Utilize este identificador para referenciar este registo: http://hdl.handle.net/10071/21398
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Campo DCValorIdioma
dc.contributor.authorDel Gaudio, F.-
dc.contributor.authorFonseca, R. A.-
dc.contributor.authorSilva, L. O.-
dc.contributor.authorGrismayer, T.-
dc.date.accessioned2021-01-20T14:37:35Z-
dc.date.available2021-01-20T14:37:35Z-
dc.date.issued2020-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10071/21398-
dc.description.abstractPhoton bursts with a wavelength smaller than the plasma interparticle distance can drive plasma wakes via Compton scattering. We investigate this fundamental process analytically and numerically for different photon frequencies, photon flux, and plasma magnetization. Our results show that Langmuir and extraordinary modes are driven efficiently when the photon energy density lies above a certain threshold. The interaction of photon bursts with magnetized plasmas is of distinguished interest as the generated extraordinary modes can convert into pure electromagnetic waves at the plasma-vacuum boundary. This could possibly be a mechanism for the generation of radio waves in astrophysical scenarios in the presence of intense sources of high energy photons.eng
dc.language.isoeng-
dc.publisherAmerican Physical Society-
dc.relation695088-
dc.relationPD/00505/2012-
dc.relationPD/BD/114323/2016-
dc.rightsopenAccess-
dc.titlePlasma wakes driven by photon bursts via compton scatteringeng
dc.typearticle-
dc.peerreviewedyes-
dc.journalPhysical Review Letters-
dc.volume125-
dc.number26-
degois.publication.issue26-
degois.publication.titlePlasma wakes driven by photon bursts via compton scatteringeng
dc.date.updated2021-01-20T14:35:37Z-
dc.description.versioninfo:eu-repo/semantics/publishedVersion-
dc.identifier.doi10.1103/PhysRevLett.125.265001-
dc.subject.fosDomínio/Área Científica::Ciências Naturais::Ciências Físicaspor
iscte.identifier.cienciahttps://ciencia.iscte-iul.pt/id/ci-pub-77961-
iscte.alternateIdentifiers.wosWOS:000602858400008-
iscte.alternateIdentifiers.scopus2-s2.0-85095130731-
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