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Context. Modelling the emission properties of compact high energy sources such as X-ray binaries, AGN or γ-ray bursts represents a complex problem. Contributions of numerous processes participate non linearly to produce the observed spectra: particle-particle, particle-photon and particle-wave interactions. Numerical simulations have been widely used to address the key properties of the high energy plasmas present in these sources.
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A 2008 study studied this question.
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