Comparing teh holographic principle inspired dark energy models
arXiv:2003.02579 · doi:10.1016/j.newast.2021.101586
Abstract
In this work, we use the statefinder parameter diagnostic to the Holographic principal inspired dark energy models, taking into consideration, the Tsallis Holographic dark energy (THDE) model, the standard Holographic dark energy (HDE) model, and the Rnyi holographic dark energy (RHDE) model. The evolutionary behaviour of first statefinder , second statefinder parameter , the statefinder parameter pairs and as well as the deceleration parameter are plotted for comparison for the various parameter values of the respective dark energy models. In the low redshift region, it is observed from these plots that the Tsallis holographic dark energy (THDE) model and Rnyi holographic dark energy (RHDE) model approach to the CDM model. While for the HDE model, the evolutionary behaviour can be differentiated from the CDM model in the low-redshift region. For all three dark energy models, a direct comparison in , , , and plane have also been done, in which the discrimination between these three models wif the CDM model) may be easily seen.
arXiv comment10 pages, 10 figures
References in corpus (69)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- The World as a Hologram
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- The Cosmological Constant
- An alternative to quintessence
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Phantom Energy and Cosmic Doomsday
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- A Model of Holographic Dark Energy
- Essentials of k-essence
- Statefinder -- a new geometrical diagnostic of dark energy
- Effective Field Theory, Black Holes, and the Cosmological Constant
- MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
- Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
- Entropy Bounds and Dark Energy
- A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
- The large-scale structure of the Universe
- Black hole thermodynamical entropy
- Probable Values of the Cosmological Constant in a Holographic Theory
- The Area of a Rough Black Hole
- Tsallis Holographic Dark Energy
- Universality of the Tachyon Potential
- Dark Energy and Gravity
- Generalized entropy formalism and a new holographic dark energy model
- Statefinder diagnostic for holographic dark energy model
- Tracking K-essence
- The new form of the equation of state for dark energy fluid and accelerating universe
- A step beyond Tsallis and Renyi entropies
- Thermodynamic approach to holographic dark energy and the Rényi entropy
- Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
- Holographic dark energy through Tsallis entropy
- Modified cosmology from extended entropy with varying exponent
- Modified Friedmann Equations from Tsallis Entropy
- Statefinder Diagnosis for Ricci Dark Energy
- Cosmological model from the holographic equipartition law with a modified Rényi entropy
- Accelerated cosmos in a non-extensive setup
- Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
- An improved model-independent assessment of the late-time cosmic expansion
- Probing the cosmological viability of non-gaussian statistics
- Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory
- Implications, consequences and interpretations of generalized entropy in the cosmological setups
- A Note on Tsallis Holographic Dark Energy
- Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
- Future CMB Constraints on Early, Cold, or Stressed Dark Energy
- Implications of the Generalized Entropy Formalisms on the Newtonian Gravity and Dynamics
- Dark energy and the Boomerang data
- Observational constraints on interacting Tsallis holographic dark energy models
- Making Sense Of The New Cosmology
- Tsallis holographic dark energy in the brane cosmology
- The generalized and extended uncertainty principles and their implications on the Jeans mass
- Dark energy beyond quintessence: Constraints from the swampland
- Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
- Stability analysis of the Tsallis holographic dark energy model
- Statefinder diagnostic for the modified polytropic Cardassian universe
- The extended uncertainty principle inspires the Rényi entropy
- Exploring the evidence for a large local void with supernovae Ia data
- Tsallis holographic dark energy in Fractal Universe
- Inflation in the Rényi cosmology
- Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
- Dark energy models toward observational tests and data
- Comparing holographic dark energy models with statefinder
- Tsallis holographic model of dark energy: Cosmic behaviour, statefinder analysis and pair in the non-flat universe
- Interacting Tsallis holographic dark energy: Cosmic behaviour, statefinder analysis and pair in the non-flat universe
- Cosmological constraints from low-redshift data
- Interacting Rényi holographic dark energy with parametrization on the interaction term