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- W3101609523 endingPage "11" @default.
- W3101609523 startingPage "11" @default.
- W3101609523 abstract "We present a new code for radiation transport around Kerr black holes, including arbitrary emission and absorption mechanisms, as well as electron scattering and polarization. The code is particularly useful for analyzing accretion flows made up of optically thick disks and optically thin coronae. We give a detailed description of the methods employed in the code and also present results from a number of numerical tests to assess its accuracy and convergence." @default.
- W3101609523 created "2020-11-23" @default.
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- W3101609523 date "2013-10-08" @default.
- W3101609523 modified "2023-09-26" @default.
- W3101609523 title "A MONTE CARLO CODE FOR RELATIVISTIC RADIATION TRANSPORT AROUND KERR BLACK HOLES" @default.
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- W3101609523 doi "https://doi.org/10.1088/0004-637x/777/1/11" @default.
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