Lowering overshoot_D_min to 10^-2 cm^2/s or below makes MESA model frequencies evolve smoothly for main-sequence stars with growing convective cores.
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Exploring Mixing Thresholds in Asteroseismic Stellar Evolution Models
Lowering overshoot_D_min to 10^-2 cm^2/s or below makes MESA model frequencies evolve smoothly for main-sequence stars with growing convective cores.