Table 1.
Initial chemical mixture adopted for the different solar calibrated models.
| Model | C | R |
|---|---|---|
| element | ||
| 1H | 7.18 × 10−1 | 7.14 × 10−1 |
| 4He | 2.69 × 10−1 | 2.72 × 10−1 |
| 7Li ( * ) | 1.03 × 10−8 | 1.03 × 10−8 |
| 9Be( † ) | 1.66 × 10−10 | 1.65 × 10−10 |
| 11B | 3.13 × 10−9 | 3.31 × 10−9 |
| 12C | 2.26 × 10−3 | 2.40 × 10−3 |
| 14N | 6.68 × 10−4 | 7.07 × 10−4 |
| 16O | 5.54 × 10−3 | 5.86 × 10−3 |
| 19F | 4.89 × 10−7 | 5.17 × 10−7 |
| 20Ne | 1.58 × 10−3 | 1.68 × 10−3 |
| 23Na | 2.83 × 10−5 | 3.00 × 10−5 |
| 24Mg | 5.35 × 10−4 | 5.66 × 10−4 |
| 27Al | 5.39 × 10−5 | 5.71 × 10−5 |
| 28Si | 5.92 × 10−4 | 6.27 × 10−4 |
| 31P | 5.65 × 10−6 | 5.97 × 10−6 |
| 32S | 2.84 × 10−4 | 3.01 × 10−4 |
| 35Cl | 6.73 × 10−8 | 7.12 × 10−8 |
| Others( * *) | 1.49 × 10−3 | 1.58 × 10−3 |
Notes. Initial abundances are given in mass fraction for the classical model (C) and the rotation model (R). Each model has been calibrated on the Sun (see Table 2). The mass fraction of metals Z is ZC = 0.0134 and ZR = 0.0142 for the classical and rotating calibrated solar models, respectively. ( * )Aini(7Li) = 3.31; ( † )Aini(9Be) = 1.41; ( * *)refers to elements heavier than chlorine.
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