Description
Abstract: This tutorial provides a hands-on introduction to computing leading-order selfforce
fluxes and gravitational waveforms. Participants will work with two opensource
libraries—the Mathematica-based Black Hole Perturbation Toolkit and the
Python-based pybhpt—to generate fluxes and waveforms for quasi-circular and
eccentric binaries. (It is recommended that participants either have Jupyter/Python
and Mathematica installed on their machine or access to Google Collab and
Wolfram Cloud, if they wish to run the notebooks during the tutorial.)
