Dark energy cosmology with generalized linear equation of state
From MaRDI portal
Publication:4665161
DOI10.1088/0264-9381/22/1/010zbMath1060.83059arXivastro-ph/0407190OpenAlexW1995015179MaRDI QIDQ4665161
Yu. N. Eroshenko, E. Babichev, Vyacheslav I. Dokuchaev
Publication date: 9 April 2005
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0407190
Related Items (34)
Bulk viscosity in Friedmann universe with a varying speed of light described by modified equation of state ⋮ Modeling the quantum evolution of the universe through classical matter ⋮ Thermodynamical and observational aspects of cosmological model with linear equation of state ⋮ Modified gravity theories on a nutshell: inflation, bounce and late-time evolution ⋮ Pre-inflationary spacetime in string cosmology ⋮ Unitarity at infinity and topological holography ⋮ DARK VISCOUS FLUID DESCRIBED BY A UNIFIED EQUATION OF STATE IN COSMOLOGY ⋮ NETWORKS OF COSMOLOGICAL HISTORIES, CROSSING OF THE PHANTOM DIVIDE LINE AND POTENTIALS WITH CUSPS ⋮ Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories ⋮ Screening of cosmological constant for de Sitter universe in non-local gravity, phantom-divide crossing and finite-time future singularities ⋮ FRW viscous fluid cosmological model with time-dependent inhomogeneous equation of state ⋮ Universal procedure to cure future singularities of dark energy models ⋮ Interpretation of f(R,T) gravity in terms of a conserved effective fluid ⋮ An exact Chameleon cosmological model unifying phantom inflation with late-time acceleration ⋮ Cosmological model with viscosity media (dark fluid) described by an effective equation of state ⋮ Inhomogeneous viscous fluid cosmological model of the universe with effective equation of state and scalar field ⋮ SOME CONSEQUENCES OF DARK ENERGY DENSITY VARYING EXPONENTIALLY WITH SCALE FACTOR ⋮ Vaidya spacetimes, black-bounces, and traversable wormholes ⋮ Qualitative study of a model with Rastall gravity ⋮ The linear stability of the n + 1 dimensional FLRW spacetimes ⋮ Evolution of a Schwarzschild black hole in phantom-like Chaplygin gas cosmologies ⋮ Charged black holes in phantom cosmology ⋮ Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy ⋮ Oscillating universe from an inhomogeneous equation of state and coupled dark energy ⋮ Holography in \((2+1)\)-dimensional cosmological model with generalized equation of state ⋮ Universe with wet dark fluid: A dynamical systems approach ⋮ THERMODYNAMICS OF A SCHWARZSCHILD BLACK HOLE IN PHANTOM COSMOLOGY WITH ENTROPY CORRECTIONS ⋮ Evolving black holes in inflation ⋮ Charged and non-charged black hole solutions in mimetic gravitational theory ⋮ DYNAMICS OF DARK ENERGY ⋮ PHANTOM UNIVERSE FROM CPT SYMMETRIC QFT ⋮ SOME ASPECTS OF GENERALIZED MODIFIED GRAVITY MODELS ⋮ Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests ⋮ Brane Kantowski-Sachs universe with linear equation of state and a future singularity
This page was built for publication: Dark energy cosmology with generalized linear equation of state