Dark Energy Constraints from the Cosmic Age and Supernova

Abstract

Using the low limit of cosmic ages from globular cluster and the white dwarfs: $t_0>12$Gyr, together with recent new high redshift supernova observations from the HST/GOODS program and previous supernova data, we give a considerable estimation of the equation of state for dark energy, with uniform priors as weak as $0.2<{\Omega }_m<0.4$ or $0.1<{\Omega }_m{h}^2<0.16$. We find cosmic age limit plays a significant role in lowering the upper bound on the variation amplitude of dark energy equation of state. We propose in this paper a new scenario of dark energy dubbed Quintom, which gives rise to the equation of state larger than -1 in the past and less than -1 today, satisfying current observations. In addition we've also considered the implications of recent X-ray gas mass fraction data on dark energy, which favors a negative running of the equation of state.

References added; Version to appear in Physics Letters B

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• Modified Holographic Dark Energy in Non-flat Kaluza-Klein Universe with Varying G
• Phenomenological Varying Modified Chaplygin Gas with Variable $G$ and $\Lambda$: Toy Models for Our Universe
• Cosmological Evolution Across Phantom Crossing and the Nature of the Horizon
• Compatibility between the scalar field models of tachyon, $k$-essence and quintessence in $f(R,T)$ gravity
• Perturbations in a scalar field model with virtues of $\Lambda$CDM
• Phenomenological Fluids from Interacting Tachyonic Scalar Fields
• Quintom evolution in power-law potentials
• Cosmic Dynamics in $F(R,\varphi )$ Gravity
• Quintessence and phantom dark energy from ghost D-branes
• High-resolution temporal constraints on the dynamics of dark energy
• Holographic kinetic k-essence model
• Notes on interacting holographic dark energy model in a closed universe
• Reconstruction of an Observationally Constrained $f(R,T)$ gravity model
• Generating scale-invariant tensor perturbations in the non-inflationary universe
• Accelerating Dark Energy Cosmological Model in Two Fluid with Hybrid Scale Factor
• Reconstruction of scalar potentials in two-field cosmological models
• A new extended quintessence
• Testing the (generalized) Chaplygin gas model with the Lookback time-Redshift data
• The dynamics of matter bounce cosmology in Weyl-type $f(Q,T)$ gravity
• Spherical collapse in the extended quintessence cosmological models
• Comparing holographic dark energy models with statefinder
• Fixed points and FLRW cosmologies: Flat case
• A more general interacting model of holographic dark energy
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmology with variable parameters and effective equation of state for Dark Energy
• Can the initial singularity be detected by cosmological tests?
• A Unified Model of Phantom Energy and Dark Matter
• Curvature Inspired Cosmological Scenario
• Parametrization of dark energy equation of state Revisited
• Statefinder diagnosis for the extended holographic Ricci dark energy model without and with interaction
• Thermodynamics of Spinor Quintom
• Coupled Multi Scalar Field Dark Energy
• Constraints on accelerating universe using ESSENCE and Gold supernovae data combined with other cosmological probes
• Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects
• Parametrization of K-essence and Its Kinetic Term
• Probing dynamics of dark energy with latest observations
• Geometrical Diagnostics for Generalized Chaplygin Gas
• Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime
• Asymptotic behavior of w in general quintom model
• Equivalence of $f(Q)$ cosmology with quintom-like scenario: the phantom field as effective realization of the non-trivial connection
• Networks of cosmological histories, crossing of the phantom divide line and potentials with cusps
• Observational constraints on a generalized equation of state model
• Testing the interaction model with cosmological data and gamma-ray bursts
• Constraining the dark energy and smoothness-parameter with supernovae
• Transient Crossing of Phantom divide line $w_{\Lambda }=-1$ under Gauss-Bonnet interaction
• Testing Oscillating Primordial Spectrum and Oscillating Dark Energy with Astronomical Observations
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Key drivers of the preference for dynamic dark energy
• Robust evidence for dynamical dark energy in light of DESI DR2 and joint ACT, SPT, and Planck data
• Self-interacting holographic dark energy
• Planck-PR4 anisotropy spectra show (better) consistency with General Relativity
• Cosmological aspects of $f(R,T)$ gravity in a simple model with a parametrization of $q$
• Dark Energy, Scalar-Tensor Gravity and Large Extra Dimensions
• $w_d=-1$ in interacting quintessence model
• Does accelerating universe indicates Brans-Dicke theory
• Stability of Closed Timelike Curves in a Galileon Model
• Reduced modified Chaplygin gas cosmology
• A stable flat universe with variable Cosmological constant in f(R,T) Gravity
• Nonlinear Spinor field in isotropic space-time and dark energy models
• Inflessence: a phenomenological model for inflationary quintessence
• The general property of dynamical quintessence field
• Age Problem in Lemaitre-Tolman-Bondi Void Models
• Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models
• Crossing the phantom divide with Ricci-like holographic dark energy
• Constraints on Quintessence From Using Cosmological Data
• Interaction of divergence-free deceleration parameter in Weyl-type $f(Q,T)$ gravity
• Linear Perturbation constraints on Multi-coupled Dark Energy
• On Energy Conditions and Stability in Effective Loop Quantum Cosmology
• Can the Big Bang Singularity be avoided by a single scalar field?
• Cosmological Implications of 5-dimensional Brans-Dicke Theory
• Latest data constraint of some parameterized dark energy models
• Cosmological constraints on the generalized holographic dark energy
• Noether gauge symmetry approach in quintom cosmology
• Holographic Dark Energy Model and Scalar-Tensor Theories
• Reconstructing the properties of dark energy from recent observations
• Dark energy, curvature, and cosmic coincidence
• Phantom universe from CPT symmetric QFT
• Statefinder hierarchy exploration of the extended Ricci dark energy
• Cosmological constraints on polytropic gas model
• Scalar Field Reconstruction of Power-Law Entropy-Corrected HDE
• Null Energy Condition and Dark Energy Models
• Phantom crossing dark energy in Horndeski's theory
• Power-law entropy-corrected HDE and NADE in Brans-Dicke cosmology
• Bouncing Universe with Non-minimally Coupled Quintom Matter
• Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
• Modified holographic Ricci dark energy model and statefinder diagnosis in flat universe
• Differentiating dark interactions with perturbation
• A Two-field Dilaton Model of Dark Energy
• Chameleon Cosmology Model Describing the Phantom Divide Line Crossing
• Observational constraints on unified dark matter including Hubble parameter data
• Crossing the phantom divide line in the Holographic dark energy model in a closed universe
• Reconstructing Dark Energy Potentials From Parameterized Deceleration Parameters
• Uncertainty on determining the dark energy equation of state due to the spatial curvature
• Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model
• New mechanism to cross the phantom divide
• Accelerating Hilbert-Einstein universe without dynamic dark energy
• Cosmological neutrino mass limit and the dynamics of dark energy
• Analytic Solutions and Observational support: A study of $f(R,T)$ gravity with $f(R,T)=R+h(T)$
• Improved cosmological constraints on the curvature and equation of state of dark energy
• Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
• Dark Energy and Neutrino CPT Violation
• Probing the origin of our universe through primordial gravitational waves by Ali CMB project
• Cosmological Evolution of Pilgrim Dark Energy
• Cosmological Constraints on the DGP braneworld model with Gamma-ray bursts
• Statefinder parameters for quantum effective Yang-Mills condensate dark energy model
• Interacting entropy-corrected holographic Chaplygin gas model
• Inflation and the cosmological (not-so) constant in unimodular gravity
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• The Most Probable Size of the Universe
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• De-Sitter nonlinear sigma model and accelerating universe
• Density perturbation in an interacting holographic dark energy model
• Crossing the Phantom divide line in the Chaplygin gas model
• The Reactor Anomaly after Daya Bay and RENO
• Constraints on Dark Energy Models Using Late Universe Probes
• Parametrizations of Dark Energy Models in the Background of General Non-canonical Scalar Field in $D$-dimensional Fractal Universe
• Interacting Viscous Dark Energy in Bianchi Type-I Universe
• Dynamics of interacting scalar field model in the realm of chiral cosmology
• Phantom Behavior Bounce with Tachyon and Non-minimal Derivative Coupling
• Cosmological constraints on holographic dark energy models under the energy conditions
• Dynamical description of a quintom cosmological model nonminimally coupled with gravity
• The effects on CMB power spectra and bispectra from the polarization rotation and its correlations with temperature and E-polarization
• A General Model for Dark Energy Crossing the Phantom Divide
• Unification of cosmological scalar fields
• Interacting Ghost Dark Energy in Complex Quintessence Theory
• Generic Phase Portrait Analysis of the Finite-time Singularities and Generalized Teleparallel Gravity
• The Integrated Sachs-Wolfe Effect in Time Varying Vacuum Model
• Galileons, phantom fields, and the fate of the Universe
• Non-minimally coupled gravity constraints from DESI DR2 data
• K-essence and kinetic gravity braiding models in two-field measure theory
• Configurational Entropy and braneworlds in f(T,B) gravity
• Holographic dark energy with time depend gravitational constant in the non-flat Ho$\check{r}$ava-Lifshitz cosmology
• Probing Dark Energy with the Kunlun Dark Universe Survey Telescope
• Constructions of $f(R,G,\mathcal{T})$ Gravity from Some Expansions of the Universe
• Quintom fields from chiral K-essence cosmology
• Quintom potentials from quantum cosmology using the FRW cosmological model
• Statefinder Parameter for Varying G in Three Fluid System
• Interacting new agegraphic Phantom model of dark energy in non-flat universe
• Perturbative stability of SFT-based cosmological models
• Neutrino generated dynamical dark energy with no dark energy field
• Statefinder diagnostic of logarithmic entropy corrected holographic dark energy with Granda-Oliveros IR cut-off
• Detecting dark energy in long baseline neutrino oscillations
• Holographic Dark Energy Interacting with Two Fluids and Validity of Generalized Second Law of Thermodynamics
• Bouncing behavior in $f(R,L_m)$ gravity: Phantom crossing and energy conditions
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: constraints on the time variation of fundamental constants from the large-scale two-point correlation function
• Stable phantom-divide crossing in two scalar models with matter
• Cosmic acceleration and phantom crossing in $f(T)$-gravity
• Figure of Merit and Different Combinations of Observational Data Sets
• Modelling Tachyon Cosmology with Non-Minimal Derivative Coupling to Gravity
• Combining Optical and X-ray Observations of Galaxy Clusters to Constrain Cosmological Parameters
• Dark Energy Perturbations Revisited
• Noether Symmetry Approach in "Cosmic Triad" Vector Field Scenario
• Holographic dilatonic model of dark energy
• Gravitational Coupling and Dynamical Reduction of The Cosmological Constant
• Fractional Einstein-Gauss-Bonnet scalar field cosmology
• Phantom without phantom or how the PT symmetry saves us from the Big Rip
• Smooth crossing of $w_{\Lambda }=-1$ line in a single scalar field model
• Cosmological Model of Interacting Tachyon Field
• Perturbations of the Yang-Mills field in the universe
• Two-Fluid Viscous Modified Gravity on a RS Brane
• Cosmological evolution of a statistical system of degenerate scalar-charged fermions with an asymmetric scalar doublet. I. Two-component system of assorted charges
• Modified holographic Ricci dark energy coupled to interacting relativistic and non-relativistic dark matter in the nonflat universe
• Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
• Direct reconstruction of dynamical dark energy from observational Hubble parameter data
• Non-singular Cyclic Cosmology without Phantom Menace
• Chameleon mechanism with a new potential
• Interacting holographic tachyon model of dark energy
• Tsallis holographic dark energy under Complex form of Quintessence model
• Remarks on generalized scalar-tensor models of dark energy
• Tachyon model of Tsallis holographic dark energy
• Is dark energy from cosmic Hawking radiation?
• First-order formalism for the quintom model of dark energy
• Evolution of magnetic component in Yang-Mills condensate dark energy models
• Form invariant transformations between n-- and m-- dimensional flat Friedmann--Robertson--Walker cosmologies
• Phantom fields: bounce solutions in the early Universe and S-branes
• The accelerated scaling attractor solution of the interacting agegraphic dark energy in Brans-Dicke theory
• Dynamical dark energy in light of cosmic distance measurements II: a study using current observations
• A Universe with a generalized ghost dark energy and Van der Waals fluid interacting with a fluid
• DGP Cosmological model with generalized Ricci dark energy
• Perturbed dark energy: classical scalar field versus tachyon
• Comments on Scalar-Tensor Representation of $f(R)$ Theories
• Dynamics of Brans-Dicke cosmology with varying mass fermions
• Higher Order Lagrangians inspired by the Pais-Uhlenbeck Oscillator and their cosmological applications
• Study of Some Parameters of Modified Chaplygin Gas in Galileon Gravity Theory from Observational Perspective
• Effect of low anisotropy on cosmological models by using supernova data
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Quintessence models with an oscillating equation of state and their potentials
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
• Deformation of the quintom cosmological model and its consequences
• Cosmology In Terms Of The Deceleration Parameter. Part II
• Reconstruction of the equation of state for the cyclic universes in homogeneous and isotropic cosmology
• A holographic cut-off inspired in the apparent horizon
• Thermodynamics in Kaluza-Klein Universe
• Quantum induced w = -1 crossing of the quintessence and phantom models
• Braneworld cosmology in the sourced-Taub background
• Transition between phantom and non-phantom phases with time dependent cosmological constant and Cardy-Verlinde formula
• Cosmological Constraints on the Phenomenological Interacting Dark Energy Model with Fermi Gamma-Ray Bursts and DESI DR2
• Two-field cosmological models and large-scale cosmic magnetic fields
• Hybrid Chaplygin gas and phantom divide crossing
• Probing Ricci dark energy model with perturbations by using WMAP seven-year cosmic microwave background measurements, BAO and Type Ia supernovae
• Reconstructing quintom from WMAP 5-year observations: Generalized ghost condensate
• Quintom wormholes
• Phantom energy from graded algebras
• Stability of the holographic description of the Universe
• Phantom of the Hartle-Hawking instanton: connecting inflation with dark energy
• Null energy condition violation and beyond Horndeski physics in light of DESI DR2 data
• Are we seeing the beginnings of Inflation?
• Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
• Time variable cosmological constant of holographic origin with interaction in Brans-Dicke theory
• Scalar Dark Energy Models and Scalar-Tensor Gravity: Theoretical Explanations for the Accelerated Expansion of Present Universe
• Metric-Affine Formalism of Higher Derivative Scalar Fields in Cosmology
• Constraints on dark energy from the CSST galaxy clusters
• "Expansion" around the vacuum: how far can we go from Lambda?
• On Dark Energy Isocurvature Perturbation
• Cosmological observations in non-local $F(R)$ cosmology
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Constraining the Lattice Fluid Dark Energy from SNe Ia, BAO and OHD
• Phantom Divide Crossing with General Non-minimal Kinetic Coupling
• Probing for cosmological parameters with LAMOST measurement
• Constraining Slow-Roll Inflation in the Presence of Dynamical Dark Energy
• An Interacting Scenario for Dark Energy in Bianchi Type-I Universe
• Equilibrium sets in quintom cosmologies: the past asymptotic dynamics
• Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
• Quintessence and phantom emerging from the split-complex field and the split-quaternion field
• Friedmann-Robertson-Walker Models with Late-Time Acceleration
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Crossing of the Cosmological Constant Boundary - an Equation of State Description
• Investigation of Bouncing Universe and Phantom Crossing in Modified Gravity Coupled with Weyl Tensor and its Reconstruction
• Symmetry analysis and exact solutions of modified Brans-Dicke cosmological equations
• Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
• Dark Energy from Ratio Gravity
• Cosmological consequences of a scalar field with oscillating equation of state. IV. Primordial nucleosynthesis and the deuterium problem
• Cosmic Steps in Modeling Dark Energy
• Black Holes in Accelerated Universe
• Dynamics of holographic dark energy with apparent-horizon cutoff and non-minimal derivative coupling gravity in non-flat FLRW universe
• Crossing the phantom divide with a classical Dirac field
• How Much NEC Breaking Can the Universe Endure?
• Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
• Modelling Cosmic Acceleration in Modified Yang - Mills Theory
• Joint constraint on primordial gravitational waves and polarization rotation angle with current CMB polarization data
• Quintom fields from chiral anisotropic cosmology
• Impact of dark energy on the equation of state in light of the latest cosmological data
• A scalar field dark matter model and its role in the large scale structure formation in the Universe
• Fine Tuning Problem of the Cosmological Constant in a Generalized Randall-Sundrum Model
• Interacting Viscous Dark Energy in Bianchi Type-III Universe
• Constraints on Dark Energy from New Observations including Pan-STARRS
• Evidence for the dynamical dark energy with evolving Hubble constant
• Exponential quintessence with momentum coupling to dark matter
• Unified dark fluid with null sound speed as an alternative to phantom dark energy
• Confinement of exotic matter. I. Static solutions
• The torsion cosmology in Kaluza-Klein theory
• Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
• Constraining Dynamical Dark Energy Models through the Abundance of High-Redshift Supermassive Black Holes
• Non-Minimal Cosmological Model in Modified Yang--Mills Theory
• Equation of state description of the dark energy transition between quintessence and phantom regimes
• Considering Late-Time Acceleration in some Cosmological Models
• Latest Cosmological Constraints on Cardassian expansion models including the updated Gamma-ray bursts
• Generalized Ghost Pilgrim Dark Energy Fractal Cosmology with Observational Constraint
• Accelerating Universe: Observational Status and Theoretical Implications
• Realizing the phantom-divide crossing with vector and scalar fields
• Observational constraints on a Yang-Mills condensate dark energy model
• Lee Wick Dark Energy
• Comparison of Supernovae datasets Constraints on Dark Energy
• Inflation is the generic feature of phantom field-not the big-rip
• Causal horizons in a bouncing universe
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Holographic Ricci dark energy and generalized second law
• Spinor quintom cosmology with intrinsic spin
• $f(R)$ Gravity and Crossing the Phantom Divide Barrier
• Cosmological singularities in non-canonical models of dark energy
• A unification of RDE model and XCDM model
• The Effects of Tachyonic and Phantom Fields in the Intermediate and Logamediate Scenarios of the Anisotropic Universe
• Reconstruction of 5D Cosmological Model From Recent Observations
• Behavior of $F(R)$ gravity around a crossing of the phantom divide
• Quantum Yang-Mills Condensate Dark Energy Models
• Phenomenologically varying $\Lambda$ and a toy model for the Universe
• A short review on Quintom dark energy theory
• Confronting dark energy in Harada's Conformal Killing Gravity with observational data
• Qualitative behaviour of higher-curvature gravity with boundary terms i.e the f(Q) gravity models by dynamical system analysis
• Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation
• Dynamical System Analysis of Randall-Sundrum Model with Tachyon Field on the Brane
• Dynamics of the universe as a "test 3-brane" in a 5D bulk
• Cosmological LTB Black Hole in a Quintom Universe
• Exact solution and exotic fluid in cosmology
• Bouncing Universe with exotic radiation
• ${\mathbf{\Omega }}_1{\mathbf{\Omega }}_2$-$\mathbf{\Lambda }$CDM: A promising phenomenological extension of the standard model of cosmology
• Dark energy from conformal symmetry breaking
• Thermodynamics and holography of tachyon cosmology
• Interaction between Tachyon and Hessence (or Hantom) dark energies
• The Stability Analysis of Brane Induced Gravity with Quintessence Field on the Brane with a Gaussian Potential
• Weak Gravity Conjecture and Holographic Dark Energy Model with Interaction and Spatial Curvature
• Spatially open Friedmann--Robertson--Walker Universe fueled with interacting sources
• Tackling tangledness of cosmic strings by knot polynomial topological invariants
• A new single-dynamical-scalar-field model of dark energy
• Cosmological Equation of State and Interacting Energies
• Red-shift parametrizations of dark energy and observational constraint on their parameters: Galileon gravity as background
• Slow Burgers Vortices in Hot Conformal Fluids
• Reconstructing cosmic evolution with a density parametrization
• Polarization exchange in colliding photon beams in a medium of an atomic gas
• Crossing the phantom divide with k-essence in brane-worlds
• Reconstructing f(R) model from Holographic DE: Using the observational evidence
• Cosmic Acceleration Data and Bulk-Brane Energy Exchange
• Statefinder Description in Generalized Holographic and Ricci Dark Energy Models
• Gravity and induced matter on Nearly Kahler Manifolds
• Evolution of the horizons for dark energy universe
• Quintom phase-space: beyond the exponential potential
• Dark Energy Simulations
• Cosmic Acceleration Caused by the Extra-Dimensional Evolution in a Generalized Randall-Sundrum Model
• Constraints on a scalar-tensor model with Gauss-Bonnet coupling from SN Ia and BAO observations
• Acceleration of the universe in matter dominant era by conformal symmetry breaking
• Phase space of multi-fluid universe in $F(T)$-gravity and some enhancements for the oscillating interaction model
• Expanding Universe: Thermodynamical Aspects From Different Models
• UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
• Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
• Singularities in and Stability of Ooguri-Vafa-Verlinde Cosmologies
• Can hyperbolic phase of Brans-Dicke field account for Dark Matter?
• Parameterization and Reconstruction of Quasi Static Universe
• Scalar field in cosmology: Potential for isotropization and inflation
• A new approach to modified-gravity models
• Results from Hubble parameter data: oscillating dark energy?
• Agegraphic dark energy from entropy of the anti-de Sitter black hole
• Apparent $w<-1$ and a Lower $S_8$ from Dark Axion and Dark Baryons Interactions
• The influence of cosmological constant on light deflection in rotating spacetimes via the generalized Gibbons-Werner method
• Testing the Anton-Schmidt dark energy model with the DESI DR2 measurements
• Perturbations and stability conditions of k-essence and kinetic gravity braiding models in two-field measure theory
• Reconstructing the Equation of State for Dark Energy In the Double Complex Symmetric Gravitational Theory
• Perturbations In Some Dark Energy Models
• Towards a de Sitter quintom-like cosmology from a reduction of a 7-dimensional $BF$ theory
• Solution to the problem of time
• Phantom Crossing with Quintom Models
• Quintessence reconstruction of interacting HDE in a non-flat universe
• The relation between Geometry and Matter in classical and quantum Gravity and Cosmology
• Noether symmetry of FRW cosmology with f - essence
• Evolution and thermodynamics of new holographic dark energy with bulk viscosity in modified $f(R,T)$ gravity
• Non-singular Bouncing Cosmology in $f(R,G,T)$--Quintom model
• Thermodynamics properties of the dark energy in loop quantum cosmology
• Cosmological Model of Interacting Phantom and Yang-Mills Fields
• Evolution of entropic dark energy and its phantom nature
• Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
• Power-law and Logarithmic Entropy Corrected Holographic Dark Energy Models in Brans-Dicke Cosmology with Granda-Oliveros Cut-Off