The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens

Abstract

In the coming decades, the space-based gravitational-wave (GW) detectors such as Taiji, TianQin, and LISA are expected to form a network capable of detecting millihertz GWs emitted by the mergers of massive black hole binaries (MBHBs). In this work, we investigate the potential of GW standard sirens from the Taiji-TianQin-LISA network in constraining cosmological parameters. For the optimistic scenario in which electromagnetic (EM) counterparts can be detected, we predict the number of detectable bright sirens based on three different MBHB population models, i.e., pop III, Q3d, and Q3nod. Our results show that the Taiji-TianQin-LISA network alone could achieve a constraint precision of $0.9\%$ for the Hubble constant, meeting the standard of precision cosmology. Moreover, the Taiji-TianQin-LISA network could effectively break the cosmological parameter degeneracies generated by the CMB data, particularly in the dynamical dark energy models. When combined with the CMB data, the joint CMB+Taiji-TianQin-LISA data offer $\sigma (w)=0.036$ in the $w$CDM model, which is close to the latest constraint result obtained from the CMB+SN data. We also consider a conservative scenario in which EM counterparts are not available. Due to the precise sky localizations of MBHBs by the Taiji-TianQin-LISA network, the constraint precision of the Hubble constant is expected to reach $1.2\%$. In conclusion, the GW standard sirens from the Taiji-TianQin-LISA network will play a critical role in helping solve the Hubble tension and shedding light on the nature of dark energy.

22 pages, 10 figures; published in Science China Physics Mechanics & Astronomy

References in corpus (60)

• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• Laser Interferometer Space Antenna
• 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
• The TianQin project: current progress on science and technology
• Cosmology with the Laser Interferometer Space Antenna
• The evolution of massive black hole seeds
• 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
• Holographic dark energy models: A comparison from the latest observational data
• Constraints on the cosmic expansion history from GWTC-3
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
• The First Round Result from the TianQin-1 Satellite
• The LISA-Taiji network
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• Binary Black Hole Accretion During Inspiral and Merger
• Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes
• A model for periodic blazars
• The Gravitational-Wave Physics II: Progress
• Accretion disks around binary black holes of unequal mass: GRMHD simulations of postdecoupling and merger
• A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• 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
• Cosmological constraints on neutrinos after BICEP2
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Detection of astrophysical gravitational wave sources by TianQin and LISA
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• 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
• Cosmology with fast radio bursts in the era of SKA
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• Exploiting the Einstein Telescope to solve the Hubble tension
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• On networks of space-based gravitational-wave detectors
• Prospects of strongly lensed repeating fast radio bursts: complementary constraints on dark energy evolution
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Polarized primordial gravitational waves in spatial covariant gravities
• Probing the interaction between dark energy and dark matter with future fast radio burst observations
• Parameter Estimation of Stellar Mass Binary Black Holes under the Network of TianQin and LISA
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Space-borne atom interferometric gravitational wave detections. Part III. Eccentricity on dark sirens
• A novel method of measuring cosmological distances using broad-line regions of quasars
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• Standard sirens and dark sector with Gaussian process
• Cosmography with bright and Love sirens
• FRB dark sirens: Measuring the Hubble constant with unlocalized fast radio bursts
• Probing the Anisotropic Universe with Gravitational Waves

Cited by in corpus (34)

• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• 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
• Gravitational waveforms from periodic orbits around a quantum-corrected black hole
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• 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
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• Premerger detection of massive black hole binaries using deep learning
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Detecting Cosmological Phase Transitions with Taiji: Sensitivity Analysis and Parameter Estimation
• Fundamental Physics and Cosmology with TianQin
• Revisiting the phenomenologically emergent dark energy model: is non-zero equation of state of dark matter favored by DESI DR2?
• Testing the cosmic distance duality relation with baryon acoustic oscillations and supernovae data
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Phase transitions in a holographic superfluid model with non-linear terms beyond the probe limit
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• 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
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra
• Source Confusion of Massive Black Hole Binaries for the Taiji Mission
• Unveiling the spectral morphological division of fast radio bursts with CHIME/FRB Catalog 2
• Gravitational-wave standard sirens and application in cosmology