A time dependent model of thermal pair plasmas

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

We developed a nonlinear Monte Carlo code based on the Large Particles method. We use it to simulate the temporal behaviour of relativistic thermal pair plasmas likely to be responsible for the hard X-ray emission from Seyfert Galaxies and Galactic Black hole candidates. We investigate the plasma response to changes in the injection compactness parameters.

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