Acceleration of ULtra High Energy Cosmic Rays: Cosmic Zevatrons?

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dc.creatorJones, T. W.
dc.date2002-10-21
dc.date.accessioned2026-07-07T02:05:47Z
dc.date.available2026-07-07T02:05:47Z
dc.descriptionIn this lecture I outline some of the underlying physics issues associated with accelerators plausibly capable of explaining the UHECRs up to ZeV energies. I concentrate on the concentrate on mechanisms and their constraints, but provide a brief background on on observations and the constraints they supply, as well.
dc.description20 pages, including 3 figures. To be published in proceedings of the 9th Chalonge School on Astrofundamental Physics, Palermo, Sicily, September 7-18, 2002. Ed: N. Sanchez, Kluwer Academic Publishers
dc.identifierhttps://arxiv.org/abs/astro-ph/0210477
dc.identifierhttp://arxiv.org/abs/astro-ph/0210477
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5209
dc.subjectAstrophysics
dc.titleAcceleration of ULtra High Energy Cosmic Rays: Cosmic Zevatrons?
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