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Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei

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Genesis and Propagation of Cosmic Rays

Part of the book series: NATO ASI Series ((ASIC,volume 220))

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Abstract

Super-high energy (~ 1020eV) cosmic rays could be accelerated in current-carrying beams associated with black-hole accretion discs in galactic nuclei. The current system might resemble an electrical circuit with a voltage source (black hole and accretion disc) coupled to a load (cosmic-ray beam) and a low impedance element (ambient conducting medium). Beam particles can be accelerated to 1020 provided that the beam channel medium behaves like an inductive circuit with high impedance. But even if these conditions are satisfied, a major difficulty the model faces is the large energy loss caused by photomeson reactions.

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© 1988 D. Reidel Publishing Company, Dordrecht, Holland

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Sorrell, W.H. (1988). Conditions for Acceleration of Super-High Energy Cosmic Rays in Active Galactic Nuclei. In: Shapiro, M.M., Wefel, J.P. (eds) Genesis and Propagation of Cosmic Rays. NATO ASI Series, vol 220. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4025-3_13

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  • DOI: https://doi.org/10.1007/978-94-009-4025-3_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8286-0

  • Online ISBN: 978-94-009-4025-3

  • eBook Packages: Springer Book Archive

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