Perfect fluids satisfying a less than extremely relativistic equation of state

DOI10.1063/1.527581zbMath0624.76136OpenAlexW2026726615MaRDI QIDQ3026678

Basilis C. Xanthopoulos

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1063/1.527581

zbMATH Keywords

inhomogeneous cosmological modelsperfect fluidsfamilies of exact solutionscollision of two plane gravitational and hydrodynamics waveslinear polarizationsspacelike, hypersurface orthogonal Killing fields

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (1)

Dark energy with generalized equation of state in Bianchi type-I cosmological model

Cites Work

• Spatially homogeneous and inhomogeneous cosmologies with equation of state p=mu
• On the Nutku—Halil solution for colliding impulsive gravitational waves
• On the collision of impulsive gravitational waves when coupled with fluid motions
• Perfect fluids with vanishing Simon tensor
• On colliding waves in the Einstein—Maxwell theory
• Eine rotationssymmetrische Lösung in der allgemeinen Relativitätstheorie

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