On average properties of inhomogeneous fluids in general relativity: Perfect fluid cosmologies
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Publication:5955373
DOI10.1023/A:1012061725841zbMath1020.83035arXivgr-qc/0102049OpenAlexW3105807893MaRDI QIDQ5955373
Publication date: 23 September 2003
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0102049
cosmologyaveraged propertiesgeneral relativistic hydrodynamicsgeneralized Friedmann's equationsirrotational perfect fluids
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
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Cites Work
- How is the local-scale gravitational instability influenced by the surrounding large-scale structure formation?
- On average properties of inhomogeneous fluids in general relativity: Dust cosmologies
- Tilted homogeneous cosmological models
- General relativistic shock waves in fluids for which pressure equals energy density
- Scalar fields in curved spacetimes
- Gauge-invariant perturbations in a scalar field dominated universe
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