Acceleration of UHE Cosmic Ray Particles at Relativistic Jets in Extragalactic Radio Sources

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dc.creatorOstrowski, M.
dc.date1996-10-23
dc.date.accessioned2026-07-07T02:22:08Z
dc.date.available2026-07-07T02:22:08Z
dc.descriptionA mechanism of ultra-high energy (UHE) cosmic ray acceleration in extragalactic radio sources at the interface between the relativistic jet and the ambient medium is discussed as a supplement to the shock acceleration in `hot spots'. Particles accelerated at the jet side boundary are expected to dominate at highest energies. The spectrum formation near the cut-off energy is modeled using the Monte Carlo particle simulations.
dc.descriptionTeX, 5 pages + 4 postscript figures; to be published in Proc. ICRR Symposium on Extremely High Energy Cosmic Rays, ed. M. Nagano, Tanashi
dc.identifierhttps://arxiv.org/abs/astro-ph/9610190
dc.identifierhttp://arxiv.org/abs/astro-ph/9610190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10766
dc.subjectAstrophysics
dc.titleAcceleration of UHE Cosmic Ray Particles at Relativistic Jets in Extragalactic Radio Sources
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