Constraining the origin of stellar binary black hole mergers by detections of their lensed host galaxies and gravitational wave signals
arXiv:2210.09892 · doi:10.3847/1538-4357/ac98b7
Abstract
A significant number of stellar binary black hole (sBBH) mergers may be lensed and detected by the third generation gravitational wave (GW) detectors. Their lensed host galaxies may be detectable, which thus helps to accurately localize these sources and provide a new approach to study the origin of sBBHs. In this paper, we investigate the detectability of the lensed host galaxies for the lensed sBBH mergers. We find that the detection fraction of the host galaxies to the lensed GW events can be significantly different for a survey with a given limiting magnitude if sBBHs are produced by different mechanisms, such as the evolution of massive binary stars, the dynamical interactions in dense star clusters, and that assisted by active galactic nuclei or massive black holes. Furthermore, we illustrate that the statistical spatial distribution of those lensed sBBHs in its hosts resulting from different sBBH formation channels can be different from each other. Therefore, with the third generation GW detectors and future large scale galaxy surveys, it is possible to independently constrain the sBBH origin via the detection fraction of those lensed events with identifiable lensing host signatures and/or even constrain the contribution fractions from different sBBH formation mechanisms
arXiv comment13 pages, 5 figures, accepted for publication in ApJ
References in corpus (92)
- A Universal Density Profile from Hierarchical Clustering
- The Structure of Cold Dark Matter Halos
- Cosmic Star Formation History
- Multi-messenger Observations of a Binary Neutron Star Merger
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- Local Supermassive Black Holes, Relics of Active Galactic Nuclei and the X-ray Background
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- An Observational Determination of the Bolometric Quasar Luminosity Function
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- Observational constraints on growth of massive black holes
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars
- Cosmology and fundamental physics with the Euclid satellite
- Double Compact Objects I: The Significance Of The Common Envelope On Merger Rates
- Data analysis of gravitational-wave signals from spinning neutron stars. I. The signal and its detection
- Detection, Measurement and Gravitational Radiation
- Black hole mergers in the universe
- Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
- Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei
- The Last Three Minutes: Issues in Gravitational Wave Measurements of Coalescing Compact Binaries
- Assisted Inspirals of Stellar Mass Black Holes Embedded in AGN Disks: Solving the "Final AU Problem"
- Accurate universal models for the mass accretion histories and concentrations of dark matter halos
- The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
- Double Compact Objects III: Gravitational Wave Detection Rates
- Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys
- Double Compact Objects II: Cosmological Merger Rates
- Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
- Formation and Evolution of Compact Object Binaries in AGN Disks
- GW150914: Implications for the stochastic gravitational wave background from binary black holes
- Measuring the neutron star equation of state with gravitational wave observations
- Intermediate mass black holes in AGN disks: I. Production & Growth
- The progenitors of compact-object binaries: impact of metallicity, common envelope and natal kicks
- The population of galaxy-galaxy strong lenses in forthcoming optical imaging surveys
- Cosmology from the Chinese Space Station Optical Survey (CSS-OS)
- PyCBC Inference: A Python-based parameter estimation toolkit for compact binary coalescence signals
- The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos
- Bayesian coherent analysis of in-spiral gravitational wave signals with a detector network
- BPASS predictions for Binary Black-Hole Mergers
- Universal structure of dark matter haloes over a mass range of 20 orders of magnitude
- Dynamical Formation of the GW150914 Binary Black Hole
- Mass and Redshift Dependence of Dark Halo Structure
- Internal and Collective Properties of Galaxies in the Sloan Digital Sky Survey
- Phenomenological model for the gravitational-wave signal from precessing binary black holes with two-spin effects
- H0LiCOW IV. Lens mass model of HE 0435-1223 and blind measurement of its time-delay distance for cosmology
- AGN as Potential Factories for Eccentric Black Hole Mergers
- Black hole and neutron star mergers in galactic nuclei
- Gravitational lensing of gravitational waves: A statistical perspective
- The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
- Precision cosmology from future lensed gravitational wave and electromagnetic signals
- Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era
- Gravitational Lensing of Gravitational Waves from Merging Neutron Star Binaries
- Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
- Eccentric Black Hole Mergers in Active Galactic Nuclei
- Redshift Evolution of the Black Hole Merger Rate from Globular Clusters
- Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
- Detecting Lensing-Induced Diffraction in Astrophysical Gravitational Waves
- Metallicity-constrained merger rates of binary black holes and the stochastic gravitational wave background
- Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
- What if LIGO's gravitational wave detections are strongly lensed by massive galaxy clusters?
- Binary black hole mergers in AGN accretion discs: gravitational wave rate density estimates
- Estimating parameters of coalescing compact binaries with proposed advanced detector networks
- Strong gravitational lensing of gravitational waves from double compact binaries - perspectives for the Einstein Telescope
- Estimating parameters of coalescing compact binaries with a detector network including LIGO Australia
- Constraints on QSO models from a relation between the QSO luminosity function and the local black hole mass function
- Massive black hole evolution models confronting the n-Hz amplitude of the stochastic gravitational wave background
- Measuring the accretion rate and kinetic luminosity functions of supermassive black holes
- Comparison of Gravitational Wave Detector Network Sky Localization Approximations
- Identifying Type II Strongly Lensed Gravitational-Wave Images in Third-Generation Gravitational-Wave Detectors
- On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors
- Strongly lensed gravitational waves from intrinsically faint double compact binaries - prediction for the Einstein Telescope
- Strong gravitational lensing of gravitational waves in Einstein Telescope
- Mass and rate of hierarchical black hole mergers in young, globular and nuclear star clusters
- Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
- How large are the globular cluster systems of early-type galaxies and do they scale with galaxy halo properties?
- Constraining cosmological parameters in FLRW metric with lensed GW+EM signals
- The correlation between the sizes of globular cluster systems and their host dark matter haloes
- Strong lensing as a giant telescope to localize the host galaxy of gravitational wave event
- Gravitational Wave Interference via Gravitational Lensing: Measurements of Luminosity Distance, Lens Mass, and Cosmological Parameters
- Detectability and parameter estimation of stellar origin black hole binaries with next generation gravitational wave detectors
- Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
- Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
- Gravitational-wave merging events from the dynamics of stellar mass binary black holes around the massive black hole in a galactic nucleus
- Stochastic Gravitational Wave Background and Eccentric Stellar Compact Binaries
- How does the Earth's rotation affect predictions of gravitational wave strong lensing rates?
- Predictions for Strong Lens Detections with the Nancy Grace Roman Space Telescope
- A Mock Catalog of Gravitationally Lensed Quasars for the LSST Survey
- Blackhole Mergers Through Evection Resonances
- Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
- Constraining the stochastic gravitational wave from string cosmology with current and future high frequency detectors
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- Multiband gravitational wave observations of stellar binary black holes at the low to middle and high frequencies
- Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass
- Event Rate of Strongly Lensed Gravitational Waves of Stellar Binary Black Hole Mergers Produced by Dynamical Interactions
- Diffractive lensing of nano-Hertz gravitational waves emitted from supermassive binary black holes by intervening galaxies
- Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
- Gravitational-wave standard sirens and application in cosmology