Table 3.
Results for various linear combinations of nucleosynthetic processes in the fitting range of 31 ≤ Z ≤ 72.
Process(es) | χ2 | Notes | Process(es) | χ2 | Notes |
---|---|---|---|---|---|
solar | 154.72 | 1 | sm2 + in9 | 66.31 | 3,2 |
in9 | 214.25 | 2 | sm2 + in15 | 51.17 | 3,2 |
in10 | 229.76 | 2 | sm5 + in9 | 59.25 | 5,2 |
in11 | 251.94 | 2 | sm5 + in15 | 74.37 | 5,2 |
in12 | 257.21 | 2 | Solar + in9 | 92.89 | 1,2 |
in13 | 304.40 | 2 | Solar + in10 | 94.82 | 1,2 |
in14 | 463.06 | 2 | Solar + in11 | 101.47 | 1,2 |
in15 | 539.71 | 2 | Solar + in12 | 103.30 | 1,2 |
sm2 | 85.90 | 3 | Solar + in13 | 109.14 | 1,2 |
sm3 | 63.56 | 4 | Solar + in14 | 101.85 | 1,2 |
sm5 | 274.66 | 5 | Solar + in15 | 94.44 | 1,2 |
sm3 + in9 | 63.15 | 4,2 | sm3 + r + in9 | 63.00 | 4,6,2 |
sm3 + in10 | 62.94 | 4,2 | sm3 + r + in10 | 62.80 | 4,6,2 |
sm3 + in11 | 62.77 | 4,2 | sm3 + r + in11 | 62.72 | 4,6,2 |
sm3 + in12 | 61.23 | 4,2 | sm3 + r + in12 | 61.23 | 4,6,2 |
sm3 + in13 | 59.95 | 4,2 | sm3 + r + in13 | 59.92 | 4,6,2 |
sm3 + in14 | 59.71 | 4,2 | sm3 + r + in14 | 59.71 | 4,6,2 |
sm3 + in15 | 54.97 | 4,2 | sm3 + r + in15 | 54.57 | 4,6,2 |
sm3 + r | 63.26 | 4,6 | 2-step i | 50.96 | 7 |
Notes. References and model details: (1): Solar abundances from Lodders (2003); (2) i-process abundances from Hampel et al. (2016), using constant temperatures of T = 0.15 GK and constant densities of ρ = 1600 g cm−3. The respective neutron densities are indicated (as logN [cm−3]) by the subscript; (3): AGB yields for Minit = 2 M⊙, Z = 0.0001 (Lugaro et al. 2012); (4): AGB yields for Minit = 3 M⊙, Z = 0.0001 (Lugaro et al. 2012); (5): AGB yields for Minit = 5 M⊙, Z = 0.0001 (Lugaro et al. 2012); (6): r-process from dynamical ejecta of binary neutron star merger (Korobkin et al. 2012); (7): i-process with two ingestion episodes of τ = 0.30 and 0.96 mbarn−1 (Sect. 5).
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