1971/09/20 by Robert H. Gowdy · 2 citations
Physics and Astronomy · #Cosmology and Gravitation Theories #Relativity and Gravitational Theory #Quantum Mechanics and Applications
paper · doi:10.1103/physrevlett.27.826
openalex publication_date 1971/09/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/04/04
New boundary conditions on the Einstein-Rosen-Bondi gravitational-wave metrics yield closed inhomogeneous universes which solve Einstein's vacuum field equations exactly. Space sections of these universes have either the three-sphere topology S3 or the wormhole (hypertorus) topology S1\ensuremath\bigotimesS2.