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Table A.2.

Relevant information of each isotope case discussed in Sect. 3.1.

Isotope Branching Decay Daughter λSet 0 ne λ Set 1 90 MK $ \lambda^{\mathrm{90\,MK}}_{\mathrm{Set\,1}} $ λ Set 1 300 MK $ \lambda^{\mathrm{300\,MK}}_{\mathrm{Set\,1}} $ Direction Relevance
isotope mode nucleus (s−1) (1026 cm−3) (s−1) (s−1) of change
64Ni stable stable stable Compare to stardust
63Ni β 63Cu 2.2 × 10−10 1 5.2 × 10−10 1.8 × 10−9 SiC grain data
9.5 3.8 × 10−10 1.7 × 10−9
64Cu β+ 64Ni 9.2 × 10−6 1 3.2 × 10−6 2.7 × 10−6
9.5 5.8 × 10−6 3.2 × 10−6
β 64Zn 5.9 × 10−6 1 6.3 × 10−6 6.4 × 10−6
9.5 6.1 × 10−6 6.3 × 10−6

80Kr stable stable stable Compare to stardust
81Kr ϵ 81Br 9.6 × 10−14 1 1.6 × 10−14 1.6 × 10−12 SiC grain data
9.5 6.4 × 10−14 4.1 × 10−11
79Se β 79Br 7.4 × 10−14 1 2.7 × 10−12 1.3 × 10−8
9.5 2.3 × 10−12 1.3 × 10−8
80Br β 80Kr 6.0 × 10−4 1 5.9 × 10−4 3.9 × 10−4
β+ 80Se 5.4 × 10−5 1 2.5 × 10−5 1.1 × 10−5
9.5 4.7 × 10−5 1.3 × 10−5

94Mo stable stable stable p-only
93Zr β 93Nb 1.4 × 10−14 1 2.6 × 10−14 6.6 × 10−14 Determine its s-process
9.5 2.0 × 10−14 6.2 × 10−14 contribution
94Nb β 94Mo 1.1 × 10−12 1 2.5 × 10−8 9.3 × 10−7 Compare to stardust
9.5 2.4 × 10−8 9.3 × 10−7 SiC grain data

108Cd stable stable stable p-only
107Pd β 107Ag 3.4 × 10−15 1 1.2 × 10−14 3.1 × 10−11 Determine its s-process
9.5 7.8 × 10−15 2.9 × 10−11 contribution
108Ag β 108Cd 4.7 × 10−3 1 4.9 × 10−3 4.2 × 10−3
β+ 108Pd 1.4 × 10−4 1 7.5 × 10−5 1.3 × 10−5
9.5 1.4 × 10−4 2.4 × 10−5

129I β 129Xe 1.4 × 10−15 1 2.4 × 10−9 4.5 × 10−8 r-only
9.5 1.9 × 10−9 4.1 × 10−8 Short-lived
128I β 128Xe 4.3 × 10−4 1 4.2 × 10−4 2.8 × 10−4 radionuclide
9.5 4.2 × 10−4 2.8 × 10−4

152Gd α 148Sm stable stable stable p-only
151Sm β 151Eu 2.4 × 10−10 1 5.0 × 10−10 9.5 × 10−9 Determine its s-process
9.5 3.4 × 10−10 8.0 × 10−9 contribution
152Eu ϵ 152Sm 1.2 × 10−9 1 6.9 × 10−9 1.8 × 10−7
9.5 7.8 × 10−9 1.1 × 10−6
β 152Gd 4.5 × 10−10 1 3.2 × 10−8 4.3 × 10−5
9.5 3.2 × 10−8 4.2 × 10−5

176Hf stable stable stable Both are s-only
176Lu β 176Hf 5.8 × 10−19 1 1.3 × 10−12 1.3 × 10−7
9.5 1.3 × 10−12 1.4 × 10−7

182Hf β 182Ta 2.5 × 10−15 1 7.4 × 10−14 1.2 × 10−9 Short-lived
9.5 6.8 × 10−14 8.9 × 10−10 radionuclide

205Pb ϵ 205Tl 1.3 × 10−15 1 1.7 × 10−9 3.1 × 10−10 ↓a Single s-only
9.5 6.4 × 10−9 1.9 × 10−9 short-lived
204Tl β 204Pb 5.6 × 10−9 1 6.3 × 10−9 1.3 × 10−6 radionuclide
9.5 6.3 × 10−9 1.2 × 10−6
205Tl βb 204Pb stable 1 1.1 × 10−12 6.1 × 10−8
9.5 1.9 × 10−17 2.0 × 10−8

Notes. Columns indicate the corresponding isotope (Col. 1), the branching isotopes (Col. 2) that affect its abundance, their decay modes, daughter nuclei, and decay rates (Col. 3-8). λSet 0 indicates the decay rate used in the Set 0 models from JINA reaclib, while λ Set 1 90 MK $ \lambda^{\mathrm{90\,MK}}_{\mathrm{Set\,1}} $ and λ Set 1 300 MK $ \lambda^{\mathrm{300\,MK}}_{\mathrm{Set\,1}} $ indicate the value of the T-dependent rate at 90 and 300 million K, respectively. The decay rate values are given for two different electron number densities, if available in the NETGEN database. The direction in which the abundance of each isotope has changed in the Set 1 models compared to the Set 0 models and the relevance of each case are shown in Cols. 9 and 10, respectively.

a

Except for the M = 4 MZ = 0.007 model.

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