Tracking black hole kicks from gravitational wave observations

Abstract

Coalescing binary black holes emit anisotropic gravitational radiation. This causes a net emission of linear momentum that produces a gradual acceleration of the source. As a result, the final remnant black hole acquires a characteristic velocity known as recoil velocity or gravitational kick. The symmetries of gravitational wave emission are reflected in the interactions of the gravitational wave modes emitted by the binary. In this work we make use of the rich information encoded in the higher-order modes of the gravitational wave emission to infer the component of the kick along the line-of-sight (or \textit{radial kick}). We do this by performing parameter inference on simulated signals given by numerical relativity waveforms for non-spinning binaries using numerical relativity templates of aligned-spin (non-precessing) binary black holes. We find that for suitable sources, namely those with mass ratio $q\ge 2$ and total mass $M\sim 100M_{\odot }$, and for modest radial kicks of $120km/s$, the $90\%$ credible intervals of our posterior probability distributions can exclude a zero kick at a signal-to-noise ratio of $15$; using a single Advanced LIGO detector working at its early sensitivity. The measurement of a non-zero radial kick component would provide the first observational signature of net transport of linear momentum by gravitational waves away from their source.

arXiv comment6 pages, 5 figures

References in corpus (40)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• Advanced Virgo: a 2nd generation interferometric gravitational wave detector
• 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
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• Tests of general relativity with GW150914
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Characterization of the LIGO detectors during their sixth science run
• GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Properties of the Binary Black Hole Merger GW150914
• Astrophysical Implications of the Binary Black-Hole Merger GW150914
• An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
• Large Merger Recoils and Spin Flips From Generic Black-Hole Binaries
• Maximum gravitational recoil
• Total recoil: the maximum kick from nonspinning black-hole binary inspiral
• Exploring short gamma-ray bursts as gravitational-wave standard sirens
• Model Waveform Accuracy Standards for Gravitational Wave Data Analysis
• Consequences of gravitational radiation recoil
• Distinguishing Spin-Aligned and Isotropic Black Hole Populations With Gravitational Waves
• First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries
• A Numerical Relativity Waveform Surrogate Model for Generically Precessing Binary Black Hole Mergers
• Hangup Kicks: Still Larger Recoils by Partial Spin/Orbit Alignment of Black-Hole Binaries
• Exploring black hole superkicks
• Georgia Tech Catalog of Gravitational Waveforms
• An improved analysis of GW150914 using a fully spin-precessing waveform model
• Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
• Further insight into gravitational recoil
• The Missing Link: Bayesian Detection and Measurement of Intermediate-Mass Black-Hole Binaries
• Search for intermediate mass black hole binaries in the first observing run of Advanced LIGO
• Impact of gravitational radiation higher order modes on single aligned-spin gravitational wave searches for binary black holes
• Superkicks in Hyperbolic Encounters of Binary Black Holes
• Searching for the full symphony of black hole binary mergers
• Detectability of gravitational waves from binary black holes: Impact of precession and higher modes
• A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
• Black hole kicks as new gravitational wave observables
• Missing black holes in brightest cluster galaxies as evidence for the occurrence of superkicks in nature
• Sensitivity of gravitational wave searches to the full signal of intermediate mass black hole binaries during the LIGO O1 Science Run
• Superkicks in ultrarelativistic encounters of spinning black holes

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