Observational constraints on the dark energy and dark matter mutual coupling

Abstract

We examine different phenomenological interaction models for Dark Energy and Dark Matter by performing statistical joint analysis with observational data arising from the 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy Probe observations, the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey and age estimates of 35 galaxies. Including the time-dependent observable, we add sensitivity of measurement and give complementary results for the fitting. The compatibility among three different data sets seem to imply that the coupling between dark energy and dark matter is a small positive value, which satisfies the requirement to solve the coincidence problem and the second law of thermodynamics, being compatible with previous estimates.

9 pages, 4 figures, accepted for publication in Phys. Lett. B

References in corpus (44)

• The Cosmological Constant and Dark Energy
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmological Constant - the Weight of the Vacuum
• Coupled Quintessence
• New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
• Constraints on the redshift dependence of the dark energy potential
• Holographic dark energy and cosmic coincidence
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Interacting Quintessence
• Dark Matter and Dark Energy
• Interacting quintessence solution to the coincidence problem
• Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
• Is there Supernova Evidence for Dark Energy Metamorphosis ?
• Probing the Coupling between Dark Components of the Universe
• The case for dynamical dark energy revisited
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and Three-Year Wilkinson Microwave Anisotropy Probe Observations
• Stationary dark energy: the present universe as a global attractor
• Constraints on the interacting holographic dark energy model
• Super-acceleration as Signature of Dark Sector Interaction
• Cosmological parameters from supernova observations: A critical comparison of three data sets
• Tracking and coupled dark energy as seen by WMAP
• Dark Energy: the equation of state description versus scalar-tensor or modified gravity
• Observational constraints on interacting quintessence models
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data
• Testing the viability of the interacting holographic dark energy model by using combined observational constraints
• Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae
• Thermodynamical description of the interaction between holographic dark energy and dark matter
• Direct Determination of the Kinematics of the Universe and Properties of the Dark Energy as Functions of Redshift
• Matter density perturbations in interacting quintessence models
• Interacting models of soft coincidence
• Model independent analysis of dark energy I: Supernova fitting result
• Phantom damping of matter perturbations
• Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem
• Lookback time as a test for brane cosmology
• An old quasar in a young dark energy-dominated universe?
• Lookback time bounds from energy conditions
• Late Universe expansion dominated by domain walls and dissipative dark matter
• Soft coincidence in late acceleration
• Static Configurations of Dark Energy and Dark Matter
• Direct Detection Rates of Dark Matter Coupled to Dark Energy
• Dark Energy and Dark Matter in Galaxy Halos

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• Evidence for interacting dark energy from BOSS
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• Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
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• Constraining interacting dark energy with CMB and BAO future surveys
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• The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
• New agegraphic dark energy in Brans-Dicke theory with logarithmic form of scalar field
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• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Deep connection between f(R) gravity and the interacting dark sector model
• Dynamics of Interacting Generalized Cosmic Chaplygin gas in Brane-world scenario
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• A new holographic dark energy model in Brans-Dicke theory with logarithmic scalar field
• Constraining the interaction between dark sectors with future HI intensity mapping observations
• Interacting $F(R,T)$ gravity with modified Chaplygin gas
• Dark energy interacting with dark matter and unparticle
• Charged strange star coupled to anisotropic dark energy in Tolman-Kuchowicz spacetime
• Effective dark energy equation of state in interacting dark energy models
• The signature of the scattering between dark sectors in large scale cosmic microwave background anisotropies
• Ultra-compact structure in radio quasars as a cosmological probe: a revised study of the interaction between cosmic dark sectors
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• The generalized second law for the interacting new agegraphic dark energy in a non-flat FRW universe enclosed by the apparent horizon
• Dynamical behavior of interacting dark energy in loop quantum cosmology
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• Interacting Generalised Cosmic Chaplygin gas in Loop quantum cosmology: A singularity free universe
• New observational constraints on interacting dark energy using galaxy clusters virial equilibrium states
• An interacting holographic dark energy model within an induced gravity brane
• Entropy-corrected new agegraphic dark energy in Horava-Lifshitz cosmology
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• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia
• How effective is new variable modified Chaplygin gas to play the role of dark energy- A dynamical system analysis in RS II Brane model
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• Reconstruction of the interaction term between dark matter and dark energy using SNe Ia, BAO, CMB, H(z) and X-ray gas mass fraction
• Signature of the interaction between dark sectors in the reionization process
• Power Law and Logarithmic Ricci Dark Energy Models in Horava-Lifshitz Cosmology
• Charged analog of anisotropic dark energy star in Rastall gravity
• Baryon Acoustic Oscillations from Integrated Neutral Gas Observations: an instrument to observe the 21cm hydrogen line in the redshift range 0.13 $<$ z $<$ 0.45 -- status update
• Cosmological Equation of State and Interacting Energies
• Interacting dark fluid in the universe bounded by event horizon : A non-equilibrium prescription
• Cosmological Equations for Interacting Energies
• The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter