Here you can find routines to compute the radiation emitted by an extreme-mass-ratio inspiral in spherically-symmetric, non-vacuum black-hole spacetimes. We specialize to the case of a black hole within a halo of matter based on the solution found in arXiv:2109.00005, but you can adapt it to other backgrounds.
EMRIs in Astrophysical Environments
Description |
References |
Download |
|---|---|---|
| Time-domain code |
Zenginoglu and Khanna arXiv:1108.1816 Cardoso + arXiv:2210.01133
|
|
| Frequency-domain code |
Cardoso, Macedo, Pani, Ferrari arXiv:1604.07845 Cardoso + arXiv:2210.01133
|
|