Using gravitational-wave standard sirens

Abstract

Gravitational waves (GWs) from supermassive binary black hole (BBH) inspirals are potentially powerful standard sirens (the GW analog to standard candles) (Schutz 1986, 2002). Because these systems are well-modeled, the space-based GW observatory LISA will be able to measure the luminosity distance (but not the redshift) to some distant massive BBH systems with 1-10% accuracy. This accuracy is largely limited by pointing error: GW sources generally are poorly localized on the sky. Localizing the binary independently (e.g., through association with an electromagnetic counterpart) greatly reduces this positional error. An electromagnetic counterpart may also allow determination of the event's redshift. In this case, BBH coalescence would constitute an extremely precise (better than 1%) standard candle visible to high redshift. In practice, gravitational lensing degrades this precision, though the candle remains precise enough to provide useful information about the distance-redshift relation. Even if very rare, these GW standard sirens would complement, and increase confidence in, other standard candles.

10 pages, 8 figures. ApJ, in press

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• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Dark-siren Cosmology with Decihertz Gravitational-wave Detectors
• A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
• Constraining cosmological parameters from strong lensing with DECIGO and B-DECIGO sources
• Eccentricity enables the earliest warning and localization of gravitational waves with ground-based detectors
• Gravitational Wave Sirens as a Triple Probe of Dark Energy
• Probing cosmic anisotropy with GW/FRB as upgraded standard sirens
• Prospects of LIGO for constraining inclination of merging compact binaries associated with three-dimensionally localized short-hard GRBs
• Source localizations with the network of space-based gravitational wave detectors
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Multi-spectral Sirens: Gravitational-wave Cosmology with (Multi-) Sub-populations of Binary Black Holes
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Gravitational wave cosmology and astrophysics with large spectroscopic galaxy surveys
• A crucial test of the phantom closed cosmological model
• A catalog of candidate double and lensed quasars from Gaia and WISE data
• Distinguish the $f(T)$ model from $\Lambda$CDM model with Gravitational Wave observations
• Gravitational wave astrophysics, data analysis and multimessenger astronomy
• Astronomy and astrophysics with gravitational waves in the Advanced Detector Era
• The appearance of a merging binary black hole very close to a spinning supermassive black hole
• Constraining the host galaxy halos of massive black holes from LISA event rates
• Luminosity distance uncertainties from gravitational wave detections by third generation observatories
• Upper Limit on the Dissipation of Gravitational Waves in Gravitationally Bound Systems
• Direct geometrical measurement of the Hubble constant from galaxy parallax: predictions for the Vera C. Rubin Observatory and Nancy Grace Roman Space Telescope
• Fundamental Physics and Cosmology with TianQin
• Probing Interacting Dark Sector with the next generation of gravitational-wave detectors
• Radiatively inefficient accretion flows induced by gravitational-wave emission before massive black hole coalescence
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
• Unveiling the Universe with Emerging Cosmological Probes
• Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in $N$-body simulations
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• A model-independent constraint on the Hubble constant with gravitational waves from the Einstein Telescope
• Cosmological model selection from standard siren detections by third-generation gravitational wave obervatories
• Precessing Binary Black Holes as Better Dark Sirens
• Measuring the Hubble Constant with Double Gravitational Wave Sources in Pulsar Timing
• Precise peculiar velocities from gravitational waves accompanied by electromagnetic signals and cosmological applications
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• Fresnel Models for Gravitational Wave Effects on Pulsar Timing
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Hubble without the Hubble: cosmology using advanced gravitational-wave detectors alone
• Novel standard candle: Collapsing axion stars
• Estimating Hubble Constant with Gravitational Observations: A Concise Review
• Cosmology and the Early Universe
• Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
• Corrections to the gravitational wave phasing
• Accelerating the standard siren method: Improved constraints on modified gravitational-wave propagation with future data
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Impact of weak lensing on bright standard siren analyses
• X- and Gamma-ray astrophysics in the era of Multi-messenger astronomy
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations II: Unique Stellar Kinematics in Integral Field Unit Spectroscopy
• Prospects of probing dark energy with eLISA: Standard versus null diagnostics
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Accelerated parameter estimation of supermassive black hole binaries in LISA using a meshfree approximation
• Hawai'i Supernova Flows: A Peculiar Velocity Survey Using Over a Thousand Supernovae in the Near-Infrared
• High precision measurement of cosmic curvature: from gravitational waves and cosmic chronometer
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• The Hubble Diagram: Jump from Supernovae to Gamma-Ray Bursts
• Modified propagation of gravitational waves from the early radiation era
• Gravitational waves from galaxy encounters
• Cosmology in the dark: How compact binaries formation impact the gravitational-waves cosmological measurements
• Modified $f(R,T)$ theory in light of gravitational wave standard sirens
• A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
• A Hubble constant estimation with dark standard sirens and galaxy cluster catalogues
• Possible use of self-calibration to reduce systematic uncertainties in determining distance-redshift relation via gravitational radiation from merging binaries
• Inferring astrophysics and cosmology with individual compact binary coalescences and their gravitational-wave stochastic background
• Sky localization of space-based detectors with time-delay interferometry
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
• Measuring the speed of gravity and the cosmic expansion with time delays between gravity and light from binary neutron stars
• Bright siren without electromagnetic counterpart by LISA-Taiji-TianQin network
• Dark energy model with very large-scale inhomogeneity
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Systematic errors in low latency gravitational wave parameter estimation impact electromagnetic follow-up observations
• El-CID: A filter for Gravitational-wave Electromagnetic Counterpart Identification
• Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
• Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
• Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals
• Confusion background from compact binaries
• Joint estimation of the cosmological model and the mass and redshift distributions of the binary black hole population with the Einstein Telescope
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• On the use of galaxy catalogs in gravitational-wave parameter estimation
• A dynamical dark energy solution to Hubble-Lemaître tension in the light of the multimessenger era
• Contaminating Electromagnetic Transients in LISA Gravitational Wave Localization Volumes. I: The Intrinsic Rates
• Scattering of Gravitational Radiation: Intensity Fluctuations
• Matters of Gravity, The Newsletter of the Division of Gravitational Physics of the American Physical Society, Volume 48, December 2016
• Measuring the Hubble Constant Near and Far in the Era of ELT's
• Calibrating systematic errors in the distance determination with the luminosity-distance space large scale structure of dark sirens and its potential applications
• Weak lensing of bright standard sirens: prospects for ${\sigma }_8$
• First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
• Pushing spectral siren cosmology into the third-generation era: a blinded mock data challenge
• Measurement of the Hubble constant using the Dark Energy Survey Year 6 Gold galaxy catalogue and the fourth Gravitational-Wave Transient Catalogue
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Particle Physics with Gravitational Wave Detector Technology
• Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA
• Standard candles and sirens rescue $H_0$
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• Search for Continuous Gravitational Wave Signals in Pulsar Timing Residuals: A New Scalable Approach with Diffusive Nested Sampling
• Listening Across the Cosmic Time: Standard Sirens from Ground- and Space-Based Missions in the Next Decade
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Gravitational-wave standard sirens and application in cosmology
• Preliminary census of galaxies in the LISA localisation volume: I. Searching for LISA candidate massive black hole binary merger hosts using Sloan Digital Sky Survey photometry
• Gravitational wave distance estimation using intrinsic signal properties: dark sirens as distance indicators
• A fully-automated end-to-end pipeline for massive black hole binary signal extraction from LISA data
• Constraining the lensing dispersion from the angular clustering of binary black hole mergers
• A Tale of Two Jets
• Precision Joint Constraints on Cosmology and Gravity Using Strongly Lensed Gravitational Wave Populations
• Prospects for measuring the Doppler magnification dipole with LSST and DESI
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• GWCloud: a searchable repository for the creation and curation of gravitational-wave inference results