Some solutions of the Einstein field equations for a rotating perfect fluid

DOI10.1063/1.522404zbMath0291.76042OpenAlexW1964896320WikidataQ124820729 ScholiaQ124820729MaRDI QIDQ4042780

Andrzej Krasiński

Publication date: 1975

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

Full work available at URL: https://doi.org/10.1063/1.522404

Mathematics Subject Classification ID

Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (11)

Study of stationary rigidly rotating anisotropic cylindrical fluids with new exact interior solutions of GR. II. More about axial pressure ⋮ Fully integrated interior solutions of GR for stationary rigidly rotating cylindrical perfect fluids ⋮ Geodesic motion and confinement in van Stockum space–time ⋮ Rotating dust solutions of Einstein’s equations with three-dimensional symmetry groups. III. All Killing fields linearly independent of uα and wα ⋮ The parameters of the Lewis metric for the Weyl class ⋮ All flow-stationary cylindrically symmetric solutions of the Einstein field equations for a rotating isentropic perfect fluid ⋮ GLOBAL AND LOCAL EFFECTS OF ROTATION: OBSERVATIONAL ASPECTS ⋮ An approximate global solution of Einstein's equations for a rotating finite body ⋮ Rotating dust solutions of Einstein’s equations with 3-dimensional symmetry groups. I. Two Killing fields spanned on uα and wα ⋮ The Linet–Tian metrics are a restricted set of Krasiński’s solutions of Einstein’s field equations for a rotating perfect fluid ⋮ An approximated solution of the Einstein equations for a rotating body with negligible mass

Cites Work

• Eindimensionale Gravitationsfelder
• Some special solutions of the equations of axially symmetric gravitational fields
• Solution of Einstein's Field Equations for a Rotating, Stationary, and Dust-Filled Universe
• New Homogeneous Solutions of Einstein's Field Equations with Incoherent Matter Obtained by a Spinor Technique
• 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

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