Enabling Lorentz boosted frame particle-in-cell simulations of laser wakefield acceleration in quasi-3D geometry

dc.contributor.authorYu, P.
dc.contributor.authorXu, X.
dc.contributor.authorDavidson, A.
dc.contributor.authorTableman, A.
dc.contributor.authorDalichaouch, T.
dc.contributor.authorLi, F.
dc.contributor.authorMeyers, M. D.
dc.contributor.authorAn, W.
dc.contributor.authorTsung, F. S.
dc.contributor.authorDecyk, V. K.
dc.contributor.authorFiuza, F.
dc.contributor.authorVieira, J.
dc.contributor.authorFonseca, R. A.
dc.contributor.authorLu, W.
dc.contributor.authorSilva, L. O.
dc.contributor.authorMori, W. B.
dc.date.accessioned2017-04-21T12:57:50Z
dc.date.available2017-04-21T12:57:50Z
dc.date.issued2016
dc.date.updated2019-04-24T10:15:38Z
dc.description.abstractWhen modeling laser wakefield acceleration (LWFA) using the particle-in-cell (PIC) algorithm in a Lorentz boosted frame, the plasma is drifting relativistically at beta(b)c towards the laser, which can lead to a computational speedup of similar to gamma(2)(b)=(1-beta(2)(b))-1. Meanwhile, when LWFA is modeled in the quasi-3D geometry in which the electromagnetic fields and current are decomposed into a limited number of azimuthal harmonics, speedups are achieved by modeling three dimensional (3D) problems with the computational loads on the order of two dimensional r-z simulations. Here, we describe a method to combine the speedups from the Lorentz boosted frame and quasi-3D algorithms. The key to the combination is the use of a hybrid Yee-FFT solver in the quasi-3D geometry that significantly mitigates the Numerical Cerenkov Instability (NCI) which inevitably arises in a Lorentz boosted frame due to the unphysical coupling of Langmuir modes and EM modes of the relativistically drifting plasma in these simulations. In addition, based on the space-time distribution of the LWFA data in the lab and boosted frame, we propose to use a moving window to follow the drifting plasma, instead of following the laser driver as is done in the LWFA lab frame simulations, in order to further reduce the computational loads. We describe the details of how the NCI is mitigated for the quasi-3D geometry, the setups for simulations which combine the Lorentz boosted frame, quasi-3D geometry, and the use of a moving window, and compare the results from these simulations against their corresponding lab frame cases. Good agreement is obtained among these sample simulations, particularly when there is no self-trapping, which demonstrates it is possible to combine the Lorentz boosted frame and the quasi-3D algorithms when modeling LWFA. We also discuss the preliminary speedups achieved in these sample simulations.eng
dc.description.versioninfo:eu-repo/semantics/submittedVersion
dc.distributionInternacionalpor
dc.identifier.doi10.1016/j.jcp.2016.04.014
dc.identifier.issn0021-9991
dc.identifier.urihttp://hdl.handle.net/10071/13095
dc.journalJournal of Computational Physics
dc.language.isoeng
dc.pagination747 - 759
dc.peerreviewedyes
dc.publicationstatusPublicadopor
dc.publisherAcademic Press/Elsevier
dc.relationinfo:eu-repo/grantAgreement/EC/FP7/267841/EU
dc.rightsopen accesspor
dc.subjectPIC simulationeng
dc.subjectHybrid Maxwell solvereng
dc.subjectRelativistic plasma drifteng
dc.subjectNumerical Cerenkov Instabilityeng
dc.subjectQuasi-3D algorithmeng
dc.subjectLorentz boosted frameeng
dc.subjectMoving windoweng
dc.subject.fosDomínio/Área Científica::Ciências Naturais::Matemáticaspor
dc.subject.fosDomínio/Área Científica::Ciências Naturais::Ciências da Computação e da Informaçãopor
dc.titleEnabling Lorentz boosted frame particle-in-cell simulations of laser wakefield acceleration in quasi-3D geometryeng
dc.typearticle
dc.volume316
degois.publication.firstPage747
degois.publication.lastPage759
degois.publication.titleEnabling Lorentz boosted frame particle-in-cell simulations of laser wakefield acceleration in quasi-3D geometryeng
dspace.entity.typePublicationen
iscte.alternateIdentifiers.scopus2-s2.0-84964461818
iscte.alternateIdentifiers.wosWOS:000375799200039
iscte.identifier.cienciahttps://ciencia.iscte-iul.pt/id/ci-pub-30290

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