Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data

Abstract

We investigate phenomenological interactions between dark matter and dark energy and constrain these models by employing the most recent cosmological data including the cosmic microwave background radiation anisotropies from Planck 2015, Type Ia supernovae, baryon acoustic oscillations, the Hubble constant and redshift-space distortions. We find that the interaction in the dark sector parameterized as an energy transfer from dark matter to dark energy is strongly suppressed by the whole updated cosmological data. On the other hand, an interaction between dark sectors with the energy flow from dark energy to dark matter is proved in better agreement with the available cosmological observations. This coupling between dark sectors is needed to alleviate the coincidence problem.

22 pages, 8 figures, 11 tables. New figures added and discussion improved. Accepted in JCAP

References in corpus (9)

• A 2.4% Determination of the Local Value of the Hubble Constant
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Indications of a late-time interaction in the dark sector
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• Testing the interaction between dark energy and dark matter via latest observations
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
• Cosmological constraints on coupled dark energy

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• Dynamical dark energy versus $\Lambda =$const. in light of observations
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• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
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• Exploring neutrino mass and mass hierarchy in interacting dark energy models
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• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
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• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
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• The Dark Sector Cosmology
• Constraining interacting dark energy models with the halo concentration-mass relation
• The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models
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• Reconciling $S_8$: Insights from Interacting Dark Sectors
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• Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations
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