inlist file 4

Evolution from photo number 616 to "pre-SN" with surface_tau_factor again adjusted to increase performance and avoid convergence/small time-step issues. In this work, as "pre-SN" we consider the case when a significant part of the star's core enters the dynamically unstable Gamma<4/3 pair-formation region at which point the models were mapped to a hydrodynamics code in the original work.

inlist_80M_sch_rotmag05crit_3 — Octet Stream, 14 kB (14834 bytes)