Rotational perturbations of charged cosmological viscous-fluid universes coupled with a scalar field

DOI10.1007/BF00653350zbMath0687.76122MaRDI QIDQ1263494

Manihar Singh Koijam

Publication date: 1989

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

zero-mass scalar fieldrotational perturbationscharged fieldperfect draggingslowly rotating charged viscous-fluid universe

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (4)

Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity ⋮ On slowly-rotating cosmological viscous-fluid model universes in general relativity ⋮ Rotational perturbations of radiating universes coupled with zero-mass scalar field ⋮ Rotational perturbations of relativistic perfect-fluid model universes interacting with gravitational field

Cites Work

• Slowly-rotating cosmological perfect fluids
• Rotational perturbations of cosmological viscous-fluid universe with zero-mass scalar field
• Rotating Fields in General Relativity
• Stationary weak gravitational fields to any order of approximation
• Charged viscous fluids: Exact solutions
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• Stationary gravitational fields due to single bodies
• Solution of Einstein's Field Equations for a Rotating, Stationary, and Dust-Filled Universe
• The gravitational field of a rotating fluid mass in general relativity

This page was built for publication: Rotational perturbations of charged cosmological viscous-fluid universes coupled with a scalar field