Solution of Einstein's Field Equations for a Rotating, Stationary, and Dust-Filled Universe

DOI10.1063/1.1704246zbMath0125.45405OpenAlexW2026975200MaRDI QIDQ5331343

James P. Wright

Publication date: 1965

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

Full work available at URL: https://doi.org/10.1063/1.1704246

zbMATH Keywords

classical field theory, relativity theory

Related Items (14)

A class of shear-free perfect fluids in general relativity. II ⋮ Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ Homogeneous and hypersurface-homogeneous shear-free perfect fluids in general relativity ⋮ All flow-stationary cylindrically symmetric solutions of the Einstein field equations for a rotating isentropic perfect fluid ⋮ Some solutions of the Einstein field equations for a rotating perfect fluid ⋮ Rotating charged perfect-fluid universes coupled with scalar field in general relativity ⋮ Rotational perturbations of magneto-viscous fluid universes coupled with zero-mass scalar field ⋮ On slowly-rotating cosmological viscous-fluid model universes in general relativity ⋮ Cylindrical systems in general relativity ⋮ Rotational perturbations of charged cosmological viscous-fluid universes coupled with a scalar field ⋮ Rotating magnetoviscous-fluid universes in general relativity ⋮ Time-dependent, finite, rotating universes ⋮ Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα ⋮ Rotational perturbations of relativistic perfect-fluid model universes interacting with gravitational field

Cites Work

• An Example of a New Type of Cosmological Solutions of Einstein's Field Equations of Gravitation

This page was built for publication: Solution of Einstein's Field Equations for a Rotating, Stationary, and Dust-Filled Universe