Cardy-Verlinde formula in FRW Universe with inhomogeneous generalized fluid and dynamical entropy bounds near the future singularity
arXiv:1002.1942 · doi:10.1140/epjc/s10052-010-1425-0
Abstract
We derive a Cardy-Verlinde-like formula which relates the entropy of the closed FRW universe to its energy, and Casimir energy, for a multicomponent coupled fluid. The generalized fluid obeys an inhomogeneous equation of state. A viscous dark fluid is included, and we include also modified gravity using its fluid representation. It is demonstrated how such an expression reduces to the standard Cardy-Verlinde formula corresponding to the 2d CFT entropy only in some special cases. The dynamical entropy bound for a closed FRW universe with dark components is obtained. The universality of the dynamical entropy bound near a future singularity (of all four types), as well as near the Big Bang singularity, is investigated. It is demonstrated that except from some special cases of Type II and Type IV singularities the dynamical entropy bound is violated near the singularity even if quantum effects are taken into account. The dynamical entropy bound seems to be universal for the case of a regular universe, including the asymptotic de Sitter one.
14 pages. Published version
References in corpus (17)
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- Future of the universe in modified gravitational theories: Approaching to the finite-time future singularity
- The future evolution and finite-time singularities in -gravity unifying the inflation and cosmic acceleration
- Dark Energy: the equation of state description versus scalar-tensor or modified gravity
- The new form of the equation of state for dark energy fluid and accelerating universe
- Reconstructing the universe history, from inflation to acceleration, with phantom and canonical scalar fields
- Worse than a big rip?
- Classification of cosmological milestones
- Dynamics of Nonlocal Cosmology
- Quantum phantom cosmology
- Avoidance of future singularities in loop quantum cosmology
- Can higher curvature corrections cure the singularity problem in f(R) gravity?
- Delicate f(R) gravity models with disappearing cosmological constant and observational constraints on the model parameters
- Viscous Dark Cosmology with Account of Quantum Effects
- Strings at future singularities
- Astronomical bounds on future big freeze singularity
- Modified f(R) gravity from scalar-tensor theory and inhomogeneous EoS dark energy
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- Viscous Cosmology for Early- and Late-Time Universe
- Dark Energy Coupled with Dark Matter in Viscous Fluid Cosmology
- Finite-time future singularities models in gravity and the effects of viscosity
- Entropic cosmology in a dissipative universe
- Cosmology of a generalised version of holographic dark energy in presence of bulk viscosity and its inflationary dynamics through slow roll parameters
- Dissipative Universe-Inflation with Soft Singularity
- The effect of thermal radiation on singularities in the dark universe
- Universal thermodynamics in different gravity theories: Conditions for generalized second law of thermodynamics and thermodynamical equilibrium on the horizons
- Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology
- Singular behavior of the dark universe under the effect of thermal radiation in curved spacetime
- WIMP dark matter in bulk viscous non-standard cosmologies
- Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies
- Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid
- Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid
- FIMP Dark Matter in bulk viscous non-standard cosmologies
- Holographic description of the dissipative model of universe with curvature
- The d-Dimensional Cosmological Constant and the Holographic Horizons