Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy

Abstract

In this work, we investigate the impacts of the future gravitational-wave (GW) standard siren observation by the Einstein Telescope (ET) on constraining the interacting dark energy (IDE) models. We simulate 1000 GW events in the redshift range of $0\lesssim z\lesssim 5$ based on the 10-year observation of the ET. We combine the simulated GW data with the current mainstream cosmological electromagnetic observations including the cosmic microwave background anisotropies, the baryon acoustic oscillations, and the type Ia supernovae to constrain the IDE models. We consider typical IDE models in the context of a perturbed universe. To avoid the large-scale instability problem for IDE models, we apply the extended parameterized post-Friedmann approach to calculate the cosmological perturbations. We find that the addition of the GW standard siren data could significantly improve the constraint accuracies for most of the cosmological parameters (e.g., $H_0$, $w$, and ${\Omega }_{\mathrm{m}}$). For the coupling parameter $\beta$, the constraint errors could also be slightly improved when adding the GW data in the cosmological fit.

arXiv comment22 pages, 5 figures; accepted for publication in JCAP

References in corpus (146)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological parameters from SDSS and WMAP
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Case for a Positive Cosmological Lambda-term
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Dark Energy and the Accelerating Universe
• Coupled Quintessence
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• A gravitational-wave standard siren measurement of the Hubble constant
• The Second Data Release of the Sloan Digital Sky Survey
• Physics, Astrophysics and Cosmology with Gravitational Waves
• Dark Energy
• Using gravitational-wave standard sirens
• Reconstructing Dark Energy
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Scaling solutions in general non-minimal coupling theories
• Interacting quintessence solution to the coincidence problem
• Non-Gaussianity of the primordial perturbation in the curvaton model
• Large-scale instability in interacting dark energy and dark matter fluids
• Probing the Coupling between Dark Components of the Universe
• Dark Energy-Dark Matter Interaction and putative violation of the Equivalence Principle from the Abell Cluster A586
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Dynamics of dark energy with a coupling to dark matter
• Indications of a late-time interaction in the dark sector
• Dynamics of interacting dark energy
• Ultra-high precision cosmology from gravitational waves
• Cosmologies with Energy Exchange
• Extreme Gravity Tests with Gravitational Waves from Compact Binary Coalescences: (I) Inspiral-Merger
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Statefinder diagnostic for coupled quintessence
• Echo of interactions in the dark sector
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• First evidence of running cosmic vacuum: challenging the concordance model
• Dark Energy and Dark Matter
• Reconciling CMB and structure growth measurements with dark energy interactions
• Linear and nonlinear interactions in the dark sector
• Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters
• Baryon bias and structure formation in an accelerating universe
• New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter
• Testing Scalar-Tensor Gravity with Gravitational-Wave Observations of Inspiralling Compact Binaries
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Observational constraints on an interacting dark energy model
• Interacting Dark Energy -- constraints and degeneracies
• Gravitational waves from cosmological compact binaries
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Constraining Interactions in Cosmology's Dark Sector
• 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
• Signature of the interaction between dark energy and dark matter in galaxy clusters
• Probing interaction and spatial curvature in the holographic dark energy model
• Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
• Cosmological coincidence problem in interacting dark energy models
• Possible signals of vacuum dynamics in the Universe
• Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Phase-space analysis of interacting phantom cosmology
• Testing the interaction between dark energy and dark matter via latest observations
• The Growth of Structure in Interacting Dark Energy Models
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
• Parametrized Post-Friedmann Signatures of Acceleration in the CMB
• Reconstructing the interaction between dark energy and dark matter using Gaussian Processes
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Adiabatic instability in coupled dark energy-dark matter models
• Interacting Dark Energy and Cosmological Equations of State
• Adiabatic initial conditions for perturbations in interacting dark energy models
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• Constraint on Coupled Dark Energy Models from Observations
• Velocities as a probe of dark sector interactions
• On the Dark Sector Interactions
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Dynamical dark energy versus $\Lambda =$const. in light of observations
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Cosmological constraints on a decomposed Chaplygin gas
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Evidence for interacting dark energy from BOSS
• Effects of dark sectors' mutual interaction on the growth of structures
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Dark Coupling and Gauge Invariance
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• Testing coupled dark energy with large scale structure observation
• 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
• Testing models of vacuum energy interacting with cold dark matter
• Constraining interacting dark energy models with latest cosmological observations
• Testing coupled dark energy models with their cosmological background evolution
• Covariantizing the interaction between dark energy and dark matter
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Gravitational wave standard sirens and cosmological parameter measurement
• Revisit of the interacting holographic dark energy model after Planck 2015
• Running coupling: Does the coupling between dark energy and dark matter change sign during the cosmological evolution?
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Correlated isocurvature perturbations from mixed inflaton-curvaton decay
• Constraining f(R) gravity in solar system, cosmology and binary pulsar systems
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• The imprint of the interaction between dark sectors in galaxy clusters
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Cosmological constant vis-a-vis dynamical vacuum: bold challenging the $\Lambda$CDM
• Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• Probing the imprint of interacting dark energy on very large scales
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Future CMB cosmological constraints in a dark coupled universe
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Constraining interacting dark energy with CMB and BAO future surveys
• Cosmic age problem revisited in the holographic dark energy model
• Waveforms of compact binary inspiral gravitational radiation in screened modified gravity
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• On the Effects of Coupled Scalar Fields on Structure Formation
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Breaking parameter degeneracy in interacting dark energy models from observations
• Observational constraint on the interacting dark energy models including the Sandage-Loeb test
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• Cosmological parameter measurement and neutral hydrogen 21 cm sky survey with the Square Kilometre Array
• Insights into Dark Energy: Interplay Between Theory and Observation
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• $\Lambda (t)$CDM Model as a Unified Origin of Holographic and Agegraphic Dark Energy Models
• Coherent ${\rho }^0$ photoproduction in bulk matter at high energies

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• In the Realm of the Hubble tension $-$ a Review of Solutions
• Non-minimal dark sector physics and cosmological tensions
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• The Gravitational-Wave Physics II: Progress
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Exploring non-singular black holes in gravitational perturbations
• A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short $\gamma$-ray bursts
• Null test for cosmic curvature using Gaussian process
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Fundamental Physics and Cosmology with TianQin
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Cosmological perturbations in the energy-momentum squared gravity theory: constraints from gravitational wave standard sirens and redshift space distortions