Estimating Hubble Constant with Gravitational Observations: A Concise Review
arXiv:2506.15410 · doi:10.3390/galaxies13030065
Abstract
The Hubble constant is of paramount importance in astrophysics and cosmology. A large number of methods have been developed with different electromagnetic probes to estimate its value. The most recent results show a tension between values obtained from Cosmic Microwave Background observations and supernovae. The simultaneous detection of gravitational waves and electromagnetic radiation from GW170817 provided a direct estimation of the Hubble constant that did not depend on the astronomical distance ladder. This concise review will present the methods to estimate the Hubble constant with the gravitational observations of compact binary mergers, discussing both bright and dark sirens and reporting the state of the art of the results.
Contribution to "Gamma-Ray Bursts in Multiwavelength: Theory, Observational Correlations and GRB Cosmology", Special Issue of Galaxies, Editors Maria Giovanna Dainotti and Nissim Fraija, https://www.mdpi.com/journal/galaxies/special_issues/VS030A19AJ#
References in corpus (117)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Planck 2015 results. XIII. Cosmological parameters
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- A 2.4% Determination of the Local Value of the Hubble Constant
- In the Realm of the Hubble tension a Review of Solutions
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
- GW190521: A Binary Black Hole Merger with a Total Mass of
- Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Short-Duration Gamma-Ray Bursts
- INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
- The X-ray counterpart to the gravitational wave event GW 170817
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- Using gravitational-wave standard sirens
- Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
- The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
- Observation of gravitational waves from two neutron star-black hole coalescences
- Cosmological implications of baryon acoustic oscillation (BAO) measurements
- GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
- Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
- Superluminal motion of a relativistic jet in the neutron star merger GW170817
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- Swift and NuSTAR observations of GW170817: detection of a blue kilonova
- A Radio Counterpart to a Neutron Star Merger
- Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
- H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
- Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant
- The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
- A 2 per cent Hubble constant measurement from standard sirens within 5 years
- Exploring short gamma-ray bursts as gravitational-wave standard sirens
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. V. Rising X-ray Emission from an Off-Axis Jet
- TDCOSMO IV: Hierarchical time-delay cosmography -- joint inference of the Hubble constant and galaxy density profiles
- The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. VI. Radio Constraints on a Relativistic Jet and Predictions for Late-Time Emission from the Kilonova Ejecta
- The Locations of Short Gamma-ray Bursts as Evidence for Compact Object Binary Progenitors
- One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
- 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
- Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field
- Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
- MASTER optical detection of the first LIGO/Virgo neutron stars merging GW170817
- Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
- Groups of Galaxies in the Two Micron All-Sky Redshift Survey
- Constraints on the cosmic expansion history from GWTC-3
- A gravitational-wave measurement of the Hubble constant following the second observing run of Advanced LIGO and Virgo
- Elucidating CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy
- STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
- A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
- Prospects for resolving the Hubble constant tension with standard sirens
- Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
- The gravitational-wave luminosity distance in modified gravity theories
- Short Gamma-Ray Bursts from the Merger of Two Black Holes
- Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
- 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 Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
- Modified gravitational-wave propagation and standard sirens
- Measurements of the Temperature and E-Mode Polarization of the CMB from 500 Square Degrees of SPTpol Data
- Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
- The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant
- The Hubble Constant from Infrared Surface Brightness Fluctuation Distances
- The Distance to NGC 4993: The Host Galaxy of the Gravitational-wave Event GW170817
- The 6dF Galaxy Survey: Peculiar Velocity Field and Cosmography
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
- A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
- A measurement of the Hubble constant from Type II supernovae
- GROWTH on S190425z: Searching thousands of square degrees to identify an optical or infrared counterpart to a binary neutron star merger with the Zwicky Transient Facility and Palomar Gattini IR
- A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
- Distance measures in gravitational-wave astrophysics and cosmology
- Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology
- A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
- Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations
- Using The Baryonic Tully-Fisher Relation to Measure
- The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant
- Electromagnetic Counterparts to Massive Black Hole Mergers
- On the Progenitor of Binary Neutron Star Merger GW170817
- GLADE+: An Extended Galaxy Catalogue for Multimessenger Searches with Advanced Gravitational-wave Detectors
- Velocity correction for Hubble constant measurements from standard sirens
- The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin
- Follow-up of the Neutron Star Bearing Gravitational Wave Candidate Events S190425z and S190426c with MMT and SOAR
- A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light -ray attenuation
- 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
- Electromagnetic signals following stellar-mass black hole mergers
- Do LIGO/Virgo black hole mergers produce AGN flares? The case of GW190521 and prospects for reaching a confident association
- Ultrafast Outflows from Black Hole Mergers with a Mini-Disk
- Direct detection of gravitational waves can measure the time variation of the Planck mass
- The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
- The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations
- Distance and properties of NGC 4993 as the host galaxy of a gravitational wave source, GW170817
- Optical measurement of superluminal motion in the neutron-star merger GW170817
- Incompleteness Matters Not: Inference of from BBH-galaxy cross-correlations
- Electromagnetic Counterparts to Black Hole Mergers
- Observation of the second LIGO/Virgo event connected with binary neutron star merger S190425z in the gamma-ray range
- Gravity in the infrared and effective nonlocal models
- Cosmology with Standard Sirens at Cosmic Noon
- Cosmological inference from standard sirens without redshift measurements
- Horndeski gravity and standard sirens
- Gravitational wave observations, distance measurement uncertainties, and cosmology
- The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source
- Gravitational waves and geometrical optics in scalar-tensor theories
- Limitations on Standard Sirens tests of gravity from screening
- A search for radio emission from double-neutron star merger GW190425 using Apertif
- A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
- The most probable host of CHIME FRB 190425A, associated with binary neutron star merger GW190425, and a late-time transient search
- A Globular Cluster Luminosity Function Distance to NGC 4993 Hosting a Binary Neutron Star Merger GW170817/GRB 170817A
- MAXI upper limits of the electromagnetic counterpart of GW170817
- Comparing the luminosity distance for gravitational waves and electromagnetic signals in a simple model of quadratic gravity
- Gravitational Wave luminosity distance in viscous cosmological models