Properties of the Binary Black Hole Merger GW150914

Abstract

On September 14, 2015, the Laser Interferometer Gravitational-wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity. GW150914 was produced by a nearly equal mass binary black hole of $36_{-4}^{+5}{M}_{\odot }$ and $29_{-4}^{+4}{M}_{\odot }$; for each parameter we report the median value and the range of the 90% credible interval. The dimensionless spin magnitude of the more massive black hole is bound to be $<0.7$ (at 90% probability). The luminosity distance to the source is $410_{-180}^{+160}$ Mpc, corresponding to a redshift $0.09_{-0.04}^{+0.03}$ assuming standard cosmology. The source location is constrained to an annulus section of $610$ deg${}^2$, primarily in the southern hemisphere. The binary merges into a black hole of $62_{-4}^{+4}{M}_{\odot }$ and spin $0.67_{-0.07}^{+0.05}$. This black hole is significantly more massive than any other inferred from electromagnetic observations in the stellar-mass regime.

19 pages, 6 figures

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• Characterization of low-significance gravitational-wave compact binary sources
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• Overcharging process around a magnetized black hole: Can the backreaction effect of magnetic field restore cosmic censorship conjecture?
• Gravitational Waves with Orbital Angular Momentum
• New Effects in Gravitational Waves and Memory
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• Radiation properties of the accretion disk around a black hole in Einstein-Maxwell-scalar theory
• Critical phenomena of charged Einstein-Gauss-Bonnet black holes with charged scalar hair
• Numerical Relativity and High Energy Physics: Recent Developments
• Parameter estimates in binary black hole collisions using neural networks
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• Constructive summation of the (2,2) quasi normal mode from a population of black holes
• Systematic calibration error requirements for gravitational-wave detectors via the Cramér-Rao bound
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• Wolf-Rayet stars, black holes and the first detected gravitational wave source
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• Constraining exotic compact stars composed of bosonic and fermionic dark matter with gravitational wave events
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• Newly Discovered Wolf-Rayet Stars in M31
• Measuring Black Hole Spins through X-ray Reflection Spectroscopy and the Relativistic Precession Model: the case of XTE J1859+226
• Gravitational waveforms for high spin and high mass-ratio binary black holes: A synergistic use of numerical-relativity codes
• Primordial Black Hole-Neutron Star Merger Rate in Modified Gravity
• Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Free-falling test particles in a charged Kalb-Ramond black hole: gravitational Doppler effect and tidal forces
• The Jiao Tong University Spectroscopic Telescope Project
• Bound on photon circular orbits in general relativity and beyond
• The spin rates of O stars in WR + O Magellanic Cloud binaries
• Bowen-York Type Initial Data for Binaries with Neutron Stars
• On tests of general relativity with binary radio pulsars
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• Compact stars in the Einstein dark energy model
• Efficient simulations of high-spin black holes with a new gauge
• Computational Techniques for Parameter Estimation of Gravitational Wave Signals
• Estimation of the gravitational wave polarizations from a non template search
• Ringdown Spectroscopy of Rotating Black Holes Pierced by Cosmic Strings
• Gravitational wave extraction in higher dimensional numerical relativity using the Weyl tensor
• Collision of Two Rotating Hayward Black Holes
• Observational test of ${\mathcal{R}}^2$ spacetimes with the S2 star in the Milky Way galactic center
• Parameterized and Consistency Tests of Gravity with Gravitational Waves: Current and Future
• Gravitational Wave Measurement in the Mid-Band with Atom Interferometers
• Bayesian Inference Analysis of Unmodelled Gravitational-Wave Transients
• Poynting-Robertson effect as a dissipative system in general relativity
• Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits
• RATIR Followup of LIGO/Virgo Gravitational Wave Events
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Retesting the no-hair theorem with GW150914
• The Design Strain Sensitivity of the Schenberg Spherical Resonant Antenna for Gravitational Waves
• How to confirm the existence of population III stars by observations of gravitational waves
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• Constraining the topological Gauss-Bonnet coupling from GW150914
• Probing Reheating Phase via Non-Helical Magnetogenesis and Secondary Gravitational Waves
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Black Hole Mass Function of Coalescing Neutron Star-Black Hole Binary Systems: The Prospect of Reconstruction with the Gravitational Wave Observations
• Constraining neutron star radii in black hole-neutron star mergers from their electromagnetic counterparts
• AEther as an Inevitable Consequence of Quantum Gravity
• Impact of calibration uncertainties on Hubble constant measurements from gravitational-wave sources
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• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• A regular metric does not ensure the regularity of spacetime
• Thermodynamics of the Weyl Geometric Gravity Black Holes
• Hypercompact stellar clusters: morphological renditions and spectro-photometric models
• Axisymmetric Hydrodynamics in Numerical Relativity Using a Multipatch Method
• Gravitational Wave Signatures from Periodic Orbits around a non-commutative inspired black hole surrounded by quintessence
• Testing black holes in a perfect fluid dark matter environment using quasinormal modes
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• The potential of advanced ground-based gravitational wave detectors to detect generic deviations from general relativity
• Gravitational waves from inspiralling compact binaries in conformal gravity
• Black holes and nilmanifolds: quasinormal modes as the fingerprints of extra dimensions?
• On similarity of binary black hole gravitational-wave skymaps: to observe or to wait?
• Quasinormal modes of gravitational perturbation for uniformly accelerated black holes
• Sunyaev-Zel'dovich anisotropy due to Primordial black holes
• Population and spectral synthesis: it doesn't work without binaries
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Recent LIGO-Virgo discoveries
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• Gravitational Wave Searches for Aligned-Spin Binary Neutron Stars Using Nonspinning Templates
• Efficiency of nonspinning templates in gravitational wave searches for aligned-spin binary black holes
• Taming systematics in distance and inclination measurements with gravitational waves: role of the detector network and higher-order modes
• Linearized Field Equations and Extra Force in $f(R,{\mathbf{T}}^{(n)})$ Extended Gravity
• Mesoscopic Quantum Thermo-mechanics: a new frontier of experimental physics
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• Exploring the cosmic censorship conjecture with a Gauss-Bonnet sector
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• Observations of red giants with suspected massive companions
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• Beyond Whittle: Nonparametric correction of a parametric likelihood with a focus on Bayesian time series analysis
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• GW170814: Gravitational wave polarization analysis
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• Coalescence of Kerr Black Holes: Binary Systems from GW150914 to GW170814
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