Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history

Abstract

In the near future, the redshift drift observations in optical and radio bands will provide precise measurements on $H(z)$ covering the redshift ranges of $2<z<5$ and $0<z<0.3$. In addition, gravitational wave (GW) standard siren observations could make measurements on the dipole anisotropy of luminosity distance, which will also provide the $H(z)$ measurements in the redshift range of $0<z<3$. In this work, we propose a multi-messenger and multi-wavelength observational strategy to measure $H(z)$ based on the three next-generation projects, E-ELT, SKA, and DECIGO, and we wish to see whether the future $H(z)$ measurements could provide tight constraints on dark-energy parameters. The dark energy models we consider include $\Lambda$CDM, $w$CDM, CPL, HDE, and I$\Lambda$CDM models. It is found that E-ELT, SKA1, and DECIGO are highly complementary in constraining dark energy models. Although any one of these three data sets can only give rather weak constraints on each model we consider, the combination of them could significantly break the parameter degeneracies and give much tighter constraints on almost all the cosmological parameters. Moreover, we find that the combination of E-ELT, SKA1, DECIGO, and CMB could further improve the constraints on dark energy parameters, e.g., $\sigma (w_0)=0.024$ and $\sigma (w_a)=0.17$ in the CPL model, which means that these three promising probes will play a key role in helping reveal the nature of dark energy.

arXiv comment18 pages, 7 figures

References in corpus (56)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Multi-messenger Observations of a Binary Neutron Star Merger
• Exploring the Expansion History of the Universe
• Accelerating Universes with Scaling Dark Matter
• A Model of Holographic Dark Energy
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results
• Possibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space
• Small Scale Cosmological Perturbations: An Analytic Approach
• Clustering of Luminous Red Galaxies IV: Baryon Acoustic Peak in the Line-of-Sight Direction and a Direct Measurement of H(z)
• Constraints on holographic dark energy from type Ia supernova observations
• Ultra-high precision cosmology from gravitational waves
• Cosmic dynamics in the era of Extremely Large Telescopes
• Gamma-Ray Bursts From Neutron Star Phase Transitions
• Direct Measurement of Cosmological Parameters from the Cosmic Deceleration of Extragalactic Objects
• Cosmography with the Einstein Telescope
• Distance Priors from Planck Final Release
• Gravitational waves from cosmological compact binaries
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Dipole of the luminosity distance: a direct measure of H(z)
• The Gravitational-Wave Physics II: Progress
• Real-time Cosmology
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• 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
• Constraining interacting dark energy models with latest cosmological observations
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Comparison of dark energy models after Planck 2015
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Gravitational wave standard sirens and cosmological parameter measurement
• 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
• 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
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Tracing the redshift evolution of Hubble parameter with gravitational-wave standard sirens
• 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
• Reducing distance errors for standard candles and standard sirens with weak-lensing shear and flexion maps
• Real-time cosmography with redshift derivatives
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Prospect for constraining holographic dark energy with gravitational wave standard sirens from the Einstein Telescope
• Cosmological Density and Power Spectrum from Peculiar Velocities: Nonlinear Corrections and PCA
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
• Forecasts of redshift drift constraints on cosmological parameters
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Real-time cosmology with SKA
• The constraint ability of Hubble parameter by gravitational wave standard sirens on cosmological parameters

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• Cosmology with the Laser Interferometer Space Antenna
• The Gravitational-Wave Physics II: Progress
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• Null test for cosmic curvature using Gaussian process
• Gravitational lensing of massive particles by a black-bounce-Schwarzschild black hole
• Constraining minimally extended varying speed of light by cosmological chronometers
• Testing the Cosmic Distance Duality Relation Using Strong Gravitational Lensing Time Delays and Type Ia Supernovae
• Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
• Quantifying effects of inhomogeneities and curvature on gravitational wave standard siren measurements of $H(z)$
• Leading-order deflection of particles by a moving Schwarzschild lens with a two-dimensional velocity
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Gravitational deflection of light in polar-axis plane of a moving Kerr-Newman black hole
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Qualitative probe of interacting dark energy with redshift-space distortions
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Dynamical analysis of the redshift drift in FLRW universes
• Leading-order gravitational time delay of massive particles by a moving Schwarzschild lens
• Strong field gravitational lensing of particles by a black-bounce-Schwarzschild black hole