Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation

Abstract

Using the measurements of tidal deformation in the binary neutron star (BNS) coalescences can obtain the information of redshifts of gravitational wave (GW) sources, and thus actually the cosmic expansion history can be investigated using solely such GW dark sirens. To do this, the key is to get a large number of accurate GW data, which can be achieved with the third-generation (3G) GW detectors. Here we wish to offer an answer to the question of whether the Hubble constant and the equation of state (EoS) of dark energy can be precisely measured using solely GW dark sirens. We find that in the era of 3G GW detectors $\mathcal{O}(10^5-10^6)$ dark siren data (with the NS tidal measurements) could be obtained in three-year observation if the EoS of NS is perfectly known, and thus using only dark sirens can actually achieve the precision cosmology. Based on a network of 3G detectors, we obtain the constraint precisions of $0.15\%$ and $0.95\%$ for the Hubble constant $H_0$ and the constant EoS of dark energy $w$, respectively; for a two-parameter EoS parametrization of dark energy, the precision of $w_0$ is $2.04\%$ and the error of $w_a$ is 0.13. We conclude that 3G GW detectors would lead to breakthroughs in solving the Hubble tension and revealing the nature of dark energy provided that the EoS of NS is perfectly known.

23 pages, 6 figures

References in corpus (73)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Cosmic Star Formation History
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• 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
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• The Pantheon+ Analysis: Cosmological Constraints
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Cosmology Intertwined II: The Hubble Constant Tension
• The Expansion of the Universe is Faster than Expected
• Late-time cosmology with 21cm intensity mapping experiments
• 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
• Constraints on the cosmic expansion history from GWTC-3
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
• Reducing the weak lensing noise for the gravitational wave Hubble diagram using the non-Gaussianity of the magnification distribution
• A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
• Implications for the Hubble tension from the ages of the oldest astrophysical objects
• The Gravitational-Wave Physics II: Progress
• Chameleon dark energy can resolve the Hubble tension
• Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
• Relieving the $H_0$ tension with a new interacting dark energy model
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• 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
• $Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• A Program for Multi-Messenger Standard Siren Cosmology in the Era of LIGO A+, Rubin Observatory, and Beyond
• $\text{GWFAST}$: a Fisher information matrix Python code for third-generation gravitational-wave detectors
• Testing H0 in Acoustic Dark Energy Models with Planck and ACT Polarization
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• 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?
• Testing the Quasar Hubble Diagram with LISA Standard Sirens
• Systematic uncertainty of standard sirens from the viewing angle of binary neutron star inspirals
• Constraints on the distance duality relation with standard sirens
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• Cosmology with Standard Sirens at Cosmic Noon
• Self-interacting dark matter from late decays and the $H_0$ tension
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Measuring the Hubble constant with black sirens
• Measuring the delay time distribution of binary neutron stars. II. Using the redshift distribution from third-generation gravitational wave detectors network
• 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
• Projected Cosmological Constraints from Strongly Lensed Supernovae with the Roman Space Telescope
• 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
• Exploiting the Einstein Telescope to solve the Hubble tension
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• 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
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• Prospects for measuring dark energy with 21 cm intensity mapping experiments: A joint survey strategy
• Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves
• Prospects for measuring dark energy with 21 cm intensity mapping experiments
• Cosmography with Standard Sirens from the Einstein Telescope
• 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
• Standard sirens and dark sector with Gaussian process
• Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
• HI intensity mapping with MeerKAT: forecast for delay power spectrum measurement using interferometer mode
• FRB dark sirens: Measuring the Hubble constant with unlocalized fast radio bursts
• Cosmography with bright and Love sirens
• Probing the Anisotropic Universe with Gravitational Waves

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