Breaking away from the near horizon of extreme Kerr
We study gravitational perturbations around the near horizon geometry of the (near) extreme Kerr black hole. By considering a consistent truncation for the metric fluctuations, we obtain a solution to the linearized Einstein equations. The dynamics is governed by two master fields which, in the c...
| Main Author: | |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
SciPost
2020-06-01
|
| Series: | SciPost Physics |
| Online Access: | https://scipost.org/SciPostPhys.8.6.089 |