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- W1637883911 abstract "We present simulations of the transport of fast particles through threedimensional turbulent magnetic field configurations. A time dependency is imposed on the plane wave modes used in constructing these fields such than acceleration via the second-order Fermi process is possible. We consider simulations of models with low and high turbulence levels for non-relativistic waves. The predictions of quasi-linear theory are discussed with respect to the simulation data. We conclude that for pure stochastic acceleration via Alfven waves to be plausible as the generator of UHECR in Cen A, the baryon number density would need to be several orders of magnitude below currently held upper-limits." @default.
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- W1637883911 date "2010-09-01" @default.
- W1637883911 modified "2023-09-26" @default.
- W1637883911 title "Relativistic Particle Acceleration in Tangled Magnetic Fields" @default.
- W1637883911 cites W3045599828 @default.
- W1637883911 doi "https://doi.org/10.21427/5j84-5563" @default.
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