Multi-dimensional Monte Carlo Simulation of High Energy Emissions from Galactic Black Holes

Details Multi-dimensional Monte Carlo Simulation of High Energy Emissions from Galactic Black Holes Multi-dimensional Monte Carlo Simulation of High Energy Emissions from Galactic Black Holes

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprn17082l&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present 2-dimensional Monte Carlo simulations of x-and-gamma-ray output from accreting black holes. The 2-d code allows us to model the energy-time-and-angle-dependent radiation from accretion models, including disk corona, hot inner disk and ADAF-like scenarios. Of particular interest are the energy-dependent time-variability and phase dependence of QPOs. We will also discuss the effects of coupled thermal-nonthermal electron populations.

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