Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters

Abstract

Several observational constraints are imposed on the interacting holographic model of Dark Energy and Dark Matter. First we use the age parameter today, as given by the WMAP results. Subsequently, we explained the reason why it is possible, as recently observed, for an old quasar to be observed in early stages of the universe. We discuss this question in terms of the evolution of the age parameter as well as in terms of the structure formation. Finally, we give a detailed discussion of the constraints implied by the observed CMB low $\ell$ suppression. As a result, the interacting holographic model has been proved to be robust and with reasonable bounds predicts a non vanishing interaction of Dark Energy and Dark Matter.

20 pages, 9 figures

References in corpus (47)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• The World as a Hologram
• Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
• Cosmological Constant - the Weight of the Vacuum
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• A Model of Holographic Dark Energy
• Coupled Quintessence
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• Cosmic Growth History and Expansion History
• Holographic dark energy and cosmic coincidence
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology
• Dark Matter and Dark Energy
• Weak Gravitational Lensing by Large-Scale Structure
• The end of unified dark matter?
• The case for dynamical dark energy revisited
• Uncorrelated Estimates of Dark Energy Evolution
• Cosmic Structure Growth and Dark Energy
• Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models
• Constraints on the interacting holographic dark energy model
• Super-acceleration as Signature of Dark Sector Interaction
• Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
• CMB Observables and Their Cosmological Implications
• Likely Values of the Cosmological Constant
• Constraints on the Dark Energy from the holographic connection to the small l CMB Suppression
• Holographic explanation of wide-angle power correlation suppression in the Cosmic Microwave Background Radiation
• Constraints on the dark energy from holography
• Discovery of an ionized Fe-K edge in the z=3.91 Broad Absorption Line Quasar APM 08279+5255 with XMM-Newton
• Relating Friedmann equation to Cardy formula in universes with cosmological constant
• A CMB/Dark Energy Cosmic Duality
• Cosmological weak lensing with the HST GEMS survey
• The Age of the Universe and the Cosmological Constant Determined from Cosmic Microwave Background Anisotropy Measurements
• Interacting models of soft coincidence
• Searching for a holographic connection between dark energy and the low-l CMB multipoles
• An estimate of Ω_m without priors
• An old quasar in a young dark energy-dominated universe?
• Restframe I-band Hubble diagram for type Ia supernovae up to redshift z ~0.5
• CMB constraints on interacting cosmological models
• Cosmic acceleration in brane cosmology
• Soft coincidence in late acceleration
• Dark Energy and the Hubble Age
• Dark Energy: The Observational Challenge
• The Need of Dark Energy for Dynamical Compactification of Extra Dimensions on the Brane

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• Evolution of density perturbations in decaying vacuum cosmology: The case of non-zero perturbations in the cosmological term
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• Agegraphic Dark Energy Model in Non-Flat Universe: Statefinder Diagnostic and $w-w^{\prime }$ Analysis
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• Exact cosmological solutions of models with an interacting dark sector
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• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
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