Double Compton and Cyclo-Synchrotron in Super-Eddington Discs, Magnetized Coronae, and Jets
Abstract
Black hole accretion discs accreting near the Eddington rate are dominated by bremsstrahlung cooling, but above the Eddington rate, the double Compton process can dominate in radiation-dominated regions, while the cyclo-synchrotron can dominate in strongly magnetized regions like a corona or a jet. We present an extension to the general relativistic radiation magnetohydrodynamic code harmrad to account for emission and absorption by thermal...
Paper Details
Title
Double Compton and Cyclo-Synchrotron in Super-Eddington Discs, Magnetized Coronae, and Jets
Published Date
Jan 30, 2017
Pages
stx227 - stx227
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