Inhomogeneous early viscous fluid universe: A concrete model for dark energy
DOI10.1142/S0219887816500377zbMath1339.83084OpenAlexW2234521214MaRDI QIDQ2805555
Publication date: 12 May 2016
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0219887816500377
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Stability and instability of geophysical and astrophysical flows (76E20) Astrophysical cosmology (85A40)
Cites Work
- Cosmological model with viscosity media (dark fluid) described by an effective equation of state
- Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
- Matter creation and bulk viscosity in early cosmology
- FRW viscous cosmology with inhomogeneous equation of state and future singularity
- VISCOUS FRW MODELS WITH PARTICLE CREATION IN EARLY UNIVERSE
- VISCOUS FRW COSMOLOGY IN MODIFIED GRAVITY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- EARLY HOMOGENEOUS UNIVERSE WITH VARIABLE COSMOLOGICAL CONSTANT: KINEMATICS TESTS
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