Table 1
Results and comparisons.
| Ref. | Theory | Method | C.L. | α0 × 103 | (1 − γ) × 105 | η × 105 | ωBD |
|---|---|---|---|---|---|---|---|
| This work | BD (η = 0) | INPOP | 99.7% | ‖1 − γ‖ < 2.50 | |||
| MCMC | 95 % | ‖1 − γ‖ < 2.40 | |||||
| 66.7% | ‖1 − γ‖ < 1.73 | ||||||
| This work | BD | INPOP | 99.7 % | <3.762 | ‖1 − γ‖ < 2.83 | ‖η‖ < 2.83 | > 35,382 |
| BD | MCMC | 95 % | <3.675 | ‖1 − γ‖ < 2.70 | |||
| 66.7% | <3.096 | ‖1 − γ‖ < 1.92 | |||||
| Bernus et al. (2022) | Dilaton | INPOP | 99.7 % | <0.237 | <0.0112 | ||
| Cost function | |||||||
| Bertotti et al. (2003) | PPN | Cassini SC | 1−σ | (−2.1 ± 2.3) | |||
| 66.7 % | ‖1 − γ‖ < 4.4 | ||||||
| Genova et al. (2018) | PPN wo Eq. (15) | MSG | 1−σ | Fixed | (−5.48 ± 7.3) | ||
| w Eq. (15) | 1−σ | Fixed | (−6.65 ± 7.2) | ||||
| Viswanathan et al. (2018) | PPN | LLR | 3−σ | 0 | ‖η‖ < 30 | ||
| Voisin et al. (2020) | BD | Pulsars | 95% | <1.9 | <0.76 | <0.76 | >[1.3−1.4] × 105 |
Notes. The first column gives the references of the published values where Cols. 2–4 give the theoretical background, the method, and the confidence level used for the publication, respectively. Finally, the last four columns give the obtained values corresponding to the following parameters: α0, (1 − γ), η, and ωBD.
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