Abstract
We present a self-consistent and time-dependent model in order to explain the variability behaviors of extreme or TeV-blazars. This model is based on the ‘Two-Flow model’ involving a relativistic pair plasma beam surrounded by a classical MHD structure. Particular symbiosis between the ultra-relativistic pairs and the turbulence generated by the MHD jet may lead to a preys–predators comportment. We also consider that the pair energy distribution is not a power-law but a ‘pile-up’ one.
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