Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins
Veome Kapil, Ilya Mandel, Jeff Riley, Evgeni Grishin, Jim Fuller, Emanuele Berti
astro-ph.HE, gr-qc
Submitted: 2026-06-22
Comments: 23 pages, 16 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Science of the Einstein Telescope
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-4.0: Population Properties of Merging Compact Binaries
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0
- Revising the Spin and Kick Connection in Isolated Binary Black Holes
- On the effective spin-mass ratio relation of binary black hole mergers that evolved in isolation
- Accretion Feedback from newly-formed black holes and its implications for LIGO Sources
- Approximations to the spin of close Black-hole-Wolf-Rayet binaries
- The first decade of gravitational-wave measurements of black hole spins
- The Effects of High-Velocity Supernova Kicks on the Orbital Properties and Sky Distributions of Neutron Star Binaries
- A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
- Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
- Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency
- Differential rotation and magnetic fields in stellar interiors
- Are black hole spins truly near-zero?
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