Are merging black holes born from stellar collapse or previous mergers?

Abstract

Advanced LIGO detectors at Hanford and Livingston made two confirmed and one marginal detection of binary black holes during their first observing run. The first event, GW150914, was from the merger of two black holes much heavier that those whose masses have been estimated so far, indicating a formation scenario that might differ from "ordinary" stellar evolution. One possibility is that these heavy black holes resulted from a previous merger. When the progenitors of a black hole binary merger result from previous mergers, they should (on average) merge later, be more massive, and have spin magnitudes clustered around a dimensionless spin ~0.7. Here we ask the following question: can gravitational-wave observations determine whether merging black holes were born from the collapse of massive stars ("first generation"), rather than being the end product of earlier mergers ("second generation")? We construct simple, observationally motivated populations of black hole binaries, and we use Bayesian model selection to show that measurements of the masses, luminosity distance (or redshift), and "effective spin" of black hole binaries can indeed distinguish between these different formation scenarios.

18 pages, 7 figures, 3 tables. Accepted for publication in PRD. Selected as PRD Editors' Suggestion

References in corpus (26)

• X-ray Properties of Black-Hole Binaries
• Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
• Pulsational Pair-Instability Supernovae
• The trouble with $H_0$
• The Evolution of Compact Binary Star Systems
• Double Compact Objects III: Gravitational Wave Detection Rates
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO
• Analysis of spin precession in binary black hole systems including quadrupole-monopole interaction
• Alignment of the spins of supermassive black holes prior to coalescence
• Are LIGO's Black Holes Made From Smaller Black Holes?
• The Masses and Spins of Neutron Stars and Stellar-Mass Black Holes
• Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy
• Remnant mass, spin, and recoil from spin aligned black-hole binaries
• Reconstructing the massive black hole cosmic history through gravitational waves
• Constraining stellar binary black hole formation scenarios with eLISA eccentricity measurements
• Effective potentials and morphological transitions for binary black-hole spin precession
• Low metallicity and ultra-luminous X-ray sources in the Cartwheel galaxy
• Orbital eccentricities in primordial black holes binaries
• Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts and Gravitational Wave Detection
• LISA extreme-mass-ratio inspiral events as probes of the black hole mass function
• Remnant of binary black-hole mergers: New simulations and peak luminosity studies
• Estimating the parameters of non-spinning binary black holes using ground-based gravitational-wave detectors: Statistical errors
• Gravitational waves from BH-NS binaries: Effective Fisher matrices and parameter estimation using higher harmonics
• Constraining properties of the black hole population using LISA
• Three observational differences for binary black holes detections with second and third generation gravitational-wave detectors

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