A fluid model for colloidal plasmas under microgravity conditions

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dc.bibliographicCitation.articleNumber32
dc.bibliographicCitation.firstPage32
dc.bibliographicCitation.journalTitleNew Journal of Physics
dc.bibliographicCitation.volume5
dc.contributor.authorGozadinos, G.
dc.contributor.authorIvlev, A. V.
dc.contributor.authorBoeuf, J. P.
dc.date.accessioned2025-03-03T12:23:11Z
dc.date.available2025-03-03T12:23:11Z
dc.date.issued2003
dc.description.abstractA numerical model is presented to simulate steady states of complex ('dusty') plasmas under microgravity conditions. The model uses a fluid description for the plasma as well as for the dust microparticles. This is achieved by using an appropriate equation of state for the crystalline phase of the dust. The only forces assumed to act on the dust particles are the electric force, ion drag and pressure gradients. The model is used to study the formation of the stable 'void' present in recent microgravity experiments. The structure of the dust clouds when the void is present is examined and explained.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/18733
dc.identifier.urihttps://doi.org/10.34657/17752
dc.language.isoeng
dc.publisher[London] : IOP
dc.relation.doihttps://doi.org/10.1088/1367-2630/5/1/332
dc.relation.essn1367-2630
dc.rights.licenseCC BY-NC-SA 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/3.0/
dc.subject.ddc530
dc.subject.otherplasmaeng
dc.subject.othermicrogravityeng
dc.subject.othermicroparticleeng
dc.titleA fluid model for colloidal plasmas under microgravity conditionseng
dc.typeArticle
dc.typeText
tib.accessRightsopenAccess
wgl.contributorINP
wgl.subjectPhysikger
wgl.typeZeitschriftenartikelger
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