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 |