Assuming that particles can be accelerated to high energies via diffusive shock acceleration process at the accretion shocks formed by the infalling flow toward the clusters of galaxies, we have calculated the expected spectrum of high-energy protons from the cosmological ensemble of the cluster accretion shocks. The model with Jokipii diffusion limit could explain the observed cosmic ray spectrum near 10 19eV with reasonable parameters and models if about 10-4 of the infalling kinetic energy can be injected into the intergalactic space as the high energy particles.

• HYESUNG KANG(Pusan National University)
• JORG P. RACHEN(Max-Planck-Institute for Radioastronomy)
• PETER L. BIERMANN(Max-Planck-Institute for Radioastronomy)