| dc.contributor.author |
Mofiz, U.A. |
|
| dc.date.accessioned |
2010-10-14T14:15:53Z |
|
| dc.date.available |
2010-10-14T14:15:53Z |
|
| dc.date.issued |
2005 |
|
| dc.identifier.uri |
http://hdl.handle.net/10361/531 |
|
| dc.description.abstract |
An overview of gravitational wave and its possible detection while propagating in a plasma is given. The linear propagation of gravitational wave in magnetized plasma is considered. It is found that a × polarized gravitational wave excites Alfve′n modes while a + polarized wave excites
magneto-acoustic waves propagating parallel to the gravitational wave. In merging binary pulsars gravitational wave energy can be converted into pulsar wind at a large scale. |
en_US |
| dc.language.iso |
en |
en_US |
| dc.publisher |
BRAC University |
en_US |
| dc.relation.ispartofseries |
BRAC University Journal, BRAC University;Vol.2, No.1,pp. 83-88 |
|
| dc.subject |
Gravitional wave |
en_US |
| dc.subject |
General theory of relatively |
en_US |
| dc.subject |
Binary pulsars |
en_US |
| dc.subject |
Plasmas |
en_US |
| dc.title |
Gravitational waves in a magnetized plasma |
en_US |
| dc.type |
Article |
en_US |