Time-dependent, finite, rotating universes

DOI10.1063/1.524850zbMath0471.70001OpenAlexW1662388525MaRDI QIDQ3926084

J. Ademir S. de Lima, M. J. Rebouças

Publication date: 1981

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.524850

zbMATH Keywords

rotationshearthree-spherefinite, homogeneous and nonsingular exact cosmological solutionst-constant sections of Bianchi type IXtime- dependent expansion

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Differential geometric methods (tensors, connections, symplectic, Poisson, contact, Riemannian, nonholonomic, etc.) for problems in mechanics (70G45) Axiomatics, foundations (70A05)

Related Items

Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα, TILTED BIANCHI TYPE-V BAROTROPIC FLUID COSMOLOGICAL MODELS WITH VARIABLE BULK VISCOSITY IN GENERAL RELATIVITY, Bianchi VI\(_ 0\) electric type cosmological models in general relativity with stiff fluid and heat conduction, Bianchi type V models with a matter distribution admitting ansiotropic pressure and heat flow, BIANCHI TYPE V COSMOLOGICAL MODELS WITH PERFECT FLUID AND HEAT CONDUCTION IN LYRA'S GEOMETRY, On nonperfect fluid cosmologies evolving towards perfect fluid cosmological models, Generalized Stephani universes, Some cosmological models with heat and null radiation flow, A CLASS OF CYLINDRICALLY SYMMETRICAL MODELS WITH HEAT FLOW, Some exact Bianchi type-V perfect fluid cosmological models with heat flow and decaying vacuum energy density \(\Lambda \): expressions for some observable quantities, FEATURES OF A ROTATING SPACETIME, Some exact Bianchi type V perfect fluid solutions with heat flow

Cites Work

• Tilted homogeneous cosmological models
• Solution of Einstein's Field Equations for a Rotating, Stationary, and Dust-Filled Universe
• IX.—The Gravitational Field of a Distribution of Particles Rotating about an Axis of Symmetry
• An Example of a New Type of Cosmological Solutions of Einstein's Field Equations of Gravitation
• Empty space-times admitting a three parameter group of motions