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dc.contributor.authorGeorgiou, A.
dc.date.accessioned2011-02-22T09:33:28Z
dc.date.available2011-02-22T09:33:28Z
dc.date.issued2003
dc.identifier.citationGeorgiou , A 2003 , ' A combined rotating charged dust-surface layer source for the McCrea electrovacuum ' , Il Nuovo Cimento B , vol. 118 , no. 4 , pp. 411-416 . https://doi.org/10.1393/ncb/i2003-10021-8
dc.identifier.issn1826-9877
dc.identifier.otherPURE: 169752
dc.identifier.otherPURE UUID: 6d16c187-55d7-4b5a-bd8e-23dab3cf085c
dc.identifier.otherdspace: 2299/5365
dc.identifier.otherScopus: 0242710757
dc.identifier.urihttp://hdl.handle.net/2299/5365
dc.descriptionThe original publication is available at http://www.sif.it/ Copyright Società Italiana di Fisica [Full text of this article is not available in the UHRA]
dc.description.abstractThe McCrea electrovacuum is one of the few known stationary cylindrically symmetric solutions of the Einstein-Maxwell field equations. In the purely gravitational case in which the electromagnetic field is absent, a source was obtained in the form of an infinitely long cylindrical shell. In this work, we obtain a source of the complete McCrea electrovacuum, which is also in the form of an infinitely long cylindrical shell, but in this case the shell is the boundary of rotating charged dust. The source of the complete McCrea electrovacuum found here therefore; is a combination of rotating charged dust, bounded by an infinitely long cylindrical shell which is rotating with the dust.en
dc.language.isoeng
dc.relation.ispartofIl Nuovo Cimento B
dc.subjectphysics
dc.titleA combined rotating charged dust-surface layer source for the McCrea electrovacuumen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1393/ncb/i2003-10021-8
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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