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Filamentary Jets as a Cosmic-Ray "Zevatron"

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Published 2004 November 3 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Mitsuru Honda and Yasuko S. Honda 2004 ApJ 617 L37 DOI 10.1086/427067

1538-4357/617/1/L37

Abstract

Strong, anisotropic turbulence reflecting magnetized filaments is considered, to model the diffusive acceleration of particles by shock waves in active galactic nucleus jets. We address that at knot A of the nearby M87 jet, the shock involving the filamentary turbulence can accelerate an iron nucleus to zetta-eV (ZeV; 1021 eV) ranges. A smaller value of the particle diffusion coefficient is found to be essential to achieve a ZeV cosmic-ray accelerator, a "Zevatron."

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10.1086/427067