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Name : | Angela V. Olinto |
Institute : | University of Chicago |
E-mail : | olinto@oddjob.uchicago.edu |
TITLE : | Origin of Super GZK particles |
ABSTRACT : | |
| Contrary to expectations, several cosmic ray events with energies
above $10^{20}$ eV have been observed. The flux of such events is well
above the predicted Greisen-Zatsepin-Kuzmin cutoff due to the pion
production of extragalactic cosmic ray protons off the cosmic
microwave background. In addition to the relatively high flux of
events, the isotropic distribution of arrival directions and an
indication of hadronic primaries strongly challenge all models
proposed to resolve this puzzle. We discuss how the GZK cutoff is
modified by the local distribution of galaxies and how astrophysical
proton sources with soft injection spectra are ruled out by AGASA
data. Sources with hard injection spectrum are barely allowed by
these observations. We present an overview of the theoretical
proposals along with their most general signatures to be tested by
future experiments.
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