Cylindrical Domain Walls and Gravitational Waves -- Einstein Rosen wave emission from momentarily static initial configuration --
Abstract
Description
A self-gravitating cylindrical domain wall is considered as an example of non-spherical wall to clarify the interaction between a domain wall and gravitational waves. We consider the time evolution from a momentarily static initial configuration within an infinitesimal time interval using the metric junction formalism. We found that the wall with a large initial radius radiates large amplitude of the gravitational waves and undergoes its large back reaction.
3 pages, latex requires mprocl.sty, no figures. To appear in the proceedings of the Eighth Marcel Grossmann Conference on General Relativity (Jerusalem, Israel, June 1997)
3 pages, latex requires mprocl.sty, no figures. To appear in the proceedings of the Eighth Marcel Grossmann Conference on General Relativity (Jerusalem, Israel, June 1997)