Observable signatures of extreme mass-ratio inspiral black hole binaries embedded in thin accretion disks
We examine the electromagnetic and gravitational wave (GW) signatures of stellar-mass compact objects (COs) spiraling into a supermassive black hole (extreme mass-ratio inspirals), embedded in a thin, radiation-pressure dominated, accretion disk. At large separations, the tidal effect of the seconda...
| Main Authors: | , , |
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| Other Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society,
2011-12-01T19:57:25Z.
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| Subjects: | |
| Online Access: | Get fulltext |