Excitation of Kerr quasinormal modes in extreme-mass-ratio inspirals
If a small compact object orbits a black hole, it is known that it can excite the black hole's quasinormal modes (QNMs), leading to high-frequency oscillations (“wiggles”) in the radiated field at J^{+}, and in the radiation-reaction self-force acting on the object after its orbit passes throug...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
American Physical Society
2020-03-01
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| Series: | Physical Review Research |
| Online Access: | http://doi.org/10.1103/PhysRevResearch.2.013365 |