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Transport of high-energy charged particles through spatially-intermittent turbulent magnetic fields

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arxiv 1808.04430 v3 pith:733WJ2HS submitted 2018-08-13 physics.plasm-ph astro-ph.GAastro-ph.HE

classification physics.plasm-phastro-ph.GAastro-ph.HE
keywords magnetictransportcosmicdiffusivefieldparticlesrayscharacterize
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Identifying the sources of the highest energy cosmic rays requires understanding how they are deflected by the stochastic, spatially intermittent intergalactic magnetic field. Here we report measurements of energetic charged-particle propagation through a laser-produced magnetized plasma with these properties. We characterize the diffusive transport of the particles experimentally. The results show that the transport is diffusive and that, for the regime of interest for the highest-energy cosmic rays, the diffusion coefficient is unaffected by the spatial intermittency of the magnetic field.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies

    astro-ph.GA 2026-08 conditional novelty 7.0 of 10

    Mass-dependent coupling of AGN winds and supernovae, including a metal-lifting fountain in dwarfs, explains the steep L_X-T relation of early-type galaxies.

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