Superradiant amplification of massless waves scattering off Kerr black holes is an important phenomena in curved spacetime. Details of the process can be found in an outstanding work by Press and Teukolsky (ApJ193, 443 (1974)), but extensive tables and routines to compute them are lacking. We provide here such data. The routines are freely available, but we would appreciate if you refer to the original work.
Amplification Factors Data
Description |
References |
Download |
|---|---|---|
|
Amplification factors of massless fields
|
Brito, Cardoso & Pani |
|
Amplification Factors Routines
Description |
References |
Download |
|---|---|---|
|
Amplification factors of the superradiant
|
Brito, Cardoso & Pani |
|
|
Amplification factors of the superradiant
|
Brito, Cardoso & Pani |
Decoupling of perturbations for spinning stars
Description |
References |
Download |
|---|---|---|
|
Radial coefficients for vector perturbations of stars
|
Cardoso, Pani & Yu |
|