Ultra High Energy Cosmic ray and gamma-ray signatures of inductive acceleration in AGN jets

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dc.creatorOuyed, Rachid
dc.creatorSigl, Guenter
dc.creatorLyutikov, Maxim
dc.date2007-06-19
dc.date.accessioned2026-07-07T08:11:05Z
dc.date.available2026-07-07T08:11:05Z
dc.descriptionThe highest energy cosmic rays could be produced by drifts in magnetized, cylindrically collimated, sheared jets of powerful active galaxies (i.e. FR II radiogalaxies; radio loud quasars and high power BL Lacs). We show that in such scenarios proton synchrotron radiation can give rise to detectable photon fluxes at energies ranging from hundreds of keV to tens of MeV.
dc.description3 journal pages (submitted to ApJ Letters)
dc.identifierhttps://arxiv.org/abs/0706.2812
dc.identifierhttp://arxiv.org/abs/0706.2812
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132014
dc.subjectAstrophysics
dc.titleUltra High Energy Cosmic ray and gamma-ray signatures of inductive acceleration in AGN jets
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