The purpose of this project is to verify different conditions to see under which a WR star can efficiently be spun up by tides to achieve high-spinning BH remnants.
- The code itself is based on a series of tasks given to me as worksheets, with the functions, ODE_solver and plot_utils files being intended for future, unrelated use as well.
- The MAIN, main_worksheet and all "testing" files are trial files which will not be updated regularly, but the calculations written in them may be reused.
- main_condition_checker is intended to output a csv file with all initial data that fullfils the condition(s) currently being verified.
- main_eq_plots serves as a direct plotter of the data provided by main_condition_checker.
- main_worksheet_population_study and main_worksheet_BH_binary are the subsequent tasks of the worksheet, which focus on the dimentionless spin parameter and the effective spin.
- the newer files (all_ok, freq_ok, freq_ok_redo and their variants) are all files in which I will work on each specific case.
- PCA is self-explanatory