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A Package to Compute mode functions for Kerr Black Hole Quasinormal modes, as well as their frequencies, seperation constants and more. Additionally provides an interface for cheap differentiation of such modes.
The purpose of this study is to investigate if it is possible to anticipate the key outcomes of a BPS simulation given a set of initial variables using machine learning techniques.
A Package to Compute wave functions for Kerr Black Hole Quasinormal modes, as well as their frequencies, seperation constants and more. Additionally provides an interface for cheap differentiation of such modes.
This repository contains computational material developed/utilized in Miller-Jones et al. 2021 to estimate the mass of the black hole in the X-ray binary Cygnus X-1.