Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
arXiv:2101.12660 · doi:10.1088/1475-7516/2021/08/026
Abstract
We present a detailed study of the methodology for correlating `dark sirens' (compact binaries coalescences without electromagnetic counterpart) with galaxy catalogs. We propose several improvements on the current state of the art, and we apply them to the GWTC-2 catalog of LIGO/Virgo gravitational wave (GW) detections, and the GLADE galaxy catalog, performing a detailed study of several sources of systematic errors that, with the expected increase in statistics, will eventually become the dominant limitation. We provide a measurement of from dark sirens alone, finding as the best result ( c.l.) which is, currently, the most stringent constraint obtained using only dark sirens. Combining dark sirens with the counterpart for GW170817 we find . We also study modified GW propagation, which is a smoking gun of dark energy and modifications of gravity at cosmological scales, and we show that current observations of dark sirens already start to provide interesting limits. From dark sirens alone, our best result for the parameter that measures deviations from GR (with in GR) is . We finally discuss limits on modified GW propagation under the tentative identification of the flare ZTF19abanrhr as the electromagnetic counterpart of the binary black hole coalescence GW190521, in which case our most stringent result is . We release the publicly available code , which is available under open source license at \url{https://github.com/CosmoStatGW/DarkSirensStat}.
arXiv commentv2: several significant technical improvements, results changed v3: minor changes, Fig 9 added. The version to appear in JCAP
References in corpus (123)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Cosmic Star Formation History
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- 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 Black Hole with a 2.6 M Compact Object
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- 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
- A gravitational-wave standard siren measurement of the Hubble constant
- Science Case for the Einstein Telescope
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors
- Dark Energy after GW170817: dead ends and the road ahead
- INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Dark Energy after GW170817 and GRB170817A
- Using gravitational-wave standard sirens
- Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
- Observing binary inspiral in gravitational radiation: One interferometer
- Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521
- Superluminal motion of a relativistic jet in the neutron star merger GW170817
- The K-Band Galaxy Luminosity Function
- An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models
- A 2 per cent Hubble constant measurement from standard sirens within 5 years
- Exploring short gamma-ray bursts as gravitational-wave standard sirens
- Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
- Extracting distribution parameters from multiple uncertain observations with selection biases
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
- Tracing the cosmic web
- Breaking a Dark Degeneracy with Gravitational Waves
- Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries
- Short GRB and binary black hole standard sirens as a probe of dark energy
- Setting the cornerstone for the IMRPhenomX family of models for gravitational waves from compact binaries: The dominant harmonic for non-precessing quasi-circular black holes
- 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
- Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
- Does the Black Hole Merger Rate Evolve with Redshift?
- Ultra-high precision cosmology from gravitational waves
- Groups of Galaxies in the Two Micron All-Sky Redshift Survey
- Cosmic Voids in Sloan Digital Sky Survey Data Release 7
- 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
- A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
- Anisotropic stress as signature of non-standard propagation of gravitational waves
- Cosmography with the Einstein Telescope
- Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
- Cosmological perturbations and structure formation in nonlocal infrared modifications of general relativity
- Prospects for resolving the Hubble constant tension with standard sirens
- Testing modified gravity at cosmological distances with LISA standard sirens
- Gravitational Rainbows: LIGO and Dark Energy at its Cutoff
- Non-local gravity and dark energy
- Planck 2018 results. VI. Cosmological parameters
- Cosmology with the lights off: Standard sirens in the Einstein Telescope era
- Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
- The gravitational-wave luminosity distance in modified gravity theories
- 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 Future Percent-Level Measurement of the Hubble Expansion at Redshift 0.8 With Advanced LIGO
- Modified gravitational-wave propagation and standard sirens
- GW170817 Falsifies Dark Matter Emulators
- Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
- Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
- Nonlocal gravity. Conceptual aspects and cosmological predictions
- Ram-pressure stripping of a kicked Hill sphere: Prompt electromagnetic emission from the merger of stellar mass black holes in an AGN accretion disk
- Limits on the number of spacetime dimensions from GW170817
- A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations
- Galaxy Strategy for LIGO-Virgo Gravitational Wave Counterpart Searches
- Phantom dark energy from non-local infrared modifications of General Relativity
- A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations
- A statistical standard siren measurement of the Hubble constant from the LIGO/Virgo gravitational wave compact object merger GW190814 and Dark Energy Survey galaxies
- Minding the gap: GW190521 as a straddling binary
- Optical Follow-up of Gravitational-wave Events with Las Cumbres Observatory
- Accounting for Source Uncertainties in Analyses of Astronomical Survey Data
- Standard sirens with a running Planck mass
- Velocity correction for Hubble constant measurements from standard sirens
- Shouts and Murmurs: Combining Individual Gravitational-Wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers
- Cosmology and dark energy from joint gravitational wave-GRB observations
- Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
- Inferring the properties of a population of compact binaries in presence of selection effects
- Dark Sirens to Resolve the Hubble-Lemaître Tension
- Current observations are insufficient to confidently associate the binary black hole merger GW190521 with AGN J124942.3+344929
- When are LIGO/Virgo's Big Black-Hole Mergers?
- Non-local gravity and comparison with observational datasets
- Direct detection of gravitational waves can measure the time variation of the Planck mass
- Nonlinear structure formation in Nonlocal Gravity
- Supplement: Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
- Cosmological dynamics and dark energy from non-local infrared modifications of gravity
- Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
- Incompleteness Matters Not: Inference of from BBH-galaxy cross-correlations
- Changing the prior: absolute neutrino mass constraints in nonlocal gravity
- Spherically symmetric static solutions in a non-local infrared modification of General Relativity
- Astrophysical Model Selection in Gravitational Wave Astronomy
- Cosmological perturbation effects on gravitational-wave luminosity distance estimates
- Non-local gravity and comparison with observational datasets. II. Updated results and Bayesian model comparison with CDM
- Testing nonlocal gravity with Lunar Laser Ranging
- Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
- Gravity in the infrared and effective nonlocal models
- Cosmological perturbations and observational constraints on nonlocal massive gravity
- Hearing gravity from the cosmos: GWTC-2 probes general relativity at cosmological scales
- Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey
- Gravitational wave friction in light of GW170817 and GW190521
- Nonlocal gravity and gravitational-wave observations
- Testing Gravity with Gravitational Wave Source Counts
- Galaxy groups in the 2MASS Redshift Survey
- The 2MASS redshift survey galaxy group catalogue derived from a graph-theory based friends-of-friends algorithm
- A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
- Probing the large scale structure using gravitational-wave observations of binary black holes
- The Loudest Gravitational Wave Events
- The potential role of binary neutron star merger afterglows in multimessenger cosmology
- Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
- Gravitational wave source counts at high redshift and in models with extra dimensions
- Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
- A Standard Siren Cosmological Measurement from the Potential GW190521 Electromagnetic Counterpart ZTF19abanrhr
- Modified Gravity and Dark Energy models Beyond CDM Testable by LSST
Cited by in corpus (5)
- 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
- Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
- Modified gravitational wave propagation and the binary neutron star mass function
- Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
- Probing modified gravitational wave propagation with strongly lensed coalescing binaries