Bayesian comparison of interacting modified holographic Ricci dark energy scenarios

@article{Cid2021BayesianCO,
  title={Bayesian comparison of interacting modified holographic Ricci dark energy scenarios},
  author={Antonella Cid and Carlos Rodriguez-Benites and M. Cataldo and Gonz Alez Casanova},
  journal={The European Physical Journal C},
  year={2021},
  volume={81},
  pages={1-10}
}
We perform a Bayesian model selection analysis for interacting scenarios of dark matter and modified holographic Ricci dark energy (MHRDE) with linear interacting terms. We use a combination of some of the latest cosmological data such as type Ia supernovae, cosmic chronometers, the local value of the Hubble constant, baryon acoustic oscillations measurements and cosmic microwave background through the angular scale of the sound horizon at last scattering. We find moderate/strong evidence… 

References

SHOWING 1-10 OF 91 REFERENCES

Current observational constraints on holographic dark energy model

We consider the cosmological constraints on the holographic dark energy model by using the data set available from the type Ia supernovae (SNIa), CMB and BAO observations. The constrained parameters

Holographic reconstruction of the k-essence and dilaton models

We propose an holographic $k$-essence and dilaton models of dark energy. The correspondence between the $k$-essence and dilaton energy densities with the holographic density, allows the

Holography, UV/IR Relation, Causal Entropy Bound, and Dark Energy

The constraint on the total energy in a given spatial region is given from holography by the mass of a black hole that just fits in that region, which leads to an UV/IR relation: the maximal energy

The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000)

The old cosmological constant problem is to understand why the vacuum energy is so small; the new problem is to understand why it is comparable to the present mass density. Several approaches to

Tensions between the early and late Universe

The standard cosmological model successfully describes many observations from widely different epochs of the Universe, from primordial nucleosynthesis to the accelerating expansion of the present

Scolnic et al., Astrophys

  • J. 859,
  • 2018

AIP Conf

  • Proc.

Barrow holographic dark energy

We formulate Barrow holographic dark energy, by applying the usual holographic principle at a cosmological framework, but using the Barrow entropy instead of the standard Bekenstein-Hawking one. The
...