# FILE STRUCTURE

This directory includes the results and analysis tools for two papers by Issa+2025 <i>Impact of 3D macro physics and nuclear physics on the</i> p <i>nuclei in O-C shell mergers</i> and <i>3D Macro Physics and Light Odd-Z Element Production in O-C Shell Mergers: Implications for $^{40}\mathrm{K}$ production and radiogenic heating inventories of rocky exoplanets</i>.

The file structure is as follows:
1. RUNS
2. MULTIZONE_MC_RUNS
3. CONDITIONS
4. ANALYSIS

In RUNS directory, all multizone runs have their out and surf files.
All runs with the prefix PPM are the 3D-inspired runs (eg. PPM3 --> 3x3D-inspired).
The ingestion rate is written in terms of $10^{27}$ g/s instead of $\mathrm{M_\odot}$/s (eg. $4\times 10^{-3}~\mathrm{M_\odot s^{-1}}$ --> hif7.95E+03)
The data is organized by RUN_NAME/INGESTION_RATE.
In addition the runs all have flux_runs which have the fixed_fluxes needed for the reaction flux plots.
The GOSH_RUNS are organized by the dip strength and does not have a flux_run (just use another run's fluxes because they should be identical).

In MULTIZONE_MC_RUNS, there are the final surf files for the Monte Carlo runs for the five mixing cases considered.
There are also the variation files that are needed to perform the correlation study.

In CONDITIONS are the initial and ingested mass fractions used for this work.

Finally, in ANALYSIS are the notebooks used to calculate the results and produce the figures in each paper.