Intrinsic selection biases of ground-based gravitational wave searches for high-mass BH-BH mergers
arXiv:1007.4213 · doi:10.1103/PhysRevD.82.104006
Abstract
The next generation of ground-based gravitational wave detectors may detect a few mergers of comparable-mass M\simeq 100-1000 Msun ("intermediate-mass'', or IMBH) spinning black holes. Black hole spin is known to have a significant impact on the orbit, merger signal, and post-merger ringdown of any binary with non-negligible spin. In particular, the detection volume for spinning binaries depends significantly on the component black hole spins. We provide a fit to the single-detector and isotropic-network detection volume versus (total) mass and arbitrary spin for equal-mass binaries. Our analysis assumes matched filtering to all significant available waveform power (up to l=6 available for fitting, but only l<= 4 significant) estimated by an array of 64 numerical simulations with component spins as large as S_{1,2}/M^2 <= 0.8. We provide a spin-dependent estimate of our uncertainty, up to S_{1,2}/M^2 <= 1. For the initial (advanced) LIGO detector, our fits are reliable for (). In the online version of this article, we also provide fits assuming incomplete information, such as the neglect of higher-order harmonics. We briefly discuss how a strong selection bias towards aligned spins influences the interpretation of future gravitational wave detections of IMBH-IMBH mergers.
arXiv comment18 pages, 15 figures, accepted by PRD. v2 is version accepted for publication, including minor changes in response to referee feedback and updated citations
References in corpus (46)
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Evolutions in 3D numerical relativity using fixed mesh refinement
- Measuring gravitational waves from binary black hole coalescences: I. Signal to noise for inspiral, merger, and ringdown
- Matching post-Newtonian and numerical relativity waveforms: systematic errors and a new phenomenological model for non-precessing black hole binaries
- A template bank for gravitational waveforms from coalescing binary black holes: non-spinning binaries
- Phenomenological template family for black-hole coalescence waveforms
- Detector Description and Performance for the First Coincidence Observations between LIGO and GEO
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Stellar-mass black holes in star clusters: implications for gravitational wave radiation
- Spin-Orbit Misalignment in Close Binaries with Two Compact Objects
- On the final spin from the coalescence of two black holes
- Predicting the direction of the final spin from the coalescence of two black holes
- Gravitational recoil from spinning binary black hole mergers
- Simulations of Binary Black Hole Mergers Using Spectral Methods
- High-spin binary black hole mergers
- Modeling kicks from the merger of generic black-hole binaries
- Unequal Mass Binary Black Hole Plunges and Gravitational Recoil
- Effective-one-body waveforms calibrated to numerical relativity simulations: coalescence of non-precessing, spinning, equal-mass black holes
- The final spin from the coalescence of aligned-spin black-hole binaries
- The Total Merger Rate of Compact Object Binaries In The Local Universe
- Binary compact object coalescence rates: The role of elliptical galaxies
- Mergers of nonspinning black-hole binaries: Gravitational radiation characteristics
- Binary Black Holes: Spin Dynamics and Gravitational Recoil
- Circularization and Final Spin in Eccentric Binary Black Hole Inspirals
- Zoom-Whirl Orbits in Black Hole Binaries
- Comparisons of eccentric binary black hole simulations with post-Newtonian models
- Kranc: a Mathematica application to generate numerical codes for tensorial evolution equations
- Comparison of Numerical and Post-Newtonian Waveforms for Generic Precessing Black-Hole Binaries
- Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
- Characteristic extraction in numerical relativity: binary black hole merger waveforms at null infinity
- Binary black hole late inspiral: Simulations for gravitational wave observations
- Observing IMBH-IMBH Binary Coalescences via Gravitational Radiation
- Matched Filtering of Numerical Relativity Templates of Spinning Binary Black Holes
- Black Hole Spin-Orbit Misalignment in Galactic X-ray Binaries
- Superkicks in Hyperbolic Encounters of Binary Black Holes
- Gravitational-wave detectability of equal-mass black-hole binaries with aligned spins
- Relativistic Mergers of Supermassive Black Holes and their Electromagnetic Signatures
- Binary black hole merger: symmetry and the spin expansion
- Final spins from the merger of precessing binary black holes
- Modelling the final state from binary black-hole coalescences
- Dynamical Interactions and the Black Hole Merger Rate of the Universe
- The spin expansion for binary black hole merger: new predictions and future directions
- Statistical studies of Spinning Black-Hole Binaries
- Final Mass and Spin of Merged Black Holes and the Golden Black Hole
- Advances in Simulations of Generic Black-Hole Binaries
- Numerical Relativity meets Data Analysis: Spinning Binary Black Hole Case
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- Spin orientations of merging black holes formed from the evolution of stellar binaries
- Observing gravitational-wave transient GW150914 with minimal assumptions
- Reconstructing phenomenological distributions of compact binaries via gravitational wave observations
- Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescence
- Gravitational-wave astrophysics with effective-spin measurements: asymmetries and selection biases
- Efficient asymptotic frame selection for binary black hole spacetimes using asymptotic radiation
- A Parameter Estimation Method that Directly Compares Gravitational Wave Observations to Numerical Relativity
- Comparing gravitational waves from nonprecessing and precessing black hole binaries in the corotating frame
- Multi-mode black hole spectroscopy
- Impact of Higher-order Modes on the Detection of Binary Black Hole Coalescences
- Search for Gravitational Waves from Intermediate Mass Binary Black Holes
- Precession during merger 1: Strong polarization changes are observationally accessible features of strong-field gravity during binary black hole merger
- Digging the population of compact binary mergers out of the noise
- Systematic challenges for future gravitational wave measurements of precessing binary black holes
- Is J enough? Comparison of gravitational waves emitted along the total angular momentum direction with other preferred orientations
- Are stellar--mass binary black hole mergers isotropically distributed?