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Table 5.
Sensitive: species most impacted by the modification of individual weak rates.
| [AZ/56Fe](a) | influencers and Di, j | |
|---|---|---|
| 4He | −7.2 | 55Fe (0.40); 54Mn (0.34); 56Co (0.34); 56Ni (-0.07) |
| 48Ca | −3.7 | 57Fe (0.50); 55Mn (0.44); 54Mn (0.42); 56Fe (0.42); 55Fe (0.34); 58Co (0.20); 56Mn (0.18); 57Co (0.17); 54Fe (0.16); 61Ni (0.15) |
| 50Ti | 0.47 | 56Fe (0.09); 54Mn (0.09); 55Fe (0.09); 57Fe (0.09); 55Mn (0.07); 58Co (0.04) |
| 54Cr | 0.87 | 55Fe (0.07); 56Fe (0.07); 54Mn (0.06); 57Fe (0.06); 55Mn (0.04) |
| 58Fe | 0.34 | 55Fe (0.06); 56Fe (0.05); 54Mn (0.04) |
| 58Ni | −0.16 | 56Ni (0.04) |
| 61Ni | −1.3 | 55Fe (0.12); 54Mn (0.09); 56Co (0.08) |
| 62Ni | −0.09 | 55Fe (0.06) |
| 64Ni | −1.1 | 57Fe (0.22); 54Mn (0.20); 56Fe (0.20); 55Mn (0.19); 55Fe (0.17); 58Co (0.10); 57Co (0.08); 54Fe (0.08); 56Mn (0.07); 61Ni (0.07) |
| 64Zn | −2.1 | 55Fe (0.04) |
| 67Zn | −2.5 | 57Fe (0.05) |
Notes. Listed are those species for which |Di, j| ≥ 0.045.
(a)
[AZ/56Fe]=log[n(AZ)/n⊙(AZ)] − log[n(56Fe)/n⊙(56Fe)], with n(AZ) the number fraction of isotope AZ in the supernova ejecta, and n⊙(AZ) its abundance in the solar system (Lodders 2003)
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