Perfect and viscous fluid cosmological models in presence of scalar fields for anisotropic metric

DOI10.1007/BF00627545zbMath0836.76105MaRDI QIDQ1905405

Pijush K. Maiti, Akhil Ranjan Roy

Publication date: 8 May 1996

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

zbMATH Keywords

Einstein equationsdissipative processesscale factorscigar singularity

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

• Viscous fluid cosmological models in the presence of the zero-mass scalar field
• Anisotropic cosmological models with energy density dependent bulk viscosity
• New cosmological models
• New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity
• The Large Scale Structure of Space-Time
• Inhomogeneous viscous cosmologies without singularity

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