Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations

Abstract

Gravitational waves (GWs) from the compact binary coalescences can be used as standard sirens to explore the cosmic expansion history. In the next decades, it is anticipated that we could obtain the multi-band GW standard siren data (from nanohertz to a few hundred hertz), which are expected to play an important role in cosmological parameter estimation. In this work, we give for the first time the joint constraints on cosmological parameters using the future multi-band GW standard siren observations. We simulate the multi-band GW standard sirens based on the SKA-era pulsar timing array (PTA), the Taiji observatory, and the Cosmic Explorer (CE) to perform cosmological analysis. In the $\Lambda$CDM model, we find that the joint PTA+Taiji+CE data could provide a tight constraint on the Hubble constant with a $0.5\%$ precision. Moreover, PTA+Taiji+CE could break the cosmological parameter degeneracies generated by CMB, especially in the dynamical dark energy models. When combining the PTA+Taiji+CE data with the CMB data, the constraint precisions of ${\Omega }_{\mathrm{m}}$ and $H_0$ are $1.0\%$ and $0.3\%$, meeting the standard of precision cosmology. The joint CMB+PTA+Taiji+CE data give $\sigma (w)=0.028$ in the $w$CDM model and $\sigma (w_0)=0.11$ and $\sigma (w_a)=0.32$ in the $w_0{w}_a$CDM model, which are comparable with or close to the latest constraint results by CMB+BAO+SN. In conclusion, it is worth expecting to use the future multi-band GW observations to explore the nature of dark energy and measure the Hubble constant.

12 pages, 6 figures; accepted for publication in Chinese Physics C

References in corpus (29)

• The Pantheon+ Analysis: Cosmological Constraints
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• The Expansion of the Universe is Faster than Expected
• A massive binary black-hole system in OJ287 and a test of general relativity
• The TianQin project: current progress on science and technology
• A possible close supermassive black-hole binary in a quasar with optical periodicity
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• The First Round Result from the TianQin-1 Satellite
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
• The Gravitational-Wave Physics II: Progress
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• A Search for TeV Gamma-ray Emission from Pulsar Tails by VERITAS
• A novel method of measuring cosmological distances using broad-line regions of quasars
• Standard sirens and dark sector with Gaussian process

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• 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
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Cosmology with fast radio bursts in the era of SKA
• Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens
• 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
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Fundamental Physics and Cosmology with TianQin
• 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
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Gravitational-wave standard sirens and application in cosmology
• Primordial gravitational waves: Model effects on time evolution and spectrum
• Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model