Buyer Beware: this code is a work in progress
TeukEvolution.jl contains routines to evolve the Teukolsky equation in
a horizon penetrating, hyperboloidally compactified system of coordinates.
There are two choices of initial data.
-
Gaussian pulse initial data.
-
Quasinormal mode initial data. These need to be read in from HDF5 files that are generated with TeukolskyQNMFunctions.jl.
The output is currently saved as .csv files, which stored in columns at
a fixed time (R,Y,value).
We use the 2d plotter in the sci-vis
to visualize code output.
ripley[at]illinois[dot]edu
If you use this code, the best thing to cite right now would be
@article{Ripley:2020xby,
author = "Ripley, Justin L. and Loutrel, Nicholas and Giorgi, Elena and Pretorius, Frans",
title = "{Numerical computation of second order vacuum perturbations of Kerr black holes}",
eprint = "2010.00162",
archivePrefix = "arXiv",
primaryClass = "gr-qc",
doi = "10.1103/PhysRevD.103.104018",
journal = "Phys. Rev. D",
volume = "103",
pages = "104018",
year = "2021"
}