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Electromagnetic field due to a non-axisymmetric current loop around Kerr blackhole

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dc.contributor.author Pandey, U. S
dc.contributor.author Dubey, G. S
dc.date.accessioned 2005-12-06T04:22:34Z
dc.date.available 2005-12-06T04:22:34Z
dc.date.issued 1983-12
dc.identifier.citation BASI, Vol. 11, No. 4, pp. 303-312 en
dc.identifier.uri http://hdl.handle.net/2248/604
dc.description.abstract We 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.extent 546901 bytes
dc.format.mimetype application/pdf
dc.language.iso en
dc.publisher Astronomical Society of India en
dc.subject General relativity en
dc.subject Blackhole en
dc.subject Electromagnetic fields en
dc.title Electromagnetic field due to a non-axisymmetric current loop around Kerr blackhole en
dc.type Article en


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