dc.contributor.author |
Pandey, U. S |
|
dc.contributor.author |
Dubey, G. S |
|
dc.date.accessioned |
2005-12-06T04:22:34Z |
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dc.date.available |
2005-12-06T04:22:34Z |
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dc.date.issued |
1983-12 |
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dc.identifier.citation |
BASI, Vol. 11, No. 4, pp. 303-312 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/604 |
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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 |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
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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 |