Particle diffusion and localized acceleration in inhomogeneous AGN jets – II. Stochastic variation

• Published in: Monthly notices of the Royal Astronomical Society 2016-05, Vol.458 (3), p.3260-3271
• Main Authors: Chen, Xuhui, Pohl, Martin, Böttcher, Markus, Gao, Shan
• Format: Article
• Language: English
• Subjects: Acceleration; Astrophysics; Correlation analysis; Flares; Flux; Mathematical models; Optics; Particle acceleration; Spectra; Spectrum analysis; Stochastic models; Stochasticity; X-ray astronomy; X-rays
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stw528

We study the stochastic variation of blazar emission under a 2D spatially resolved leptonic jet model we previously developed. Random events of particle acceleration and injection in small zones within the emission region are assumed to be responsible for flux variations. In addition to producing spectral energy distributions that describe the observed flux of Mrk 421, we further analyse the timing properties of the simulated light curves, such as the power spectral density (PSD) at different bands, flux–flux correlations, as well as the cross-correlation function between X-rays and TeV γ-rays. We find spectral breaks in the PSD at a time-scale comparable to the dominant characteristic time-scale in the system, which is usually the pre-defined decay time-scale of an acceleration event. Cooling imposes a delay, and so PSDs taken at lower energy bands in each emission component (synchrotron or inverse Compton) generally break at longer time-scales. The flux–flux correlation between X-rays and TeV γ-rays can be either quadratic or linear, depending on whether or not there are large variation of the injection into the particle acceleration process. When the relationship is quadratic, the TeV flares lag the X-ray flares, and the optical and GeV flares are large enough to be comparable to the ones in X-ray. When the relationship is linear, the lags are insignificant, and the optical and GeV flares are small.