On the simultaneous generation of high energy emission and submillimeter/infrared radiation from active galactic nuclei

Abstract

For active galactic nuclei (AGNs) we study the role of the mechanism of quasi-linear diffusion (QLD) in producing the high energy emission in the MeV-GeV domains strongly connected with the submillimeter/infrared radiation. Considering the kinetic equation governing the stationary regime of the QLD we investigate the feedback of the diffusion on electrons. We show that this process leads to the distribution of particles by the pitch angles, implying that the synchrotron mechanism is no longer prevented by energy losses. Examining a reasonable interval of physical parameters, we show that it is possible to produce MeV-GeV gamma-rays, strongly correlated with submillimeter/infrared bands.

arXiv comment7 pages, 3 figures

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• Very High Energy Gamma-Ray Astronomy
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Cited by in corpus (8)

• Non-thermal Processes in Black-Hole-Jet Magnetospheres
• VHE gamma-ray Emission from Passive Supermassive Black Holes: Constraints for NGC 1399
• The influence of corotation on the high energy synchrotron emission in Crab-like pulsars
• Synchrotron emission driven by the Cherenkov-drift instability in active galactic nuclei
• The generation of connected high and very high energy $\gamma$-rays and radio emission in active galactic nuclei
• Synchrotron emission from a nearby zone of SgrA${}^{\ast }$
• Radio emission of magnetars driven by the quasi-linear diffusion
• On the mechanism of the pulsed high energy emission from the pulsar PSR B1509-58