Rotating magnetoviscous-fluid universes in general relativity

DOI10.1007/BF00653560zbMath0688.76080OpenAlexW2001935757MaRDI QIDQ1264081

Koijam Maniharsingh

Publication date: 1990

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

Full work available at URL: https://doi.org/10.1007/bf00653560

zbMATH Keywords

analytic solutionsmagnetoviscous-fluid distributionRotating models

Mathematics Subject Classification ID

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

Related Items

Some rotating perfect fluid universes coupled with electromagnetic field interacting with gravitation ⋮ 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

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