A Generalized Interacting Tsallis Holographic Dark Energy Model and its thermodynamic implications

Abstract

The paper deals with a theoretical model for interacting Tsallis holographic dark energy (THDE) whose infrared (IR) cut-off scale is set by the Hubble length. The interaction $Q$ between the dark sectors (dark energy and pressureless dark matter) of the universe has been assumed to be non-gravitational in nature. The functional form of $Q$ is chosen in such a way that it reproduces well known and most used interactions as special cases. We then study the nature of the THDE density parameter, the equation of state parameter, the deceleration parameter and the jerk parameter for this interacting THDE model. Our study shows that the universe exhibits the usual thermal history, namely the successive sequence of radiation, dark matter and dark energy epochs, before resulting in a complete dark energy domination in the far future. It is shown the evolution of the Hubble parameter for our model and compared that with the latest Hubble parameter data. Finally, we also investigate both the stability and thermodynamic nature of this model in the present context.

arXiv commentv3: minor corrections, published in EPJC

References in corpus (93)

• 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
• Dynamics of dark energy
• The World as a Hologram
• Cosmological parameters from SDSS and WMAP
• Cosmological Constant - the Weight of the Vacuum
• Thermodynamics of Spacetime: The Einstein Equation of State
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• 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
• Coupled Quintessence
• Effective Field Theory, Black Holes, and the Cosmological Constant
• 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
• Entropy Bounds and Dark Energy
• Holographic dark energy and cosmic coincidence
• Black hole thermodynamical entropy
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Interacting quintessence solution to the coincidence problem
• Thermodynamic Behavior of Friedmann Equation at Apparent Horizon of FRW Universe
• f(T) Gravity and local Lorentz invariance
• Holographic Dark Energy
• Infrared cut-off proposal for the Holographic density
• The Holographic Dark Energy in a Non-flat Universe
• Cosmic Holography
• Large-scale instability in interacting dark energy and dark matter fluids
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Tsallis Holographic Dark Energy
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Dynamics of dark energy with a coupling to dark matter
• Dark energy and the generalized second law
• New infrared cut-off for the holographic scalar fields models of dark energy
• A kinematical approach to dark energy studies
• Interacting holographic dark energy model in non-flat universe
• Constraints on the interacting holographic dark energy model
• Dynamics of interacting dark energy
• Tracking and coupled dark energy as seen by WMAP
• Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
• Cosmology and the S-matrix
• Inflation and de Sitter Thermodynamics
• Le Chatelier-Braun principle in cosmological physics
• Thermodynamics of dark energy interacting with dark matter and radiation
• Interactions in Scalar Field Cosmology
• Covariant Generalized Holographic Dark Energy and Accelerating Universe
• Observational constraints on interacting quintessence models
• Holographic dark energy through Tsallis entropy
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression
• Dark Interactions and Cosmological Fine-Tuning
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Interacting holographic dark energy in Brans-Dicke theory
• Interacting holographic dark energy
• Constraints on the dark energy from holography
• Transplanckian energy production and slow roll inflation
• Holographic dark energy from nonadditive entropy: cosmological perturbations and observational constraints
• Generalized entropies and corresponding holographic dark energy models
• Testing the interaction between dark energy and dark matter via latest observations
• A parametric reconstruction of the deceleration parameter
• Probing the cosmological viability of non-gaussian statistics
• Implications, consequences and interpretations of generalized entropy in the cosmological setups
• Tsallis holographic dark energy in the Brans-Dicke cosmology
• A Note on Tsallis Holographic Dark Energy
• Signature of the interaction between dark energy and dark matter in observations
• Holographic Scalar Fields Models of Dark Energy
• The generalized second law of thermodynamics in Horava-Lifshitz cosmology
• Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology
• A divergence free parametrization of deceleration parameter for scalar field dark energy
• Holographic dark energy in the DGP braneworld with GO cutoff
• Cosmic slowing down of acceleration for several dark energy parametrizations
• Observational constraints on interacting Tsallis holographic dark energy models
• Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations
• Tsallis holographic dark energy in the brane cosmology
• Curvature constraints from Large Scale Structure
• Constraints on a generalized deceleration parameter from cosmic chronometers
• Tsallis Agegraphic Dark Energy Model
• Dynamics and cosmological evolution in Λ-varying cosmology
• Teleparallel Gravity: An Overview
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Non-singular models of universes in teleparallel theories
• Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
• Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
• Cosmic acceleration in non-canonical scalar field model - An interacting scenario
• Utility of observational Hubble parameter data on dark energy evolution
• Holographic dark energy with the sign-changeable interaction term
• A note on the Virasoro blocks at order $1/c$
• Thermodynamical description of the ghost dark energy model
• The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
• Interacting Tsallis holographic dark energy: Cosmic behaviour, statefinder analysis and ${\omega }_D-{\omega }_D^{\prime }$ pair in the non-flat universe
• A new parametrization for dark energy density and future deceleration

Cited by in corpus (10)

• Dynamics of an Interacting Barrow Holographic Dark Energy Model and its Thermodynamic Implications
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Barrow holographic dark energy in the Brans-Dicke cosmology
• Observational constraints of the modified cosmology through Barrow entropy
• Tsallis holographic dark energy for inflation
• Observational constraints on Tsallis modified gravity
• Generalized interacting Barrow Holographic Dark Energy: cosmological predictions and thermodynamic considerations
• Tsallis Holographic Dark Energy Reconsidered
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Rips and regular future scenario with Holographic Dark Energy: A comprehensive look