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

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

2007-01-29

arxiv.org/abs/gr-qc/0701161v3

Phys.Rev.D75:084011,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Minor corrections to references. A note added in proof

Scientific paper

10.1103/PhysRevD.75.084011

New 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.

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