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dc.contributor.authorGeorgiou, A.
dc.date.accessioned2011-02-21T17:36:55Z
dc.date.available2011-02-21T17:36:55Z
dc.date.issued2005
dc.identifier.citationGeorgiou , A 2005 , ' Perfectly conducting rapidly rotating sphere and pulsar electrodynamics ' , Il Nuovo Cimento B , vol. 120 , no. 5 , pp. 541-550 . https://doi.org/10.1393/ncb/i2005-10080-9
dc.identifier.issn1826-9877
dc.identifier.otherPURE: 181908
dc.identifier.otherPURE UUID: 8e049646-56ce-4f69-8eb3-6a3b44fe7204
dc.identifier.otherdspace: 2299/5360
dc.identifier.otherScopus: 28744446721
dc.identifier.urihttp://hdl.handle.net/2299/5360
dc.descriptionThe original publication is available at : http://www.sif.it/ Copyright Società italiana di fisica [Full text of this article is not available on the UHRA]
dc.description.abstractWe consider a perfectly conducting fluid with spherical boundary, rotating with constant angular velocity in an electromagnetic field. We then obtain, in the framework of special relativity, the exact forms of the equations of the interior and exterior electrodynamics for the case where the rotation axis is not aligned along the magnetic dipole field. Connections between this work and the electrodynamics of rotating magnetized neutron stars will be noted.en
dc.language.isoeng
dc.relation.ispartofIl Nuovo Cimento B
dc.subjectAstronomy
dc.titlePerfectly conducting rapidly rotating sphere and pulsar electrodynamicsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1393/ncb/i2005-10080-9
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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