An interacting holographic dark energy model within an induced gravity brane
arXiv:1812.06782 · doi:10.1142/S0218271820500662
Abstract
In this paper, we present a model for the late-time evolution of the universe where a dark energy-dark matter interaction is invoked. Dark energy is modeled through an holographic Ricci dark energy component. The model is embedded within an induced gravity brane-world model. For suitable choices of the interaction coupling, the big rip and little rip induced by the holographic Ricci dark energy, in a relativistic model and in an induced gravity brane-world model, are removed. In this scenario, the holographic dark energy will have a phantom-like behaviour even though the brane is asymptotically de Sitter.
arXiv comment16 pages, 16 figures. Style and presentation improved. References added. Physics unchanged. Text overlap with our former work arXiv:1112.5836
References in corpus (52)
- The Cosmological Constant and Dark Energy
- The World as a Hologram
- A Model of Holographic Dark Energy
- Essentials of k-essence
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Properties of singularities in (phantom) dark energy universe
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- Cosmology on a Brane in Minkowski Bulk
- Entropy Bounds and 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
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- A Holographic Dark Energy Model from Ricci Scalar Curvature
- Probing the Coupling between Dark Components of the Universe
- Dynamics of dark energy with a coupling to dark matter
- Constraints on the interacting holographic dark energy model
- The Little Rip
- Viscous Little Rip Cosmology
- Le Chatelier-Braun principle in cosmological physics
- "Expansion" around the vacuum equation of state - sudden future singularities and asymptotic behavior
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Worse than a big rip?
- New Cosmological Singularities in Braneworld Models
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Toward a solution of the coincidence problem
- Testing the interaction between dark energy and dark matter via latest observations
- Observational constraints on the dark energy and dark matter mutual coupling
- Brane cosmology with curvature corrections
- Interacting models of soft coincidence
- Evidence for interacting dark energy from BOSS
- Dynamics of interacting dark energy model in Einstein and Loop Quantum Cosmology
- Holographic dark energy in the DGP braneworld with GO cutoff
- The little sibling of the big rip singularity
- A model of interacting holographic dark energy at the Ricci's scale
- Phantom-like behaviour in dilatonic brane-world scenario with induced gravity
- The cosmology of an holographic induced gravity model with curvature effects
- Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
- Modified holographic Ricci dark energy coupled to interacting dark matter and a non interacting baryonic component
- The holographic induced gravity model with a Ricci dark energy: smoothing the little rip and big rip through Gauss-Bonnet effects?
- Soft coincidence in late acceleration
- Tradeoff between Smoother and Sooner "Little Rip"
- Dark matter, dark energy, and dark radiation coupled with a transversal interaction
- The late Universe with non-linear interaction in the dark sector: the coincidence problem
- More on the holographic Ricci dark energy model: smoothing Rips through interaction effects?
- Finite time future singularities in the interacting dark sector
- Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld
- New holographic dark energy model inspired by the DGP braneworld
- Cosmological constraints on Agegraphic dark energy in DGP braneworld gravity
- Aspects of Some New Versions of Pilgrim Dark Energy in DGP Braneworld
- Probing Lambda-DGP Braneworld Model