Astroparticle yield and transport in extragalactic jets: Multi-scale simulations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

In this work we present a new numerical method to handle relativistic particle transport in complex flows. The code couples 3D fluid magneto-hydrodamics to stochastic differential equations. We apply it to the transport effects on cosmic-rays in extragalactic jets and particularly to the hot spots of FRII radio galaxies. From the observations, we selected the best candidates for the production of ultra high energy cosmic-rays and neutrinos. and evaluate the contribution of the strongest astroparticle sources to the different extragalactic diffuse backgrounds.

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