Observational constraint on interacting Tsallis holographic dark energy in logarithmic Brans-Dicke theory

Abstract

In this paper, we investigate the dark energy phenomenon by studying the Tsallis holographic dark energy within the framework of Brans-Dicke (BD) scalar-tensor theory of gravity [Phys. Rev. \textbf{124}, 925 (1961)]. In this context, we choose the BD scalar field $\varphi$ as a logarithmic function of the average scale factor $a(t)$ and Hubble horizon as the IR cutoff ($L=H^{-1}$). We reconstruct two cases of non-interacting and interacting fluid (dark sectors of cosmos) scenario. The physical behavior of the models are discussed with the help of graphical representation to explore the accelerated expansion of the universe. Moreover, the stability of the models are checked through squared sound speed $v_s^2$. The well-known cosmological plane i.e., ${\omega }_{de}-{\omega }_{de}^{\prime }$ is constructed for our models. We also include comparison of our findings of these dynamical parameters with observational constraints. It is also quite interesting to mention here that the results of deceleration, equation of state parameters and ${\omega }_{de}-{\omega }_{de}^{\prime }$ plane coincide with the modern observational data.

arXiv comment12 pages, 15 figures

References in corpus (84)

• 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
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Modified Gravity and Cosmology
• The World as a Hologram
• Cosmological Imprint of an Energy Component with General Equation of State
• A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• Cosmology and the Fate of Dilatation Symmetry
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• An alternative to quintessence
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
• A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
• A Model of Holographic Dark Energy
• Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Dark Energy Constraints from the Cosmic Age and Supernova
• Properties of singularities in (phantom) dark energy universe
• Tachyon Matter
• Accelerated expansion of the universe driven by tachyonic matter
• Quantum deSitter cosmology and phantom matter
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
• Quintom Cosmology: Theoretical implications and observations
• Holographic dark energy and cosmic coincidence
• Black hole thermodynamical entropy
• The Physics of Cosmic Acceleration
• Infrared cut-off proposal for the Holographic density
• Role of Modified Chaplygin Gas in Accelerated Universe
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Tsallis Holographic Dark Energy
• Large Scale Structure as a Probe of Gravitational Slip
• Dark Energy Anisotropic Stress and Large Scale Structure Formation
• Generalized entropy formalism and a new holographic dark energy model
• Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models
• Modified gravity models of dark energy
• Holographic Chaplygin gas model
• Cosmic acceleration without quintessence
• From cosmic deceleration to acceleration: new constraints from SN Ia and BAO/CMB
• Thermodynamic approach to holographic dark energy and the Rényi entropy
• Interacting Holographic Phantom
• Holographic dark energy through Tsallis entropy
• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Modified cosmology from extended entropy with varying exponent
• Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
• Hamiltonian dynamics and Noether symmetries in Extended Gravity Cosmology
• Holographic explanation of wide-angle power correlation suppression in the Cosmic Microwave Background Radiation
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Holographic inflation
• Improved Constraints on the Acceleration History of the Universe and the Properties of the Dark Energy
• Interacting holographic dark energy
• Interacting holographic dark energy in Brans-Dicke theory
• Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
• Probing the cosmological viability of non-gaussian statistics
• Tsallis holographic dark energy in the Brans-Dicke cosmology
• A Note on Tsallis Holographic Dark Energy
• On the Dark Sector Interactions
• Interacting tachyon dark energy in non-flat universe
• Signature of the interaction between dark energy and dark matter in observations
• Revisiting Generalized Chaplygin Gas as a Unified Dark Matter and Dark Energy Model
• Cosmological constraints on a decomposed Chaplygin gas
• Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• The Abell Cluster A586 and the Detection of the Equivalence Principle
• Higher order corrections of the extended Chaplygin gas cosmology with varying $G$ and $\Lambda$
• Observing the clustering properties of galaxy clusters in dynamical dark-energy cosmologies
• Observational constraints on interacting Tsallis holographic dark energy models
• SO(1,1) dark energy model and the universe transition
• Tsallis holographic dark energy in the brane cosmology
• A model of interacting holographic dark energy at the Ricci's scale
• The universe dominated by the extended Chaplygin gas
• New holographic reconstruction of scalar field dark energy models in the framework of chameleon Brans-Dicke cosmology
• Observational Constraints to Ricci Dark Energy Model by Using: SN, BAO, OHD, fgas Data Sets
• Interacting Ghost Dark Energy Models with Variable $G$ and $\Lambda$
• Unified universe history through phantom extended Chaplygin gas
• New agegraphic dark energy in Brans-Dicke theory with logarithmic form of scalar field
• Interacting Holographic Extended Chaplygin Gas and Phantom Cosmology in the Light of BICEP2
• Phenomenological Varying Modified Chaplygin Gas with Variable $G$ and $\Lambda$: Toy Models for Our Universe
• A new holographic dark energy model in Brans-Dicke theory with logarithmic scalar field
• Thermodynamical description of the ghost dark energy model
• Limits on the parameters of the equation of state for interacting dark energy
• On detecting interactions in the dark sector with H(z) data

Cited by in corpus (16)

• Barrow holographic dark energy
• Accelerated Expansion of the Universe in Non-minimally Coupled Gravity
• Cosmography in $f(Q)$ gravity
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Power-law solution for homogeneous and isotropic universe in $f(R,T)$ gravity
• Imprints of Barrow-Tsallis Cosmology in Primordial Gravitational Waves
• Saez-Ballester gravity in Kantowski-Sachs Universe: a new reconstruction paradigm for Barrow Holographic Dark Energy
• Exploring the Sharma-Mittal HDE models with different diagnostic tools
• Accelerating bianchi type dark energy cosmological model with cosmic string in f(T) Gravity
• Note on Tsallis holographic dark energy in Brans-Dicke cosmology
• Tsallis Holographic Dark Energy Reconsidered
• Lagrangian reconstruction of Barrow holographic dark energy in interacting tachyon model
• Nonextensive entropies impact onto thermodynamics and phase structure of Kerr-Newman black holes
• Lagrangian formulation of the Tsallis entropy
• Diagnosing the R$\acute{e}$nyi Holographic Dark Energy model in a flat Universe
• Comparing teh holographic principle inspired dark energy models