| 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 |