Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/604
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dc.contributor.authorPandey, U. S-
dc.contributor.authorDubey, G. S-
dc.date.accessioned2005-12-06T04:22:34Z-
dc.date.available2005-12-06T04:22:34Z-
dc.date.issued1983-12-
dc.identifier.citationBASI, Vol. 11, No. 4, pp. 303-312en
dc.identifier.urihttp://hdl.handle.net/2248/604-
dc.description.abstractWe derive for test electromagnetic field of a non-axisymmetric current loop around a Kerr blackhole. For this, we write complete solution for the `inside` as well as 'out side' regions of the current loop using vacuum solutions of King (1977). We calculate discontinuities in two ways. First, we integrate radially the inhomogeneous Maxwell equations across a thin shell at r/subo/ the loop radius, written in Newmann-Penrose (NP) formalism. Second, the discontinuity in the electromagnetic field components is obtained from the complete solution in which the 'inside' solution is characterized by a complex constant Alpha im and the outside solution by beta im. Now we equate the two discontinuities and the determine the complete solution. A particular solution, namely, electromagnetic field of an equatorial current loop is obtained.en
dc.format.extent546901 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectGeneral relativityen
dc.subjectBlackholeen
dc.subjectElectromagnetic fieldsen
dc.titleElectromagnetic field due to a non-axisymmetric current loop around Kerr blackholeen
dc.typeArticleen
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