Expanding a Monte Carlo Radiation Transfer Scheme to include Anisotropic Magnetic Fields and Bulk Velocities, and Applications to AGN's

Statistics – Applications

Scientific paper

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Scientific paper

To extend its usefulness to applications for AGN's, astrophysical jets, and other myriad sources, our Monte Carlo radiation transport has been modified in several important ways. Previously, magnetic fields were considered as having no angle dependence or "structure". Changes have made it possible to consider fields which point in any direction in each simulation cell, which will be vital for properly modelling AGN's, whose fields are strongly anisotropic. Similarly, other modifications have added the capability of treating the simulation plasma as having macroscopic flow. That is, the emission, scattering, and transport of photons in the volume is now dependent on the bulk motion of the plasma. This will be especially important when simulating jets, where speeds may be a considerable fraction of the speed of light.

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