Characteristic properties of two different viscous cosmology models for the future universe
From MaRDI portal
Publication:2968286
DOI10.1142/S0217732317500262zbMath1357.83021arXiv1612.01794MaRDI QIDQ2968286
Ben David Normann, Iver Brevik
Publication date: 13 March 2017
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1612.01794
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
Related Items (11)
Bianchi type-\(I\) bulk viscosity with a DE cosmological model ⋮ Can the Hubble tension be resolved by bulk viscosity? ⋮ Inflation in terms of a viscous van der Waals coupled fluid ⋮ Dark energy nature of viscus universe in f(Q)-gravity with observational constraints ⋮ FRW viscous fluid cosmological model with time-dependent inhomogeneous equation of state ⋮ Phantom dark energy nature of bulk-viscosity universe in modified f(Q)-gravity ⋮ Cosmology with viscous generalized Chaplygin gas in \(f(Q)\) gravity ⋮ Bulk viscous cosmological model in f(R,T) theory of gravity ⋮ Black holes in the turbulence phase of viscous rip cosmology ⋮ Reconstruction of \(\Lambda\)CDM model from \(f(T)\) gravity in viscous-fluid universe with observational constraints ⋮ Nonlinear viscous cosmological models in f(R,T) gravity
Cites Work
- Viscous varying generalized Chaplygin gas with cosmological constant and space curvature
- Viscous \(\Lambda \)CDM universe models
- Viscous inflationary universe models
- Black holes in bulk viscous cosmology
- Quantum de Sitter cosmology and phantom matter
- Dark energy and viscous cosmology
- Modified Chaplygin gas cosmology with bulk viscosity
- CROSSING OF THE w = -1 BARRIER IN VISCOUS MODIFIED GRAVITY
This page was built for publication: Characteristic properties of two different viscous cosmology models for the future universe
