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Table 1.

Selected key results of the stellar evolution models for all the tracks discussed in this section.

|fPDCZ| |fCE| Max Nn τ Split after Max Nn Remerge (a) Final C/O # Pulses after PIE
[cm−3] [mb−1]
0.000 0.000 9.15 × 1014 27.256 n n 19.256 3
0.000 0.016 8.04 × 1014 25.50 n n 20.939 4
0.000 0.128 5.99 × 1014 21.54 n n 19.804 4
0.008 0.000 8.98 × 1013 23.17 y n 8.06 0
0.016 0.000 9.01 × 1013 20.57 n t 6.33 0
0.016 (†) 0.000 9.75 × 1013 22.65 y t 5.93 0
0.032 0.000 1.24 × 1014 18.76 n p 3.976 0
0.008 0.016 1.00 × 1014 22.71 n t 7.858 0
0.008 (†) 0.016 8.42 × 1013 22.65 y t 7.792 0
0.008 0.128 1.32 × 1014 20.20 n t 8.013 0
0.016 0.016 5.6 × 1013 12.28 n t 6.436 0
0.016 (†) 0.016 6.24 × 1013 13.50 y p 6.651 0
0.016 0.128 4.73 × 1013 5.04 n t 7.516 0
0.032 0.016 7.45 × 1013 10.23 n t 4.904 0
0.032 0.128 5.40 × 1013 6.59 n p 5.294 0

Notes.

(a)

Whether the split PDCZ remerges again: n for no, t for temporarily, p for permanently.

(†)

Track run without the geometrical cutoff to the overshoot.

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