Precise LIGO lensing rate predictions for binary black holes
We show how LIGO is expected to detect coalescing binary black holes at z>1 that are lensed by the intervening galaxy population. Gravitational magnification, μ, strengthens gravitational-wave signals by √μ without altering their frequencies, which if unrecognized leads to an underestimate of the...
| Hlavní autoři: | , , , |
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| Další autoři: | |
| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
American Physical Society
2018
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| On-line přístup: | http://hdl.handle.net/1721.1/114520 |