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.

7 pages, 3 figures

References in corpus (4)

• VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope
• Variable VHE gamma-ray emission from non-blazar AGNs
• On the efficiency of particle acceleration by rotating magnetospheres in AGN
• The Synchrotron Emission Mechanism in the Recently Detected Very High Energy Radiation from the Crab Pulsar

Cited by in corpus (3)

• On the mechanism of the pulsed high energy emission from the pulsar PSR B1509-58
• Radio emission of magnetars driven by the quasi-linear diffusion
• Synchrotron emission from a nearby zone of SgrA${}^{\ast }$