{ "id": "0911.4004", "version": "v1", "published": "2009-11-20T10:44:33.000Z", "updated": "2009-11-20T10:44:33.000Z", "title": "Cosmic Ray Acceleration in Active Galactic Nuclei - On Centaurus A as a possible UHECR Source", "authors": [ "Frank M. Rieger" ], "comment": "8 pages, one figure; based on invited talk at the JEM-EUSO Workshop, Torino/Italy, December 2008. To appear in Proceedings of the JEM-EUSO Workshop, under publication by UAP Tokyo, Japan", "categories": [ "astro-ph.HE" ], "abstract": "We discuss a representative selection of particle acceleration mechanisms believed to be operating in Active Galactic Nuclei. Starting from direct electrostatic field acceleration in the vicinity of the black hole up to Fermi-type particle acceleration in the jet and beyond, possible efficiency constraints on the energization of ultra-high energy cosmic rays (UHECR) are evaluated. When paradigmatically applied to Cen A, the following results are obtained: (i) Proton acceleration to energies of $E_c = 5\\times 10^{19}$ eV and beyond remains challenging and most likely requires the operation of an additional mechanism capable of boosting energetic seed protons up by a factor of $\\sim$ten. It is argued that shear acceleration along the large-scale jet in Cen A could be a promising candidate for this. (ii) Heavier elements, like iron nuclei, are more easily accelerated (by, e.g., shocks or direct electrostatic fields) and may not need additional boosting to reach $E \\geq E_c$; (iii) If Cen A indeed proves to be an UHECR source, the cosmic ray composition might thus be expected to become heavier above energies of a few times $10^{19}$ eV.", "revisions": [ { "version": "v1", "updated": "2009-11-20T10:44:33.000Z" } ], "analyses": { "keywords": [ "active galactic nuclei", "cosmic ray acceleration", "uhecr source", "direct electrostatic field acceleration", "ultra-high energy cosmic rays" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable", "inspire": 837441, "adsabs": "2009arXiv0911.4004R" } } }