Salvato in:
| Autori principali: | , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2025
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| Soggetti: | |
| Accesso online: | https://arxiv.org/abs/2508.21541 |
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Sommario:
- We explore the potential variation of two fundamental constants, the fine-structure constant $α$ and the proton-to-electron mass ratio $μ$, within the framework of modified gravity theories and finite-temperature effects. Utilising high-precision white dwarf observations from the Gaia-DR3 survey, we construct a robust mass--radius relation using a Bayesian-inspired machine learning framework. This empirical relation is rigorously compared with theoretical predictions derived from scalar-tensor gravity models and temperature-dependent equations of state. Our results demonstrate that both underlying gravitational theory and temperature substantially influence the inferred constraints on $α$ and $μ$. We obtain the strongest constraints as $|Δα/α|=2.10^{+32.56}_{-39.26}\times10^{-7}$ and $|Δμ/μ|=1.61^{+37.16}_{-34.67}\times10^{-7}$ for modified gravity parameter $γ\simeq -3.69\times10^{13}\,\mathrm{cm}^2$, while for the finite temperature case, these are $|Δα/α|=1.60^{+37.31}_{-35.42}\times10^{-7}$ and $|Δμ/μ|=1.23^{+37.02}_{-35.71}\times10^{-7}$ for $T \simeq 1.1 \times 10^7\rm\, K$. These findings yield tighter constraints than those reported in earlier studies and underscore the critical roles of gravitational and thermal physics in testing the constancy of fundamental parameters.