Dark Sirens to Resolve the Hubble-Lemaître Tension

Abstract

The planned sensitivity upgrades to the LIGO and Virgo facilities could uniquely identify host galaxies of dark sirens-compact binary coalescences without any electromagnetic counterparts-within a redshift of z = 0.1. This is aided by the higher order spherical harmonic modes present in the gravitational-wave signal, which also improve distance estimation. In conjunction, sensitivity upgrades and higher modes will facilitate an accurate, independent measurement of the host galaxy's redshift in addition to the luminosity distance from the gravitational wave observation to infer the Hubble-Lemaître constant H0 to better than a few percent in five years. A possible Voyager upgrade or third generation facilities would further solidify the role of dark sirens for precision cosmology in the future.

arXiv comment7 pages, 3 figures

References in corpus (32)

• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Characterization of the LIGO detectors during their sixth science run
• Tensions between the Early and the Late Universe
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Frequency-domain gravitational waves from non-precessing black-hole binaries. I. New numerical waveforms and anatomy of the signal
• Using gravitational-wave standard sirens
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
• Cosmography with the Einstein Telescope
• Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• GLADE: A Galaxy Catalogue for Multi-Messenger Searches in the Advanced Gravitational-Wave Detector Era
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• A Cryogenic Silicon Interferometer for Gravitational-wave Detection
• Higher signal harmonics, LISA's angular resolution, and dark energy
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Estimating the parameters of non-spinning binary black holes using ground-based gravitational-wave detectors: Statistical errors
• The Advanced LIGO Photon Calibrators
• Binary black hole spectroscopy
• Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO
• Parameter Estimation with a spinning multi-mode waveform model: IMRPhenomHM
• Measurement of Hubble constant with stellar-mass binary black holes
• Host galaxy identification for binary black hole mergers with long baseline gravitational wave detectors

Cited by in corpus (61)

• Science with the Einstein Telescope: a comparison of different designs
• New Horizons for Fundamental Physics with LISA
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Constraints on the cosmic expansion history from GWTC-3
• Accurate precision Cosmology with redshift unknown gravitational wave sources
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• The Science of the Einstein Telescope
• Gwbench: a novel Fisher information package for gravitational-wave benchmarking
• 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
• Testing Late Time Cosmic Acceleration with uncorrelated Baryon Acoustic Oscillations dataset
• Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• 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
• Cosmology with Standard Sirens at Cosmic Noon
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• 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
• The Lunar Gravitational-wave Antenna: Mission Studies and Science Case
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Cosmography with next-generation gravitational wave detectors
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Eccentricity of Long Inspiraling Compact Binaries Sheds Light on Dark Sirens
• Gravitational wave populations and cosmology with neural posterior estimation
• Neutron star-black hole mergers in next generation gravitational-wave observatories
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Using Gray Sirens to Resolve the Hubble-Lemaître Tension
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• 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
• Improving the Cosmological Constraints by Inferring the Formation Channel of Extreme-mass-ratio Inspirals
• No slip gravity in light of LISA standard sirens
• Reconstructing the Hubble parameter with future Gravitational Wave missions using Machine Learning
• Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
• Detectability of gravitational higher order modes in the third-generation era
• Impact of unmodeled eccentricity on the tidal deformability measurement and implications for gravitational wave physics inference
• Eccentricity enables the earliest warning and localization of gravitational waves with ground-based detectors
• Space-borne atom interferometric gravitational wave detections. Part II. Dark sirens and finding the one
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Premerger localization of intermediate mass binary black holes with LISA and prospects of joint observations with Athena and LSST
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Precessing Binary Black Holes as Better Dark Sirens
• Inferring Binary Properties from Gravitational Wave Signals
• Cosmology of fermionic dark energy coupled to curvature
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Forecast cosmological constraints from the number counts of Gravitational Waves events
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Modeling Relative Peak Times of Gravitational Wave Harmonics
• Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
• Constraining the lensing dispersion from the angular clustering of binary black hole mergers
• Gravitational-wave standard sirens and application in cosmology
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX