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Table A.1

The Li yield grid and the effect of IGW mixing on Li yield.

Z Mass/M YLi (IGW)/M YLi (no IGW)/M YLi (IGW-no IGW)/M
0.014 3.5 −5.1 × 10−9 −6.1 × 10−9 1.0× 10−9
0.014 4.0 1.2 × 10−8 −4.7 × 10−11 1.2× 10−8
0.014 4.5 1.9× 10−8 6.6 × 10−9 1.2× 10−9
0.014 5.0 5.3 × 10−9 1.4× 10−9 3.9 × 10−9
0.014 5.5 3.4× 10−9 1.1× 10−9 2.3 × 10−9
0.014 6.0 5.1 × 10−9 1.6× 10−9 3.5 × 10−9
0.014 6.5 1.4× 10−8 8.1 × 10−9 7.1 × 10−9
0.014 7.0 4.4× 10−8 3.1 × 10−8 1.3× 10−8
0.014 7.5 1.0× 10−7 9.7 × 10−8 3.3 × 10−9
0.004 3.5 1.3× 10−8 5.5 × 10−9 8.6 × 10−9
0.004 4.0 1.5× 10−8 8.2× 10−9 7.1 × 10−9
0.004 4.5 7.2× 10−9 5.3 × 10−9 1.9× 10−9
0.004 5.0 4.9× 10−9 3.6 × 10−9 1.3× 10−9
0.004 5.5 8.2× 10−9 6.1 × 10−9 2.1 × 10−9
0.004 6.0 6.6× 10−9 5.6 × 10−9 9.8 × 10−10
0.004 6.5 3.9× 10−8 3.8 × 10−8 9.2× 10−10
0.004 7.0 1.5× 10−7 1.5× 10−7 3.2× 10−9
0.004 7.5 2.8 × 10−10 7.1 × 10−10 −4.3 × 10−10
0.0014 3.5 2.2× 10−8 1.5× 10−8 6.9 × 10−9
0.0014 4.0 9.4× 10−9 6.5 × 10−9 2.9 × 10−9
0.0014 4.5 4.7× 10−9 3.4× 10−9 1.3× 10−9
0.0014 5.0 2.9× 10−9 2.2× 10−9 7.1 × 10−10
0.0014 5.5 2.5 × 10−9 2.2× 10−9 2.9× 10−10
0.0014 6.0 4.9× 10−9 4.6 × 10−9 3.2× 10−10
0.0014 6.5 6.2× 10−8 5.8 × 10−8 3.9 × 10−9
0.0014 7.0 3.9 × 10−10 5.9× 10−10 −2.0 × 10−10
0.0014 7.5 −6.1 × 10−10 3.9× 10−11 −6.5 × 10−10
0.00014 3.5 1.8× 10−8 1.2× 10−8 6.1 × 10−9
0.00014 4.0 9.6× 10−9 3.2× 10−9 6.4× 10−9
0.00014 4.5 5.7× 10−9 2.3 × 10−9 3.4× 10−9
0.00014 5.0 8.4× 10−10 6.1 × 10−10 2.3 × 10−10
0.00014 5.5 −8.4 × 10−10 −6.1 × 10−10 −2.3 × 10−10
0.00014 6.0 2.7× 10−9 7.4× 10−9 −4.7 × 10−9
0.00014 6.5 5.7× 10−8 7.2× 10−8 −1.5 × 10−8
0.00014 7.0 −1.3 × 10−9 2.3 × 10−10 −1.1 × 10−9
0.00014 7.5 3.2× 10−8 1.2× 10−7 −8.7 × 10−8

Notes. Li yields YLi (M) produced by the intermediate-mass AGB stars with different metallicities (the first column) and initial masses (the second column) for the models with and without IGW mixing. Li yields represent the net contribution of Li to the ISM after subtracting the initial Li mass inherited from the ISM. The third column represent Li yield with IGW mixing, which the forth column represent Li yield without IGW mixing. The last column corresponds to the third column minus the forth column.

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