Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
arXiv:1605.05264 · doi:10.1088/1475-7516/2016/12/009
Abstract
Large-scale structure has been shown as a promising cosmic probe for distinguishing and constraining dark energy models. Using the growth index parametrization, we obtain an analytic formula for the growth rate of structures in a coupled dark energy model in which the exchange of energy-momentum is proportional to the dark energy density. We find that the evolution of can be determined analytically once we know the coupling, the dark energy equation of state, the present value of the dark energy density parameter and the current mean amplitude of dark matter fluctuations. After correcting the growth function for the correspondence with the velocity field through the continuity equation in the interacting model, we use our analytic result to compare the model's predictions with large-scale structure observations.
26 pages. (v2) Added a correction term to the growth function, due to the interaction, in order to enable comparison with the observational data. (v3) Minor changes
References in corpus (21)
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Cosmology and Fundamental Physics with the Euclid Satellite
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Large-scale instability in interacting dark energy and dark matter fluids
- Effects of the interaction between dark energy and dark matter on cosmological parameters
- Stability of the curvature perturbation in dark sectors' mutual interacting models
- Signature of the interaction between dark energy and dark matter in galaxy clusters
- J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey
- Testing the interaction between dark energy and dark matter via latest observations
- Interacting models of soft coincidence
- Growth rate of cosmological perturbations at z ~ 0.1 from a new observational test
- Growth factor parametrization and modified gravity
- On the large-scale instability in interacting dark energy and dark matter fluids
- The growth of matter perturbations in some scalar-tensor DE models
- Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
- Growth factor parametrization in curved space
- BINGO: a single dish approach to 21cm intensity mapping
- Prospects for dark matter detection with IceCube in the context of the CMSSM
- BINGO - A novel method to detect BAOs using a total-power radio telescope
- Exploring a new interaction between dark matter and dark energy using the growth rate of structure
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- Tale of stable interacting dark energy, observational signatures, and the tension
- Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
- Listening to the sound of dark sector interactions with gravitational wave standard sirens
- Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
- Observational constraints on dark matter-dark energy scattering cross section
- On structure formation from a small-scales-interacting dark sector
- Constraining interacting dark energy with CMB and BAO future surveys
- Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
- J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
- Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
- Fractional Dark Matter decay: cosmological imprints and observational constraints
- Metastable dark energy
- The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
- Fractional dark energy
- Growth of structure in interacting vacuum cosmologies
- CMB and matter power spectra with non-linear dark-sector interactions
- A note on interacting holographic dark energy with a Hubble-scale cutoff
- Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids
- Constraining the interaction between dark sectors with future HI intensity mapping observations
- Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
- Cosmological perturbations and dynamical analysis for interacting quintessence
- Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
- III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
- New parameterization for unified dark matter and dark energy
- Constraints on interacting dark energy revisited: implications for the Hubble tension
- Reconstructing a non-linear interaction in the dark sector with cosmological observations
- Interacting dark energy in the dark model
- Are redshift-space distortions actually a probe of growth of structure?
- I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
- Inverted dipole feature in directional detection of exothermic dark matter
- New parameterizations of generalized Chaplygin gas model constrained at background and perturbation levels
- Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis
- Interacting Dark Energy and Its Implications for Unified Dark Sector
- A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
- Observational and Thermodynamic aspects of one-dimensional Dark Energy EoS parametrization models
- The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter