Shock formation in electron–ion plasmas: mechanism and timing

dc.contributor.authorStockem, A.
dc.contributor.authorBret, A.
dc.contributor.authorFonseca, R. A.
dc.contributor.authorSilva, L. O.
dc.date.accessioned2015-05-08T14:13:45Z
dc.date.available2015-05-08T14:13:45Z
dc.date.issued2015
dc.date.updated2019-05-03T12:00:11Z
dc.description.abstractWe analyze the full shock formation process in electron-ion plasmas in theory and simulations. It is accepted that electromagnetic shocks in initially unmagnetized relativistic plasmas are triggered by filamentation instability. However, the transition from the first unstable phase to the quasi-steady shock is still missing. We derive a theoretical model for the shock formation time, taking into account filament merging in the nonlinear phase of the filamentation instability. This process is much slower than in electron-positron pair shocks, and so the shock formation is longer by a factor proportional to root m(i)/m(e) ln (m(i)/m(e)).eng
dc.description.versioninfo:eu-repo/semantics/publishedVersion
dc.distributionInternacionalpor
dc.identifier.doi10.1088/2041-8205/803/2/L29
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/10071/8898
dc.journalAstrophysical Journal Letters
dc.language.isoeng
dc.number2
dc.paginationL29por
dc.peerreviewedyes
dc.publicationstatusPublicadopor
dc.publisherIOP Publishing
dc.relationinfo:eu-repo/grantAgreement/EC/FP7/267841/EU
dc.rightsopen accesspor
dc.subjectInstabilitieseng
dc.subjectRelativistic processeseng
dc.subjectShock waveseng
dc.subject.fosDomínio/Área Científica::Ciências Naturais::Ciências Físicaspor
dc.titleShock formation in electron–ion plasmas: mechanism and timingeng
dc.typearticle
dc.volume803
degois.publication.firstPageL29por
degois.publication.issue2
degois.publication.titleShock formation in electron–ion plasmas: mechanism and timingeng
dspace.entity.typePublicationen
iscte.alternateIdentifiers.scopus2-s2.0-84938412657
iscte.alternateIdentifiers.wosWOS:000353818000015
iscte.identifier.cienciahttps://ciencia.iscte-iul.pt/id/ci-pub-23450

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