When the stars don't align: Investigating inconsistencies in binary black hole formation across population synthesis codes
astro-ph.HE, astro-ph.GA, astro-ph.SR
Submitted: 2026-08-21
Updated: 2026-09-21
Comments: 40 pages, 22 figures, 1 table. Submitted to ApJ
Code: https://github.com/POSYDON-code/POSYDON
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- A Stellar Role Reversal: Multiple Features in the Mass and Mass Ratio Distributions of Merging Binary Black Holes from Stable Mass Transfer
- Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis
- How Common Are Common Envelopes? Quantifying Their Role in Forming Gravitational-Wave Sources
- Propagating Uncertainties from Nuclear Physics to Gamma-rays in Core Collapse Supernovae
- Twin Peaks: Resolving Features in the Binary Black Hole Mass Function with COSMIC-METISSE
- The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity
- Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions
- Wide-Field InfraRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA Final Report
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- GWTC-5.0: 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
- Binary neutron star populations across cosmic time: the impact of binary stellar evolution uncertainties
- Streamlining and standardizing software citations with The Software Citation Station
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