Viscous Fluid Holographic Bounce
arXiv:1911.09519 · doi:10.1142/S0219887820500231
Abstract
We investigate bounce cosmological models in the presence of a viscous fluid, making use of generalized holographic cutoffs introduced by Nojiri and Odintsov (2017). We consider both an exponential, a power-law, and a double exponential form for the scale factor. By use of these models we calculate expressions for infrared cutoffs analytically, such that they correspond to the particle horizon at the bounce. Finally we derive the energy conservation equation, from the holographic point of view. In that way the relationship between the viscous fluid bounce and the holographic bounce is demonstrated.
10 pages; to appear in International Journal of Geometric Methods in Modern Physics
References in corpus (41)
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A Model of Holographic Dark Energy
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
- Holographic dark energy and cosmic coincidence
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Holographic Dark Energy
- Constraints on holographic dark energy from type Ia supernova observations
- Towards a Nonsingular Bouncing Cosmology
- The Holographic Dark Energy in a Non-flat Universe
- Dark Energy: Vacuum Fluctuations, the Effective Phantom Phase, and Holography
- Observational constraints on dark energy with generalized equations of state
- Bouncing Cosmologies: Progress and Problems
- Statefinder diagnostic for holographic dark energy model
- Supernova Constraints on a holographic dark energy model
- Holographic dark energy models: A comparison from the latest observational data
- Bounce cosmology from gravity and bigravity
- Covariant Generalized Holographic Dark Energy and Accelerating Universe
- Exploring Bouncing Cosmologies with Cosmological Surveys
- Holography and Variable Cosmological Constant
- Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
- Categorizing Different Approaches to the Cosmological Constant Problem
- Constraints on the dark energy from holography
- Holography for inflation using conformal perturbation theory
- A CMB/Dark Energy Cosmic Duality
- Matter Bounce Loop Quantum Cosmology from Gravity
- Observational constraints on holographic dark energy with varying gravitational constant
- Bouncing cosmologies with dark matter and dark energy
- An Extended Matter Bounce Scenario: current status and challenges
- The Holographic Universe
- Hint for Quintessence-like Scalars from Holographic Dark Energy
- Inflationary universe in terms of a van der Waals viscous fluid
- Characteristic Properties of Two Different Viscous Cosmology Models for the Future Universe
- Unstable growth of curvature perturbation in non-singular bouncing cosmologies
- Inhomogeneous viscous fluids in FRW universe and finite-future time singularities
- Bounce Universe Induced by an Inhomogeneous Dark Fluid Coupled with Dark Matter
- Inhomogeneous viscous dark fluid coupled with dark matter in the FRW universe
- Viscous Coupled Fluids in Inflationary Cosmology
- Inflationary Universe with a Viscous Fluid Avoiding Self-Reproduction
Cited by in corpus (11)
- Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
- An analysis of the tension problem in a universe with a viscous dark fluid
- Holographic realization from inflation to reheating in generalized entropic cosmology
- Holographic representation of the unified early and late universe via a viscous dark fluid
- An approach to cold dark matter deviation and the tension problem by using machine learning
- Little Rip, Pseudo Rip and bounce cosmology with generalized equation of state in non-standard backgrounds
- Holographic cosmology with two coupled fluids in the presence of viscosity
- The Holographic cosmology with axion field
- Thermodynamics of the most generalized form of Holographic Dark Energy and some particular cases with Corrected Entropies
- Non-Singular Bouncing cosmology from Phantom Scalar-Gauss-Bonnet Coupling: Reconstruction with Observational Insights
- Implementation of cosmological bounce inflation with Nojiri-Odintsov generalized holographic dark fluid