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류동수

Ryu, Dongsu
Astrophysics Lab.
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Transport of High-energy Charged Particles through Spatially Intermittent Turbulent Magnetic Fields

Author(s)
Chen, L. E.Bott, A. F. A.Tzeferacos, P.Rigby, A.Bell, A.Bingham, R.Graziani, C.Katz, J.Koenig, M.Li, C. K.Petrasso, R.Park, H.-S.Ross, J. S.Ryu, DongsuWhite, T. G.Reville, B.Matthews, J.Meinecke, J.Miniati, F.Zweibel, E. G.Sarkar, S.Schekochihin, A. A.Lamb, D. Q.Froula, D. H.Gregori, G.
Issued Date
2020-04
DOI
10.3847/1538-4357/ab7a19
URI
https://scholarworks.unist.ac.kr/handle/201301/31911
Fulltext
https://iopscience.iop.org/article/10.3847/1538-4357/ab7a19
Citation
ASTROPHYSICAL JOURNAL, v.892, no.2, pp.114
Abstract
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.
Publisher
IOP PUBLISHING LTD
ISSN
0004-637X
Keyword (Author)
High energy astrophysicsUltra-high-energy cosmic radiationMagnetic fieldsLaboratory astrophysicsPlasma astrophysicsIntergalactic mediumParticle astrophysics
Keyword
COSMIC-RAY PROPAGATIONSIMULATIONSANISOTROPYFLASH

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