Rotational perturbations of magneto-viscous fluid universes coupled with zero-mass scalar field

DOI10.1007/BF00648181zbMath0850.76897OpenAlexW2063240989MaRDI QIDQ1177120

Koijam Maniharsingh

Publication date: 26 June 1992

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

Full work available at URL: https://doi.org/10.1007/bf00648181

Mathematics Subject Classification ID

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

Related Items (5)

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 ⋮ Radiating anisotropic two-fluid model universes involving rotation in general relativity ⋮ 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
• Slowly rotating perfect-fluid universes coupled with zero-mass scalar field
• Rotating Fields in General Relativity
• Stationary weak gravitational fields to any order of approximation
• 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

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