Constraining interacting dark energy with CMB and BAO future surveys

Abstract

In this paper, we perform a forecast analysis to test the capacity of future baryon acoustic oscillation (BAO) and cosmic microwave background (CMB) experiments to constrain phenomenological interacting dark energy models using the Fisher matrix formalism. We consider a Euclid-like experiment, in which BAO measurements is one of the main goals, to constrain the cosmological parameters of alternative cosmological models. Moreover, additional experimental probes can more efficiently provide information on the parameters forecast, justifying also the inclusion in the analysis of a future ground-based CMB experiment mainly designed to measure the polarization signal with high precision. In the interacting dark energy scenario, a coupling between dark matter and dark energy modifies the conservation equations such that the fluid equations for both constituents are conserved as the total energy density of the dark sector. In this context, we consider three phenomenological models which have been deeply investigated in literature over the past years. We find that the combination of both CMB and BAO information can break degeneracies among the dark sector parameters for all three models, although to different extents. We found powerful constraints on, for example, the coupling constant when comparing it with present limits for two of the models, and their future statistical 3-$\sigma$ bounds could potentially exclude the null interaction for the combination of probes that is considered. However, for one of the models, the constraint on the coupling parameter does not improve the present result (achieved using a large combination of surveys), and a larger combination of probes appears to be necessary to eventually claim whether or not interaction is favored in that context.

arXiv comment15 pages, 10 figures. Replaced to match published version

References in corpus (99)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• Particle Dark Matter: Evidence, Candidates and Constraints
• Efficient Computation of CMB anisotropies in closed FRW models
• Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
• Quintessence, Cosmic Coincidence, and the Cosmological Constant
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Dark Matter Candidates from Particle Physics and Methods of Detection
• An All-Sky Analysis of Polarization in the Microwave Background
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Cosmology and Fundamental Physics with the Euclid Satellite
• Cosmology and fundamental physics with the Euclid satellite
• Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
• Dark Energy
• Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Interacting quintessence solution to the coincidence problem
• Beyond $\Lambda$CDM: Problems, solutions, and the road ahead
• Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
• Measuring cosmological parameters with galaxy surveys
• Can interacting dark energy solve the $H_0$ tension?
• Probing the Coupling between Dark Components of the Universe
• Planck 2015 results. XIV. Dark energy and modified gravity
• Cosmic Complementarity: Joint Parameter Estimation from CMB Experiments and Redshift Surveys
• Late-time cosmology with 21cm intensity mapping experiments
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Indications of a late-time interaction in the dark sector
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Echo of interactions in the dark sector
• Interacting dark energy, holographic principle and coincidence problem
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• Interacting Dark Energy -- constraints and degeneracies
• New constraints on interacting dark energy from cosmic chronometers
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• New constraints on Coupled Dark Energy from Planck
• Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
• Cosmological coincidence problem in interacting dark energy models
• Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
• Interacting models may be key to solve the cosmic coincidence problem
• Toward a solution of the coincidence problem
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• The dark degeneracy: On the number and nature of dark components
• Testing the interaction between dark energy and dark matter via latest observations
• The Growth of Structure in Interacting Dark Energy Models
• Observational constraints on the dark energy and dark matter mutual coupling
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Coupled dark matter-dark energy in light of near Universe observations
• Testing modified gravity with Planck: the case of coupled dark energy
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Precision Epoch of Reionization studies with next-generation CMB experiments
• Evidence for interacting dark energy from BOSS
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Testing coupled dark energy with large scale structure observation
• Constraints on coupled dark energy using CMB data from WMAP and SPT
• Testing models of vacuum energy interacting with cold dark matter
• Testing coupled dark energy models with their cosmological background evolution
• Interacting Dark Energy and the Cosmic Coincidence Problem
• Constraining interacting dark energy models with latest cosmological observations
• On the Validity of Cosmological Fisher Matrix Forecasts
• Constraining the time evolution of dark energy, curvature and neutrino properties with cosmic chronometers
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Testing coupled dark energy with next-generation large-scale observations
• Fisher Matrices and Confidence Ellipses: A Quick-Start Guide and Software
• Coupled dark energy with perturbed Hubble expansion rate
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Cosmological constraints on coupled dark energy
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• Constraints on early dark energy from CMB lensing and weak lensing tomography
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Future CMB cosmological constraints in a dark coupled universe
• Yang-Mills condensate dark energy coupled with matter and radiation
• Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
• Constraining Modified Gravity with Euclid
• Future weak lensing constraints in a dark coupled universe
• CMB-lensing beyond the leading order: temperature and polarization anisotropies
• New Limits on Coupled Dark Energy from Planck
• Maps of CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies
• Update on the BINGO 21cm intensity mapping experiment
• Cosmological model of the interaction between dark matter and dark energy
• CMB and matter power spectra with non-linear dark-sector interactions
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Fitting and forecasting non-linear coupled dark energy
• Dark sectors of the Universe: A Euclid survey approach
• Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
• Cold dark energy constraints from the abundance of galaxy clusters
• Neutrinos and dark energy constraints from future galaxy surveys and CMB lensing information
• On detecting interactions in the dark sector with H(z) data
• Finding structure in the dark: coupled dark energy, weak lensing, and the mildly nonlinear regime
• Marginalized Fisher Forecast for Horndeski Dark Energy Models
• Elucidating Dark Energy with Future 21 cm Observations at the Epoch of Reionization
• Searches for Particle Dark Matter: An Introduction
• Constraining the interaction between dark matter and dark energy with CMB data

Cited by in corpus (32)

• Non-minimal dark sector physics and cosmological tensions
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
• Testing interacting dark matter and dark energy model with cosmological data
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• Probing the effects of primordial black holes on 21-cm EDGES signal along with interacting dark energy and dark matter - baryon scattering
• J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
• Background evolution and growth of structures in interacting dark energy through dynamical system analysis
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Probing Interacting Dark Energy and Scattering of Baryons with Dark Matter in Light of EDGES 21cm Signal
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• Testing the consistency of early and late cosmological parameters with BAO and CMB data
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• The Fisher gAlaxy suRvey cOde ($\text{FARO}$)
• Interacting Dark Energy: New parametrization and observational constraints
• Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints
• The model-independent degeneracy-breaking point in cosmological models with interacting Dark Energy and Dark Matter
• Revisiting dynamics of interacting quintessence