Three observational differences for binary black holes detections with second- and third-generation gravitational-wave detectors
Advanced gravitational-wave observatories, such as LIGO and Virgo, will detect hundreds of gravitational-wave signals emitted by binary black holes in the next few years. The collection of detected sources is expected to have certain properties. It is expected that a selection bias will exist toward...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society,
2017-02-14T21:13:35Z.
|
| Subjects: | |
| Online Access: | Get fulltext |