Shaping binary black hole merger efficiency with gravitational wave observations
astro-ph.HE, astro-ph.CO
Submitted: 2026-09-29
Updated: 2026-09-29
Code: https://github.com/sterinaldi/FIGARO
Terminology
Sources
- From cosmological simulations to binary black hole mergers: The impact of using analytical star formation history models on gravitational-wave source populations
- Intermediate-mass black hole seeding in galactic nuclei from star cluster migration
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion