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류동수

Ryu, Dongsu
Astrophysics Lab.
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dc.citation.number 2 -
dc.citation.startPage 114 -
dc.citation.title ASTROPHYSICAL JOURNAL -
dc.citation.volume 892 -
dc.contributor.author Chen, L. E. -
dc.contributor.author Bott, A. F. A. -
dc.contributor.author Tzeferacos, P. -
dc.contributor.author Rigby, A. -
dc.contributor.author Bell, A. -
dc.contributor.author Bingham, R. -
dc.contributor.author Graziani, C. -
dc.contributor.author Katz, J. -
dc.contributor.author Koenig, M. -
dc.contributor.author Li, C. K. -
dc.contributor.author Petrasso, R. -
dc.contributor.author Park, H.-S. -
dc.contributor.author Ross, J. S. -
dc.contributor.author Ryu, Dongsu -
dc.contributor.author White, T. G. -
dc.contributor.author Reville, B. -
dc.contributor.author Matthews, J. -
dc.contributor.author Meinecke, J. -
dc.contributor.author Miniati, F. -
dc.contributor.author Zweibel, E. G. -
dc.contributor.author Sarkar, S. -
dc.contributor.author Schekochihin, A. A. -
dc.contributor.author Lamb, D. Q. -
dc.contributor.author Froula, D. H. -
dc.contributor.author Gregori, G. -
dc.date.accessioned 2023-12-21T17:42:58Z -
dc.date.available 2023-12-21T17:42:58Z -
dc.date.created 2020-04-13 -
dc.date.issued 2020-04 -
dc.description.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. -
dc.identifier.bibliographicCitation ASTROPHYSICAL JOURNAL, v.892, no.2, pp.114 -
dc.identifier.doi 10.3847/1538-4357/ab7a19 -
dc.identifier.issn 0004-637X -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/31911 -
dc.identifier.url https://iopscience.iop.org/article/10.3847/1538-4357/ab7a19 -
dc.identifier.wosid 000523478900001 -
dc.language 영어 -
dc.publisher IOP PUBLISHING LTD -
dc.title Transport of High-energy Charged Particles through Spatially Intermittent Turbulent Magnetic Fields -
dc.type Article -
dc.description.isOpenAccess FALSE -
dc.relation.journalWebOfScienceCategory Astronomy & Astrophysics -
dc.relation.journalResearchArea Astronomy & Astrophysics -
dc.type.docType Article -
dc.description.journalRegisteredClass scie -
dc.description.journalRegisteredClass scopus -
dc.subject.keywordAuthor High energy astrophysics -
dc.subject.keywordAuthor Ultra-high-energy cosmic radiation -
dc.subject.keywordAuthor Magnetic fields -
dc.subject.keywordAuthor Laboratory astrophysics -
dc.subject.keywordAuthor Plasma astrophysics -
dc.subject.keywordAuthor Intergalactic medium -
dc.subject.keywordAuthor Particle astrophysics -
dc.subject.keywordPlus COSMIC-RAY PROPAGATION -
dc.subject.keywordPlus SIMULATIONS -
dc.subject.keywordPlus ANISOTROPY -
dc.subject.keywordPlus FLASH -

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