1975
DOI: 10.1063/1.522529
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Closed gravitational−wave universes: Analytic solutions with two−parameter symmetry

Abstract: Einstein’s vacuum field equations are solved for spacetimes with two−parameter spacelike symmetry, a space−reflection symmetry, and space sections homeomorphic to either S1×S2 or S3. All integrals are evaluated, and the spacetime metrics are presented in analytic form.

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Cited by 20 publications
(15 citation statements)
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“…They may therefore be considered as Gowdy-type space-times [20], [21]. It can readily be verified that here the regularity conditions across the null hypersurface η = ζ are satisfied.…”
Section: Toroidal Waves In a Closed Frw Modelmentioning
confidence: 82%
“…They may therefore be considered as Gowdy-type space-times [20], [21]. It can readily be verified that here the regularity conditions across the null hypersurface η = ζ are satisfied.…”
Section: Toroidal Waves In a Closed Frw Modelmentioning
confidence: 82%
“…However, it was common knowledge among relativists that gravitational waves (which have T μν = 0) carry both energy and angular momentum, and their energy too must have inertia. In fact, Gowdy (1975) has produced a closed universe solution of Einstein's equations, which is closed by the gravity of the gravitational waves in it whose stress tensor is zero everywhere. Jiri Bicak has great expertise in gravitational waves.…”
Section: Einstein Also Wrotementioning
confidence: 99%
“…Various generalizations of the Kerr solution have been done (see, e.g., [16] and [2]). Gowdy [6]- [7] constructed a new kind of solutions of the vacuum Einstein's equations, these solutions provide a new type of cosmological model. This model describes a closed inhomogeneous universe, space sections of these universes have either the three-sphere topology S 3 or the wormhole (hypertorus) topology S 1 ⊗ S 2 .…”
mentioning
confidence: 99%
“…According to the authors' knowledge, (6) gives the first time-periodic solution to the Einstein's field equations. Here we would like to point out that, by using our method, we can re-derive almost all known exact solutions to the vacuum Einstein's field equations, for examples, Gödel's solution [5], Khan-Penrose's solution [11], Gowdy's solution [6]- [7], etc. Our method can also be used to find exact solutions of the Einstein's field equations in higher dimensions which will be of interests in string theory.…”
mentioning
confidence: 99%