Cylindrical gravitational waves in expanding universes: Models for waves from compact sources

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dc.creatorGowdy, Robert H.
dc.creatorEdmonds, B. Douglas
dc.date2007-01-29
dc.date2007-04-06
dc.date.accessioned2026-07-07T11:01:39Z
dc.date.available2026-07-07T11:01:39Z
dc.descriptionNew boundary conditions are imposed on the familiar cylindrical gravitational wave vacuum spacetimes. The new spacetime family represents cylindrical waves in a flat expanding (Kasner) universe. Space sections are flat and nonconical where the waves have not reached and wave amplitudes fall off more rapidly than they do in Einstein-Rosen solutions, permitting a more regular null inifinity.
dc.descriptionMinor corrections to references. A note added in proof
dc.identifierhttps://arxiv.org/abs/gr-qc/0701161
dc.identifierhttp://arxiv.org/abs/gr-qc/0701161
dc.identifierPhys.Rev.D75:084011,2007
dc.identifierdoi:10.1103/PhysRevD.75.084011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188014
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCylindrical gravitational waves in expanding universes: Models for waves from compact sources
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