Electron-positron processes and spectral evolution in black hole accretion disk dynamo models for AGN sources of the cosmic X-ray and gamma ray backgrounds

Details Electron-positron processes and spectral evolution in black hole accretion disk dynamo models for AGN sources of the cosmic X-ray and gamma ray backgrounds Electron-positron processes and spectral evolution in black hole accretion disk dynamo models for AGN sources of the cosmic X-ray and gamma ray backgrounds

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101..337l&link_type=abstract

IN: Positron-electron pairs in astrophysics; Proceedings of the Workshop, Greenbelt, MD, January 6-8, 1983 (A85-31276 13-90). Ne

Astronomy and Astrophysics

Astronomy

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Dynamo Theory, Gamma Ray Astronomy, Background Radiation, Bremsstrahlung, Compton Effect, Cyclotron Radiation, Electron Plasma, Pair Production, Plasma Jets, Positrons, Spectrum Analysis, Stellar Luminosity, Thermal Emission, X Ray Sources

Scientific paper

This work discusses a black hole accretion disk dynamo model for active
galactic nuclei sources of the cosmic X-ray and gamma-ray backgrounds
which involves both thermal and nonthermal accretion disk processes
around ≥108M_sun; Kerr black holes.

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