Monte Carlo simulations of high energy radiation from compact objects

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Radiation Transport, Neutron Stars

Scientific paper

We discuss the space-and-time-dependent Monte Carlo code we have developed to simulate the relativistic radiation output from compact astrophysical objects with self-consistent hybrid lepton populations determined by a Fokker-Planck code. We highlight some sample recent results obtained with this code, which are relevant to the emission from a magnetized neutron star magnetospheric shell reprocessing the stellar radiation, or a magnetic disk corona reprocessing disk radiation.

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