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arXiv · 1208.5284

A two-component model for the high-energy variability of blazars. Application to PKS 2155-304

Matías M. Reynoso·Gustavo E. Romero·María C. Medina
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Abstract

We study the production of VHE emission in blazars as a superposition of a steady component from a baryonic jet and a time- dependent contribution from an inner e-e+ beam launched by the black hole. Both primary relativistic electrons and protons are injected in the jet, and the particle distributions along it are found by solving a one-dimensional transport equation that accounts for convection and cooling. The short-timescale variability of the emission is explained by local pair injections in turbulent regions of the inner beam. For illustration, we apply the model to the case of PKS 2155-304, reproducing a quiescent state of emission with inverse Compton and synchrotron radiation from primary electrons, as well as proton-proton interactions in the jet. The latter also yield an accompanying neutrino flux that could be observed with a new generation km-scale detector in the northern hemisphere such as KM3NeT.

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Matías M. Reynoso, Gustavo E. Romero, María C. Medina. 2012-09-23. A two-component model for the high-energy variability of blazars. Application to PKS 2155-304. https://doi.org/10.1051/0004-6361%2F201219873

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