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Observation of the suppression of the flux of cosmic rays above 4 x 10 (19) eV.

Abstract:
The energy spectrum of cosmic rays above 2.5 x 10;{18} eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index gamma of the particle flux, J proportional, variantE;{-gamma}, at energies between 4 x 10;{18} eV and 4 x 10;{19} eV is 2.69+/-0.02(stat)+/-0.06(syst), steepening to 4.2+/-0.4(stat)+/-0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.
Publication status:
Published

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Publisher copy:
10.1103/physrevlett.101.061101

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Journal:
Physical Review Letters More from this journal
Volume:
101
Issue:
6
Pages:
061101
Publication date:
2008-08-01
DOI:
EISSN:
1079-7114
ISSN:
0031-9007


Language:
English
Keywords:
Pubs id:
pubs:5997
UUID:
uuid:1f7fbc63-c89d-49f6-a7ce-bfc8b789a0c3
Local pid:
pubs:5997
Source identifiers:
5997
Deposit date:
2012-12-19
ARK identifier:

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