Magnetization of all stationary cylindrically symmetric vacuum metrics

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1270

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DC Field	Value	Language
dc.contributor.author	Iyer, B.R.	-
dc.contributor.author	Vishveshwara, C.V.	-
dc.date.accessioned	2006-05-16T11:20:30Z	-
dc.date.available	2006-05-16T11:20:30Z	-
dc.date.issued	1983-06	-
dc.identifier.citation	Journal of Mathematical Physics, 1983, Vol.24, p1568-1573.	en
dc.identifier.issn	0022-2488	-
dc.identifier.uri	http://hdl.handle.net/2289/1270	-
dc.description.abstract	New 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.extent	304101 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The American Institute of Physics	en
dc.relation.uri	http://link.aip.org/link/?jmp/24/1568	en
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.title	Magnetization of all stationary cylindrically symmetric vacuum metrics	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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