Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
The detection of gravitational waves has brought to light a population of binary black holes that merge within a Hubble time. Multiple formation channels can contribute to this population, making it difficult to definitively associate particular population features with underlying stellar physics. B...
| Published in: | The Astrophysical Journal |
|---|---|
| Main Authors: | , , , , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adf4c6 |
