arXiv Analytics

Sign in

arXiv:1805.09953 [astro-ph.HE]AbstractReferencesReviewsResources

Blazar Spectra with Hard-sphere-like Acceleration of Electrons

Katsuaki Asano, Masaaki Hayashida

Published 2018-05-25Version 1

Electrons emitting non-thermal photons in blazars are possibly accelerated by turbulences developed in jets. In this paper, we consider the case so-called hard-sphere scattering as an interaction model between turbulences and electrons, in which the acceleration timescale is independent of the electron energy. We numerically simulate broad-band emission from blazar jets with a one-zone time-dependent code, taking into account the turbulence acceleration. Our model reproduces various blazar spectra with simple assumptions, such as constant particle injection rate, constant diffusion coefficient, and conical geometry of the jet. We also discuss possible mechanism to realize the hard-sphere-like acceleration in blazar jets.

Comments: 7 pages, 7 figures, accepted for ApJ
Categories: astro-ph.HE
Related articles: Most relevant | Search more
arXiv:1005.4999 [astro-ph.HE] (Published 2010-05-27)
Modelling the emission from blazar jets - the case of PKS 2155-304
arXiv:1404.4193 [astro-ph.HE] (Published 2014-04-16)
Polarimetric Tomography of Blazar Jets
arXiv:1410.8502 [astro-ph.HE] (Published 2014-10-30)
MOJAVE XII: Acceleration and Collimation of Blazar Jets on Parsec Scales
D. C. Homan et al.