On particle acceleration in turbulent shear boundary layers of relativistic jets

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dc.creatorOstrowski, M.
dc.creatorStawarz, L.
dc.date2002-07-08
dc.date.accessioned2026-07-07T02:04:12Z
dc.date.available2026-07-07T02:04:12Z
dc.descriptionWe discuss processes accelerating cosmic ray electrons at boundaries of relativistic jets. The resulting spectrum is expected to posses two characteristic components: a power-law distribution at lower energies and a harder high energy component preceding the high energy cut-off. An example of high energy spectrum from such electron distribution is presented, including the synchrotron and the inverse-Compton components. A characteristic feature of the synchrotron spectrum of such electrons is its highest frequency part which occurs above the power-law fitted to the low frequency spectral range.
dc.description4 pages, 1 figure included. Proceedings of the Workshop `Blazar Astrophysics with BeppoSAX and other Observatories', Frascati, Dec. 2001
dc.identifierhttps://arxiv.org/abs/astro-ph/0207159
dc.identifierhttp://arxiv.org/abs/astro-ph/0207159
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4661
dc.subjectAstrophysics
dc.titleOn particle acceleration in turbulent shear boundary layers of relativistic jets
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