Test the long-term stability of convective-reactive layer classifications
Determine whether the Type I–V convective-reactive layer classification remains unchanged on timescales substantially longer than those covered by the simulated oxygen–neon shell merger.
References
Whether the classification remains unchanged on timescales considerably longer than those simulated here cannot be assessed with the present data and requires longer simulations.
— Structure of Convective-Reactive Zone in a Supernova Progenitor
(2610.01239 - Mocak et al., 1 Oct 2026) in Section 3.13, Subsection “Robustness of observed layering”