Dortmund 2006 – wissenschaftliches Programm
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T: Teilchenphysik
T 407: Kosmische Strahlung III
T 407.9: Vortrag
Mittwoch, 29. März 2006, 18:20–18:35, HG2-HS3
Photons at the end of the cosmic-ray spectrum? — •Markus Risse1,2, Piotr Homola2, Ralph Engel1, Dariusz Gora2,3, Dieter Heck1, Jan Pekala2, Barbara Wilczynska2, and Henryk Wilczynski2 — 1Forschungszentrum Karlsruhe, Institut für Kernphysik, 76021 Karlsruhe — 2Institute of Nuclear Physics PAN, 31-342 Krakow, Poland — 3Universität Karlsruhe, Institut für Experimentelle Kernphysik, 76021 Karlsruhe
Photons above 10 EeV might provide a key for understanding the origin of cosmic rays. Substantial fluxes of these ultrahigh-energy (UHE) photons are predicted in top-down models of cosmic-ray origin. UHE photons are also produced by the GZK process of resonant photoproduction of pions, in analogy to GZK neutrinos. Experimentally, UHE photons can be discriminated from nuclear primaries due to differences in the expected air shower signatures. So far, no photon detection has been claimed. In this work, recent results on upper limits to the fraction of photons are presented. The statistics collected so far already allows us to constrain some top-down models. With increasing data statistics from the Pierre Auger Observatory, further constraints are expected.