Extragalactic Sources for Ultra High Energy Cosmic Ray Nuclei

Abstract

In this article we examine the hypothesis that the highest energy cosmic rays are complex nuclei from extragalactic sources. Under reasonable physical assumptions, we show that the nearby metally rich starburst galaxies (M82 and NGC 253) can produce all the events observed above the ankle. This requires diffusion of particles below $10^{20}$ eV in extragalactic magnetic fields $B\approx 15$ nG. Above $10^{19}$ eV, the model predicts the presence of significant fluxes of medium mass and heavy nuclei with small rate of change of composition. Notwithstanding, the most salient feature of the starburst-hypothesis is a slight anisotropy induced by iron debris just before the spectrum-cutoff.

To appear in Phys. Rev. D, reference added

References in corpus (1)

• An Auger test of the Cen A model of highest energy cosmic rays

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• Ultrahigh energy cosmic rays from nearby starburst galaxies
• Ultra-High Energy Cosmic Ray Nuclei from Individual Magnetized Sources