Inhomogeneous viscous fluid cosmological model of the universe with effective equation of state and scalar field

DOI10.1142/S0219887818500780zbMath1387.83128MaRDI QIDQ4635342

G. S. Khadekar, Rupali Talole

Publication date: 16 April 2018

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

scalar fielddark energyeffective equation of stateinhomogeneous viscous fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Cites Work

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• Gauge fields and inflation
• Viscous inflationary universe models
• Remarks on the viscosity concept in the early universe
• Quantum de Sitter cosmology and phantom matter
• Dark energy and viscous cosmology
• Viscous brane cosmology with a brane-bulk energy interchange term
• FRW viscous cosmology with inhomogeneous equation of state and future singularity
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• VISCOUS FRW COSMOLOGY IN MODIFIED GRAVITY
• Cosmological solutions with nonlinear bulk viscosity
• Modified Friedmann equations in R  ¹ -modified gravity
• FRW viscous fluid cosmological model with time-dependent inhomogeneous equation of state
• Dark energy cosmology with generalized linear equation of state
• SUPERQUINTESSENCE
• Full causal bulk-viscous cosmological models
• Sudden future singularities
• Viscous cosmology for early- and late-time universe