Holographic description of the dissipative unified dark fluid model with axion field
arXiv:2309.06916 · doi:10.1142/S0218271823500852
Abstract
In this article we extend an axion F(R) gravity model, and apply the holographic principle to describe in a unifying manner the early and the late-time universe when the general equation of state (EoS) contains a bulk viscosity. We assume a spatially flat Friedmann-Robertson-Walker (FRW) universe model. We use a description based on the generalized infrared-cutoff holographic dark energy proposed by Nojiri and Odintsov (2006, 2017), and explore the evolution of the universe when the EoS describes the asymptotic behavior between the dust in the early universe and the late universe. We explore various forms of the bulk viscosity, and calculate analytical expressions for the infrared cutoffs in terms of the particle horizon. In this way we obtain a unifying description of the early and the late-time universe in the presence of axion matter, via a viscous holographic fluid model.
arXiv comment7 pages, latex 2e, to appear in Int. J. Mod. Phys. D
References in corpus (33)
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A Model of Holographic Dark Energy
- The holographic principle
- 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
- 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
- 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
- Covariant Generalized Holographic Dark Energy and Accelerating Universe
- Barrow entropic dark energy: A member of generalized holographic dark energy family
- Unifying Holographic Inflation with Holographic Dark Energy: a Covariant Approach
- Constraints on the dark energy from holography
- A CMB/Dark Energy Cosmic Duality
- Unification of Inflation with Dark Energy in Gravity and Axion Dark Matter
- Observational constraints on holographic dark energy with varying gravitational constant
- Geometric Inflation and Dark Energy with Axion Gravity
- Hint for Quintessence-like Scalars from Holographic Dark Energy
- Aspects of Axion Gravity
- Multiple Lambda cosmology: dark fluid with time-dependent equation of state as classical analog of cosmological landscape
- Gravity with an Axion-like Particle: Dynamics, Gravity Waves, Late and Early-time Phenomenology
- Is the axionic dark matter an equilibrium system?
- Dissipative Unified Dark Fluid Model
- Holographic representation of the unified early and late universe via a viscous dark fluid
- Some models of holographic dark energy on the Randall-Sundrum brane and observational data
- A Viable Dark Fluid Model
- The Holographic cosmology with axion field