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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/18150
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dc.contributor.authorProtheroe, R.-
dc.contributor.authorMeli, A.-
dc.contributor.authorDonea, A.-
dc.date.issued2003-
dc.identifier.citationSpace Science Reviews, 2003; 107(1-2):369-372-
dc.identifier.issn0038-6308-
dc.identifier.issn1572-9672-
dc.identifier.urihttp://hdl.handle.net/2440/18150-
dc.descriptionCopyright © 2003. Space Science Reviews. All rights reserved. Printed in U.S.A. Submitted to Cornell University’s online archive www.arXiv.org in 2003 by Ray Protheroe. Post-print sourced from www.arxiv.org.-
dc.description.abstractWe investigate ways of accurately simulating the propagation of energetic charged particles over small times where the standard Monte Carlo approximation to diffusive transport breaks down. We find that a small-angle scattering procedure with appropriately chosen step-lengths and scattering angles gives accurate results, and we apply this to the simulation of propagation upstream in relativistic shock acceleration.-
dc.description.statementofresponsibilityR.J. Protheroe, A. Meli and A.-C. Donea-
dc.language.isoen-
dc.publisherKluwer Academic Publ-
dc.source.urihttp://dx.doi.org/10.1023/a:1025541704838-
dc.subjectcosmic rays-
dc.subjectdiffusion theory-
dc.subjectrelativistic shock acceleration-
dc.titleSmall-angle scattering and diffusion: Application to relativistic shock acceleration-
dc.typeJournal article-
dc.identifier.doi10.1023/A:1025541704838-
pubs.publication-statusPublished-
Appears in Collections:Aurora harvest 2
Physics publications

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