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.

arXiv comment12 pages, 6 figures; accepted for publication in Chinese Physics C

References in corpus (123)

• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• 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
• In the Realm of the Hubble tension $-$ a Review of Solutions
• The Pantheon+ Analysis: Cosmological Constraints
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Tensions between the Early and the Late Universe
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• Cosmology and Fundamental Physics with the Euclid Satellite
• Challenges for $\Lambda$CDM: An update
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
• Using gravitational-wave standard sirens
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• Taiji Program: Gravitational-Wave Sources
• Cosmology Intertwined II: The Hubble Constant Tension
• New physics in light of the $H_0$ tension: an alternative view
• Science with the space-based interferometer eLISA. I: Supermassive black hole binaries
• The missing link: Merging neutron stars naturally produce jet-like structures and can power short Gamma-Ray Bursts
• The Expansion of the Universe is Faster than Expected
• The North American Nanohertz Observatory for Gravitational Waves
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Non-minimal dark sector physics and cosmological tensions
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• A massive binary black-hole system in OJ287 and a test of general relativity
• A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
• The TianQin project: current progress on science and technology
• A possible close supermassive black-hole binary in a quasar with optical periodicity
• A Critical Assessment of Photometric Redshift Methods: A CANDELS Investigation
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• The Association of Jet Production with Geometrically Thick Accretion Flows and Black Hole Rotation
• A systematic search for close supermassive black hole binaries in the Catalina Real-Time Transient Survey
• Short GRB and binary black hole standard sirens as a probe of dark energy
• 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
• Three Dimensional MHD Simulation of Circumbinary Accretion Disks: Disk Structures and Angular Momentum Transport
• Ultra-high precision cosmology from gravitational waves
• A Population of Short-Period Variable Quasars from PTF as Supermassive Black Hole Binary Candidates
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
• Science with the space-based interferometer eLISA. III: Probing the expansion of the Universe using gravitational wave standard sirens
• The Parkes Pulsar Timing Array
• Distance Priors from Planck Final Release
• Dual Jets from Binary Black Holes
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• Pulsar searches and timing with the SKA
• Finding the Electromagnetic Counterparts of Cosmological Standard Sirens
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• The First Round Result from the TianQin-1 Satellite
• Can the $H_0$ tension be resolved in extensions to $\Lambda$CDM cosmology?
• Massive black hole binaries: dynamical evolution and observational signatures
• 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
• $f(T)$ gravity after GW170817 and GRB170817A
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Parkes Pulsar Timing Array constraints on ultralight scalar-field dark matter
• Optimal strategies for continuous gravitational wave detection in pulsar timing arrays
• On Estimation of the Post-Newtonian Parameters in the Gravitational-Wave Emission of a Coalescing Binary
• Spectroscopic Indication for a Centi-parsec Supermassive Black Hole Binary in the Galactic Center of NGC 5548
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• Measuring the Hubble constant with neutron star black hole mergers
• The Gravitational-Wave Physics II: Progress
• Velocity correction for Hubble constant measurements from standard sirens
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Chameleon dark energy can resolve the Hubble tension
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• On the detectability of dual jets from binary black holes
• Relieving the $H_0$ tension with a new interacting dark energy model
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Probing cosmic anisotropy with gravitational waves as standard sirens
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• A probable Milli-Parsec Supermassive Binary Black Hole in the Nearest Quasar Mrk 231
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Gravitational wave standard sirens and cosmological parameter measurement
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• Preliminary study on parameter estimation accuracy of supermassive black hole binary inspirals for TianQin
• SDSS J0159+0105: A Radio-Quiet Quasar with a Centi-Parsec Supermassive Black Hole Binary Candidate
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• How can gravitational-wave standard sirens and 21 cm intensity mapping jointly provide a precise late-universe cosmological probe?
• Can Non-standard Recombination Resolve the Hubble Tension?
• Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
• Testing the Quasar Hubble Diagram with LISA Standard Sirens
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Constraints on the distance duality relation with standard sirens
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• A Possible ~20 yr Periodicity in Long-term Optical Photometric and Spectral Variations of the Nearby Radio-Quiet Active Galactic Nucleus Ark 120
• Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• The LISA-Taiji network: precision localization of massive black hole binaries
• Cosmology with Standard Sirens at Cosmic Noon
• Late time cosmology with LISA: probing the cosmic expansion with massive black hole binary mergers as standard sirens
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Measuring the Hubble constant with black sirens
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Testing primordial black hole and measuring the Hubble constant with multiband gravitational-wave observations
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• A new way to explore cosmological tensions using gravitational waves and strong gravitational lensing
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Inflation model selection revisited after a 1.91% measurement of the Hubble constant
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Blindly Detecting Merging Supermassive Black Holes with Radio Surveys
• Hyperunified field theory and Taiji program in space for GWD
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Cosmography with Standard Sirens from the Einstein Telescope
• Blindly detecting orbital modulations of jets from merging supermassive black holes
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• A novel method of measuring cosmological distances using broad-line regions of quasars
• A Search for TeV Gamma-ray Emission from Pulsar Tails by VERITAS
• Standard sirens and dark sector with Gaussian process

Cited by in corpus (22)

• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• 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