Measuring the Hubble constant with coalescences of binary neutron star and neutron star-black hole: bright sirens \& dark sirens

Abstract

The observations of gravitational wave (GW) provide us a new probe to study the universe. GW events can be used as standard sirens if their redshifts are measured. Normally, stardard sirens can be divided into bright/dark sirens according to whether the redshifts are measured by electromagnetic (EM) counterpart observations. Firstly, we investigate the capability of the 2.5-meter Wide-Field Survey Telescope (WFST) to take follow-up observations of kilonova counterparts. For binary neutron star (BNS) bright sirens, WFST is expected to observe 10-20 kilonovae per year in the second-generation (2G) GW detection era. As for neutron star-black hole (NSBH) mergers, when a BH spin is extremely high and the NS is stiff, the observation rate is $\sim 10$ per year. Combining optical and GW observations, the bright sirens are expected to constrain the Hubble constant $H_0$ to $\sim 2.8\%$ in five years of observations. As for dark sirens, tidal effects of neutron stars (NSs) during merging time provide us a cosmological model-independent approach to measure the redshifts of GW sources. Then we investigate the applications of tidal effects in redshift measurements. We find in 3G era, the host galaxy groups of around 45\% BNS mergers at $z<0.1$ can be identified through this method, if the EOS is ms1, which is roughly equivalent to the results from luminosity distant constraints. Therefore, tidal effect observations provide a reliable and cosmological model-independent method of identifying BNS mergers' host galaxy groups. Using this method, the BNS/NSBH dark sirens can constrain $H_0$ to 0.2\%/0.3\% over a five-year observation period.

arXiv comment26 pages, 13 figures, submitted to APJS, comments welcome

References in corpus (179)

• 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
• The Seventh Data Release of the Sloan Digital Sky Survey
• A Massive Pulsar in a Compact Relativistic Binary
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• LSST: from Science Drivers to Reference Design and Anticipated Data Products
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• GW170817: Measurements of Neutron Star Radii and Equation of State
• GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• GW190814: Gravitational Waves from the Coalescence of a 23 M${}_{\odot }$ Black Hole with a 2.6 M${}_{\odot }$ Compact Object
• GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
• An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
• The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
• Masses, Radii, and Equation of State of Neutron Stars
• GW190521: A Binary Black Hole Merger with a Total Mass of $150M_{\odot }$
• Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
• A gravitational-wave standard siren measurement of the Hubble constant
• Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• The Dark Energy Camera
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
• Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
• A kilonova as the electromagnetic counterpart to a gravitational-wave source
• Physics, Astrophysics and Cosmology with Gravitational Waves
• The Zwicky Transient Facility: Science Objectives
• Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
• Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
• Using gravitational-wave standard sirens
• The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• Use and Abuse of the Fisher Information Matrix in the Assessment of Gravitational-Wave Parameter-Estimation Prospects
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
• Swift and NuSTAR observations of GW170817: detection of a blue kilonova
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South
• Systematics of dynamical mass ejection, nucleosynthesis, and radioactively powered electromagnetic signals from neutron-star mergers
• The mass ejection from the merger of binary neutron stars
• The Last Three Minutes: Issues in Gravitational Wave Measurements of Coalescing Compact Binaries
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta
• The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
• Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts and Nucleosynthesis
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational Wave Event S190521g
• Dynamical Mass Ejection from Binary Neutron Star Mergers
• Revealing the High-Redshift Star Formation Rate with Gamma-Ray Bursts
• Gravitational radiation from inspiralling compact binaries completed at the third post-Newtonian order
• Slowing the Spins of Stellar Cores
• The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes
• Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
• Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger
• Evolution of the Galaxy - Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos
• The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity
• Most Black Holes are Born Very Slowly Rotating
• Dimensional regularization of the gravitational interaction of point masses
• Dynamical mass ejection from the merger of asymmetric binary neutron stars: Radiation-hydrodynamics study in general relativity
• The rate, luminosity function and time delay of non-Collapsar short GRBs
• Prompt merger collapse and the maximum mass of neutron stars
• 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
• Hierarchical Black Hole Mergers in Active Galactic Nuclei
• Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
• Gravitational-Wave Inspiral of Compact Binary Systems to 7/2 Post-Newtonian Order
• The Uchuu Simulations: Data Release 1 and Dark Matter Halo Concentrations
• Multi-messenger Bayesian parameter inference of a binary neutron-star merger
• MASTER optical detection of the first LIGO/Virgo neutron stars merging GW170817
• Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
• Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
• The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO
• IndIGO and LIGO-India: Scope and Plans for Gravitational Wave Research and Precision Metrology in India
• Measuring the Spins of Accreting Black Holes
• Constraints on the cosmic expansion history from GWTC-3
• 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
• Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state
• Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
• A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart
• Dimensional regularization of the third post-Newtonian dynamics of point particles in harmonic coordinates
• Cosmography with the Einstein Telescope
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Spin orientations of merging black holes formed from the evolution of stellar binaries
• Remnant baryon mass outside of the black hole after a neutron star-black hole merger
• Three-dimensional GRMHD simulations of neutrino-cooled accretion disks from neutron star mergers
• Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs
• J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817
• Cosmological Inference using Gravitational Wave Standard Sirens: A Mock Data Challenge
• r-Process Nucleosynthesis in Hot Accretion Disk Flows from Black Hole - Neutron Star Mergers
• A Gravitational Wave Detector with Cosmological Reach
• POSSIS: predicting spectra, light curves and polarization for multi-dimensional models of supernovae and kilonovae
• Effective action approach to higher-order relativistic tidal interactions in binary systems and their effective one body description
• Unequal mass binary neutron star mergers and multimessenger signals
• Constraints on binary neutron star merger product from short GRB observations
• Modeling dynamical ejecta from binary neutron star mergers and implications for electromagnetic counterparts
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Nuclear Equation of State from Observations of Short Gamma-Ray Burst Remnants
• The Rapid Reddening and Featureless Optical Spectra of the optical counterpart of GW170817, AT 2017gfo, During the First Four Days
• Estimates for Disk and Ejecta Masses Produced in Compact Binary Mergers
• Galaxy Occupation Statistics of Dark Matter Haloes: Observational Results
• Constraints on interquark interaction parameters with GW170817 in a binary strange star scenario
• New derivation of a third post-Newtonian equation of motion for relativistic compact binaries without ambiguity
• Observations of the first electromagnetic counterpart to a gravitational wave source by the TOROS collaboration
• Geometrical Expression for the Angular Resolution of a Network of Gravitational-Wave Detectors
• Forecasting the detection capabilities of third-generation gravitational-wave detectors using $\text{GWFAST}$
• Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers
• On the Origin of Black Hole Spin in High-mass X-Ray Binaries
• 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
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for 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
• On the Conditions for Neutron-Rich Gamma-Ray Burst Outflows
• Black hole-neutron star binary merger: Dependence on black hole spin orientation and equations of state
• Data-driven expectations for electromagnetic counterpart searches based on LIGO/Virgo public alerts
• Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)
• First-post-Newtonian quadrupole tidal interactions in binary systems
• Populating Dark Matter Haloes with Galaxies: Comparing the 2dFGRS with Mock Galaxy Redshift Surveys
• GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger
• Optical Follow-up of Gravitational-wave Events with Las Cumbres Observatory
• Inadequacies of the Fisher Information Matrix in gravitational-wave parameter estimation
• Internal X-ray plateau in short GRBs: Signature of supramassive fast-rotating quark stars?
• Optical follow-up of the neutron star-black hole mergers S200105ae and S200115j
• Kilonova Luminosity Function Constraints based on Zwicky Transient Facility Searches for 13 Neutron Star Mergers
• Equation of motion for relativistic compact binaries with the strong field point particle limit: Third post-Newtonian order
• Neutron star equation of state from the quark level in the light of GW170817
• GRANDMA Observations of Advanced LIGO's and Advanced Virgo's Third Observational Campaign
• Spiral-wave wind for the blue kilonova
• Hadamard regularization of the third post-Newtonian gravitational wave generation of two point masses
• Optical Observations of LIGO Source GW 170817 by the Antarctic Survey Telescopes at Dome A, Antarctica
• An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8
• Tight multi-messenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light curve synthesis
• Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
• Dark Sirens to Resolve the Hubble-Lemaître Tension
• Equation of motion for relativistic compact binaries with the strong field point particle limit : the second and half post-Newtonian order
• 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
• Cosmological inference using only gravitational wave observations of binary neutron stars
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• The Hitchhiker's guide to the galaxy catalog approach for gravitational wave cosmology
• Optimizing searches for electromagnetic counterparts of gravitational wave triggers
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Comparison of Gravitational Wave Detector Network Sky Localization Approximations
• Post-Newtonian spin-tidal couplings for compact binaries
• Prospects for improving cosmological parameter estimation with gravitational-wave standard sirens from Taiji
• Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• Kilonova Emission From Black Hole-Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches
• Hunting for the host galaxy groups of binary black holes and the application in constraining Hubble constant
• Kilonova Emission From Black Hole-Neutron Star Mergers. I. Viewing-Angle-Dependent Lightcurves
• Multi-messenger Detection Rates and distributions of Binary Neutron Star Mergers and Their Cosmological Implications
• A trend in the effective spin distribution of LIGO binary black holes with mass
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Measurement of Hubble constant with stellar-mass binary black holes
• Constraining the observer angle of the kilonova AT2017gfo associated with GW170817: Implications for the Hubble constant
• GROWTH on S190510g: DECam Observation Planning and Follow-Up of a Distant Binary Neutron Star Merger Candidate
• Gravitomagnetic tidal effects in gravitational waves from neutron star binaries
• Prospects for Measuring the Hubble Constant with Neutron-Star-Black-Hole Mergers
• Sound velocity in dense stellar matter with strangeness and compact stars
• Comprehensive analysis of the tidal effect in gravitational waves and implication for cosmology
• The Angular Momenta of Neutron Stars and Black Holes as a Window on Supernovae
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Optimizing Serendipitous Detections of Kilonovae: Cadence and Filter Selection
• A Measurement of the Hubble Constant using Gravitational Waves from the Binary Merger GW190814
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• On using inspiralling supermassive binary black holes in the PTA frequency band as standard sirens to constrain dark energy
• Realistic observing scenarios for the next decade of early warning detection of binary neutron stars
• Target of Opportunity Observations Detectability of Kilonovae with WFST
• The luminosity functions of kilonovae from binary neutron star mergers under different equation of states
• On the equation of motion of compact binaries in Post-Newtonian approximation
• Multi-messenger astronomy with a Southern-Hemisphere gravitational-wave observatory
• The electromagnetic and gravitational-wave radiations of X-ray transient CDF-S XT2

Cited by in corpus (8)

• Model-independent $H_0$ within FLRW: Joint constraints from GWTC-3 standard sirens and strong lensing time delays
• 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
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• 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
• Influence of cosmic expansion on gravitational waveforms
• Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies
• Gravitational-wave standard sirens and application in cosmology