Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/604
Full metadata record
DC Field | Value | Language |
---|---|---|
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 |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
PANDEY.pdf | 534.08 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.