Synchrotron self-Compton flaring of TeV blazars II. Linear and nonlinear electron cooling

摘要: A theoretical radiation model for the flaring of TeV blazars is discussed here case a nonlinear electron synchrotron cooling in these sources. We compute analytically optically thick and thin intensities photon density distributions emission knot as functions frequency time followed by self-Compton intensity fluence range using Thomson approximation inverse Compton cross section. At all times frequencies, part process shown to provide dominant contribution quantities, while always negligible. Afterwards, we compare linear data record PKS 2155-304 on MJD 53944 favouring injected monoenergetic electrons. The good agreement both with supports relativistic pickup operating this source. Additionally, discuss scattering, applying full Klein-Nishina section achieve most accurate results distributions.