Cylindrical Domain Walls and Gravitational Waves -- Einstein Rosen wave emission from momentarily static initial configuration --

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dc.creatorNakamura, K.
dc.creatorIshihara, H.
dc.date1997-10-15
dc.date.accessioned2026-07-07T03:31:53Z
dc.date.available2026-07-07T03:31:53Z
dc.descriptionA 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.
dc.description3 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)
dc.identifierhttps://arxiv.org/abs/gr-qc/9710078
dc.identifierhttp://arxiv.org/abs/gr-qc/9710078
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36028
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCylindrical Domain Walls and Gravitational Waves -- Einstein Rosen wave emission from momentarily static initial configuration --
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