Effects of the shear viscosity on the character of cosmological evolution

DOI10.1063/1.528901zbMath0704.76072arXivgr-qc/0308060OpenAlexW3098105837MaRDI QIDQ3484581

Wung-Hong Huang

Publication date: 1990

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0308060

zbMATH Keywords

shear viscosityenergy densitystiff fluidpower functionBianchi type I cosmological modelsisotropic Friedmann universecosmological evolutionsEinstein initial singularityHubble functions

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 (3)

Anisotropic cosmological models with energy density dependent bulk viscosity ⋮ STRING DUST COSMOLOGICAL MODEL IN HIGHER-DIMENSIONAL SPACE–TIME ⋮ Viscous cosmologies

Cites Work

• Isotropic homogeneous universe with viscous fluid
• Bianchi type I cosmological model with a viscous fluid
• Inflationary universe: A possible solution to the horizon and flatness problems

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