Table 1
White dwarf evolutionary sequences computed in this work.
| MWD/M⊙ | Gi/G0 | ||
|
|
|||
| Ġ/G = −5 × 10-11 | Ġ/G = −1 × 10-11 | Ġ/G = −1 × 10-12 | |
|
|
|||
| 0.525 | 1.40 (−4.40) | 1.10 (−4.37) | 1.010 (−4.33) |
| 0.525 | 1.30 (−4.20) | 1.05 (−4.05) | 1.005 (−4.00) |
| 0.525 | 1.20 (−4.05) | 1.02 (−3.66) | |
| 0.525 | 1.10 (−3.77) | ||
|
|
|||
| 0.609 | 1.50 (−4.83) | 1.20 (<−5) | 1.100 (<−5) |
| 0.609 | 1.40 (−4.40) | 1.10 (−4.30) | 1.050 (<−5) |
| 0.609 | 1.30 (−4.19) | 1.05 (−4.02) | 1.020 (<−5) |
| 0.609 | 1.20 (−4.02) | 1.02 (−3.60) | |
| 0.609 | 1.10 (−3.68) | ||
|
|
|||
| 1.000 | 1.24 (−4.64) | 1.10 (−4.55) | 1.020 (<−5) |
| 1.000 | 1.20 (−4.12) | 1.05 (−3.68) | 1.010 (−4.30) |
| 1.000 | 1.10 (−3.23) | 1.02 (−3.10) | 1.005 (−3.56) |
Notes. We list the white dwarf stellar mass (in solar units) and, for each value of the rate of change of G, Ġ/G (in units of yr-1), the initial value of G at the beginning of the white dwarf cooling phase, Gi/G0. The numbers in brackets give the stellar luminosity, log (L/L⊙), at which the present value of the gravitational constant, G0, occurs.
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