Radiation from Kinetic Poynting Flux Acceleration

dc.creatorLiang, Edison
dc.creatorNoguchi, Koichi
dc.date2007-04-13
dc.date2007-11-18
dc.date.accessioned2026-07-07T08:43:13Z
dc.date.available2026-07-07T08:43:13Z
dc.descriptionWe derive analytic formulas for the power output and critical frequency of radiation by electrons accelerated by relativistic kinetic Poynting flux, and validate these results with Particle-In-Cell plasma simulations. We find that the in-situ radiation power output and critical frequency are much below those predicted by the classical synchrotron formulae. We discuss potential astrophysical applications of these results.
dc.description25 pages, 11 figures, revised paper resubmitted to Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/0704.1843
dc.identifierhttp://arxiv.org/abs/0704.1843
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142238
dc.subjectAstrophysics
dc.titleRadiation from Kinetic Poynting Flux Acceleration
dc.typetext

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