Viscous fluid cosmological models in the presence of the zero-mass scalar field

DOI10.1007/BF00644207zbMath0756.76098MaRDI QIDQ1194614

Pijush K. Maiti, Akhil Ranjan Roy

Publication date: 13 October 1992

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

zbMATH Keywords

shear viscosityinitial singularitynon-static scalar fields

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (4)

Perfect and viscous fluid cosmological models in presence of scalar fields for anisotropic metric ⋮ Singularity-free RW viscous fluid cosmological models in presence of massive scalar fields ⋮ Singularity-free RW viscous fluid cosmological models in presence of massive scalar fields ⋮ Magneto-viscous fluid cosmological models in presence of zero-mass scalar field

Cites Work

• R-W cosmological models with zero-mass scalar fields for different equations of state
• Relativity theory and the creation of matter

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