Add to ORKGWe perform a dynamical system analysis and a Bayesian model selection for a new set of interacting scenarios in the framework of modified holographic Ricci dark energy models (MHR-IDE). The dynamical analysis shows a modified radiation epoch and a late-time attractor corresponding to dark energy. We use a combination of background data such as type Ia supernovae, cosmic chronometers, cosmic microwave background, and baryon acoustic oscillations measurements. We find evidence against all the MHR-IDE scenarios studied with respect to $\Lambda$CDM, when the full joint analysis is considered.Comment: 21 page
We consider two models of interacting dark energy, both of which interact only through momentum exch...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...
We extend the holographic Ricci dark energy model to include some direct, non-gravitational interact...
We examine a Friedmann-Robertson-Walker universe filled with interacting dark matter, modified holog...
We revise the dynamical properties of a class of cosmological models where the dark sector interacts...
The background cosmological dynamics of the late Universe is analysed on the framework of a dark ene...
We consider the Interacting Tsallis Holographic Dark Energy (THDE) as dynamical vacuum, with the Gra...
The phenomenologically emergent dark energy (PEDE) model is a varying dark energy model with no extr...
We construct a holographic model for dark energy in the Brans-Dicke cosmology by using the holograph...
We investigate both the interacting and non-interacting R\'{e}nyi Holographic Dark Energy (RHDE) mod...
In this work we explore the scope of two holographic dark energy models within the interacting scena...
In this paper, we examine two types of interacting holographic dark energy model using Pantheon supe...
We extend the holographic Ricci dark energy model to include some direct, non-gravitational interact...
We formulate power-law holographic dark energy, which is a modified holographic dark energy model ba...
Cosmological features of Barrow Holographic Dark Energy (BHDE), a recent generalization of original ...
We consider two models of interacting dark energy, both of which interact only through momentum exch...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...
We extend the holographic Ricci dark energy model to include some direct, non-gravitational interact...
We examine a Friedmann-Robertson-Walker universe filled with interacting dark matter, modified holog...
We revise the dynamical properties of a class of cosmological models where the dark sector interacts...
The background cosmological dynamics of the late Universe is analysed on the framework of a dark ene...
We consider the Interacting Tsallis Holographic Dark Energy (THDE) as dynamical vacuum, with the Gra...
The phenomenologically emergent dark energy (PEDE) model is a varying dark energy model with no extr...
We construct a holographic model for dark energy in the Brans-Dicke cosmology by using the holograph...
We investigate both the interacting and non-interacting R\'{e}nyi Holographic Dark Energy (RHDE) mod...
In this work we explore the scope of two holographic dark energy models within the interacting scena...
In this paper, we examine two types of interacting holographic dark energy model using Pantheon supe...
We extend the holographic Ricci dark energy model to include some direct, non-gravitational interact...
We formulate power-law holographic dark energy, which is a modified holographic dark energy model ba...
Cosmological features of Barrow Holographic Dark Energy (BHDE), a recent generalization of original ...
We consider two models of interacting dark energy, both of which interact only through momentum exch...
Using various latest cosmological datasets including Type-Ia supernovae, cosmic microwave background...
We extend the holographic Ricci dark energy model to include some direct, non-gravitational interact...