Inlists for the paper "Mixed-mode coupling in the Red Clump: I. Standard single star models"

This repository contains the inlists and run_star_extras used for the paper  "Mixed-mode coupling in the Red Clump: I. Standard single star models" by Walter E. van Rossem, Andrea Miglio, and Josefina Montalban for use with MESA-11701. The grid cycles through masses first (0.7, 1.0, 1.5, 2.3, 3.0 msol) and then metallicity ([Fe/H] = -1.0, -0.5, 0.0, 0.25, 0.4).

Runs 0000-0004 have initial [Fe/H] = -1.0 and masses 0.7, 1.0, 1.5, 2.3, 3.0 solar masses respectively. The next five runs (0005-0009) have [Fe/H] = -0.5 and the same order of masses, and so on.

The previous version had an error in the calculation for the non-parallel approximation and was missing a squareroot in the subroutine calc_dlnc_ds_s0_part_ap when calculating Nred_km1 and Nred_k.