Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy

Abstract

We reconstruct Barrow Holographic Dark Energy (BHDE) within the framework of Saez-Ballester Scalar Tensor Theory. As a specific background, we consider a homogeneous and anisotropic Kantowski-Sachs Universe filled up with BHDE and dark matter. By assuming the Hubble radius as an IR cutoff, we investigate both the cases of non-interacting and interacting dark energy scenarios. We analyze the evolutionary behavior of various model parameters, such as skewness parameter, Equation-of-State parameter, deceleration parameter, jerk parameter and squared sound speed. We also draw the trajectories of ${\omega }_D-{\omega }_D^{\prime }$ phase plane and examine statefinder diagnosis. Observational consistency is discussed by inferring the current value of Hubble's parameter through the best fit curve of data points from Differential Age (DA) and Baryon Acoustic Oscillations (BAO) and commenting on cosmological perturbations and growth rate of matter fluctuations in BHDE. We show that our model satisfactorily retraces the history of the Universe, thus providing a potential candidate explanation for dark energy. Comparison with other reconstructions of BHDE is finally analyzed.

arXiv comment17 pages, 13 labeled figures, 3 tabs (accepted for publication in Physics of the Dark Universe)

References in corpus (83)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Planck 2013 results. XVI. Cosmological parameters
• Cosmological parameters from SDSS and WMAP
• Extended Theories of Gravity
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Hilbert Space Representation of the Minimal Length Uncertainty Relation
• 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
• Statefinder -- a new geometrical diagnostic of dark energy
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Generalized Uncertainty Principle in Quantum Gravity from Micro-Black Hole Gedanken Experiment
• Entropy Bounds and Dark Energy
• The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
• Holographic dark energy and cosmic coincidence
• Statistical mechanics in the context of special relativity
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• New physics in light of the $H_0$ tension: an alternative view
• Probable Values of the Cosmological Constant in a Holographic Theory
• The Area of a Rough Black Hole
• Holographic Dark Energy
• The Holographic Dark Energy in a Non-flat Universe
• Tsallis Holographic Dark Energy
• New infrared cut-off for the holographic scalar fields models of dark energy
• Constraints on the interacting holographic dark energy model
• Dynamics of interacting dark energy
• Holographic dark energy models: A comparison from the latest observational data
• Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts
• Local determination of the Hubble constant and the deceleration parameter
• QUANTUM FIELD THEORY OF FERMION MIXING
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• Covariant Generalized Holographic Dark Energy and Accelerating Universe
• Holographic dark energy through Tsallis entropy
• Modified cosmology from extended entropy with varying exponent
• Bulk-Brane Interaction and Holographic Dark Energy
• Probing cosmic isotropy with a new X-ray galaxy cluster sample through the $L_{\text{X}}-T$ scaling relation
• Barrow entropic dark energy: A member of generalized holographic dark energy family
• Measuring the Speed of Sound of Quintessence
• Big Bang Nucleosynthesis constraints on Barrow entropy
• Holographic inflation
• Kaniadakis holographic dark energy and cosmology
• Generalized entropies and corresponding holographic dark energy models
• Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
• Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory
• Tsallis holographic dark energy in the Brans-Dicke cosmology
• Barrow Entropy Corrections to Friedmann Equations
• Observational constraints on holographic dark energy with varying gravitational constant
• Nonsaturated Holographic Dark Energy
• Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
• Physical approximations for the nonlinear evolution of perturbations in dark energy scenarios
• Cosmological Constraints on the Sign-Changeable Interactions
• Holographic dark energy in the DGP braneworld with GO cutoff
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Cosmological Evolution of Interacting New Holographic Dark Energy in Non-flat Universe
• Brans-Dicke Theory as a Unified Model for Dark Matter - Dark Energy
• Phase structure of the massive chiral Gross-Neveu model from Hartree-Fock
• Geometrical observational bounds on a fractal horizon holographic dark energy
• Einstein, Planck and Vera Rubin: relevant encounters between the Cosmological and the Quantum Worlds
• Baryon asymmetry from Barrow entropy: theoretical predictions and observational constraints
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Cosmic evolution and thermal stability of Barrow holographic dark energy in nonflat Friedmann-Robertson-Walker Universe
• Growth of Perturbations in Tsallis and Barrow Cosmology
• Barrow holographic dark energy in the Brans-Dicke cosmology
• Baryogenesis in non-extensive Tsallis Cosmology
• Constraining Barrow entropy-based Cosmology with power-law inflation
• Hubble tension as a guide for refining the early Universe: Cosmologies with explicit local Lorentz and diffeomorphism violation
• Thermodynamic aspects of dark energy fluids
• Accelerating Bianchi Type-V Cosmology with Perfect Fluid and Heat Flow in Saez-Ballester Theory
• Quantum vacuum, dark matter, dark energy and spontaneous supersymmetry breaking
• Questioning the $H_0$ tension via the look-back time
• Late time cosmic acceleration in modified Sáez-Ballester theory
• Boson mixing and flavor vacuum in the expanding Universe: a possible candidate for the dark energy
• Precision Cosmology: Successes and Challenges
• Neutrino capture on tritium as a probe of flavor vacuum condensate and dark matter
• Modified Saez-Ballester scalar-tensor theory from 5D space-time
• $f(R)$ gravity and Tsallis holographic dark energy
• Tachyon model of Tsallis holographic dark energy
• On the flavor/mass dichotomy for mixed neutrinos: a phenomenologically motivated analysis based on lepton charge conservation in neutron decay
• Thermodynamic parametrization of dark energy

Cited by in corpus (15)

• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• The state of the dark energy equation of state circa 2023
• Observational Constraints and Cosmological Implications of Scalar-Tensor $f(R,T)$ Gravity
• Phase structure of charged AdS black holes surrounded by exotic fluid with modified Chaplygin equation of state
• A comprehensive numerical study on four categories of holographic dark energy models
• Barrow and Tsallis entropies after the DESI DR2 BAO data
• Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model
• Kaniadakis entropy in extreme gravitational and cosmological environments: a review on the state-of-the-art and future prospects
• Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data
• Quantum Entropy-Driven Modifications to Holographic Dark Energy in $f(G,T)$ Gravity
• Dark Universe inspired by the Kaluza-Klein gravity and impact on Primordial Gravitational Waves
• Holographic connection of f(G) gravity through Barrow and a generalized version of holographic dark fluid
• Cosmic Evolution of the Kantowski-Sachs Universe in the Context of a Bulk Viscous String in Teleparallel Gravity
• Hints Beyond $\Lambda$CDM from Barrow and Tsallis Holographic Dark Energy with GO cutoff
• Gravitational Foundations and Exact Solutions in $n$-Dimensional Fractional Cosmology