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Magnetization of all stationary cylindrically symmetric vacuum metrics

dc.contributor.authorIyer, B R
dc.contributor.authorVishveshwara, C V
dc.date.accessioned2006-05-16T11:20:30Z
dc.date.available2006-05-16T11:20:30Z
dc.date.issued1983-06
dc.description.abstractNew exact solutions of the Einstein–Maxwell equations are obtained by a Harrison-type transformation applied to the most general stationary cylindrically symmetric vacuum spacetime. These solutions include generalizations of the well-known Melvin Magnetic Universe, and the Weyl–Levi-Cività magnetic solution in addition to a new class of magnetic stationary axisymmetric spacetimes.en
dc.format.extent304101 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationJournal of Mathematical Physics, 1983, Vol.24, p1568-1573.en
dc.identifier.issn0022-2488
dc.identifier.urihttp://hdl.handle.net/2289/1270
dc.language.isoenen
dc.publisherThe American Institute of Physicsen
dc.relation.urihttp://link.aip.org/link/?jmp/24/1568en
dc.rights(1983) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics.en
dc.titleMagnetization of all stationary cylindrically symmetric vacuum metricsen
dc.typeArticleen

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