Kaniadakis holographic dark energy: observational constraints and global dynamics

Abstract

We investigate Kaniadakis-holographic dark energy by confronting it with observations. We perform a Markov Chain Monte Carlo analysis using cosmic chronometers, supernovae type Ia, and Baryon Acoustic Oscillations data. Concerning the Kaniadakis parameter, we find that it is constrained around zero, namely around the value in which Kaniadakis entropy recovers standard Bekenstein-Hawking one. Additionally, for the present matter density parameter ${\Omega }_m^{(0)}$, we obtain a value slightly smaller compared to $\Lambda$CDM scenario. Furthermore, we reconstruct the evolution of the Hubble, deceleration and jerk parameters extracting the deceleration-acceleration transition redshift as $z_T=0.86_{-0.14}^{+0.21}$. Finally, performing a detailed local and global dynamical system analysis, we find that the past attractor of the Universe is the matter-dominated solution, while the late-time stable solution is the dark-energy-dominated one.

Version accepted in MNRAS

References in corpus (81)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• emcee: The MCMC Hammer
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Dynamics of dark energy
• The World as a Hologram
• Extended Theories of Gravity
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• A Model of Holographic Dark Energy
• f(T) teleparallel gravity and cosmology
• Exponential potentials and cosmological scaling solutions
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Brane-World Gravity
• Quintom Cosmology: Theoretical implications and observations
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• Holographic dark energy and cosmic coincidence
• Einstein-Gauss-Bonnet gravity in 4-dimensional space-time
• Statistical mechanics in the context of special relativity
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• A Dark Energy Model Characterized by the Age of the Universe
• Structure formation with a self-tuning scalar field
• Cosmology Intertwined II: The Hubble Constant Tension
• Holographic Dark Energy
• Constraints on holographic dark energy from type Ia supernova observations
• Statistical mechanics in the context of special relativity II
• On the Hubble constant tension in the SNe Ia Pantheon sample
• Barrow holographic dark energy
• To H0 or not to H0?
• Holographic dark energy models: A comparison from the latest observational data
• Modified Gravity and Cosmology: An Update by the CANTATA Network
• STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
• Sounds Discordant: Classical Distance Ladder & $\Lambda$CDM -based Determinations of the Cosmological Sound Horizon
• Extended Holographic dark energy
• Covariant Generalized Holographic Dark Energy and Accelerating Universe
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Holography and Variable Cosmological Constant
• Equation of state for an interacting holographic dark energy model
• Holographic dark energy through Tsallis entropy
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Restoring Holographic Dark Energy in Brane Cosmology
• The Cardassian expansion revisited: constraints from updated Hubble parameter measurements and Type Ia Supernovae data
• The generalized second law of thermodynamics with Barrow entropy
• Generalized entropies and corresponding holographic dark energy models
• Correspondence between Holographic and Gauss-Bonnet dark energy models
• Phase-space analysis of interacting phantom cosmology
• Observational constraints on holographic dark energy with varying gravitational constant
• Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
• Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
• Cosmological parameter analyses using transversal BAO data
• TDCOSMO V: strategies for precise and accurate measurements of the Hubble constant with strong lensing
• Observational constraints on holographic tachyonic dark energy in interaction with dark matter
• Holographic Dark Energy in Braneworld Models with Moving Branes and the w=-1 Crossing
• Ricci-Gauss-Bonnet holographic dark energy
• Geometrical observational bounds on a fractal horizon holographic dark energy
• Testing Low-Redshift Cosmic Acceleration with Large-Scale Structure
• Cosmological constraints on alternative model to Chaplygin fluid revisited
• A Critique of Holographic Dark Energy
• Observational constraints on the interacting Ricci dark energy model
• Generalized Emergent Dark Energy: observational Hubble data constraints and stability analysis
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Tsallis and Kaniadakis statistics from a point of view of the holographic equipartition law
• The cosmology of an holographic induced gravity model with curvature effects
• Accelerated and decelerated expansion in a causal dissipative cosmology
• Jeans instability criterion from the viewpoint of non-gaussian statistics
• Cosmic acceleration in unimodular gravity
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• Brane with variable tension as a possible solution to the problem of the late cosmic acceleration
• Energy exchange for homogeneous and isotropic universes with a scalar field coupled to matter
• Interacting quintessence dark energy models in Lyra manifold
• Constraints and cosmography of $\Lambda$CDM in presence of viscosity
• The generalized Chaplygin-Jacobi gas
• Growth Rate and Configurational Entropy in Tsallis Holographic Dark Energy
• Stability analysis and constraints on interacting viscous cosmology
• Cosmological test on viscous bulk models using Hubble Parameter measurements and type Ia Supernovae data
• Flat limits of curved interacting cosmic fluids
• Constraining a causal dissipative cosmological model
• An effective field theory of holographic dark energy