra and interactions

96.50.sd Extensive air showers

95.30.Cq Elementary particle processes

96.50.sh Interplanetary propagation and effects

Subjects

Particle physics and field theory

Astrophysics and astroparticles

Dates

Issue 5 (May 2003)

Received 20 November 2002, in final form 12 December 2002

Published 9 April 2003



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