grmonty: a Monte Carlo Code for Relativistic Radiative Transport

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, no. 2 (2009): 387.0-397.0

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We describe a Monte Carlo radiative transport code intended for calculating spectra of hot, optically thin plasmas in full general relativity. The version we describe here is designed to model hot accretion flows in the Kerr metric and therefore incorporates synchrotron emission and absorption, and Compton scattering. The code can be read...更多

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