Updated Constraints on the Variations of the FineStructure Constant from an Analysis of White-Dwarf Spectra

I fused observed spectra from the white-dwarf star G191-B2B to constrain the spatial and temporal variation of the fine-structure constant, . The analysis was combined with laboratory-measured and astronomically observed lines in [Ni V] to find . The obtained result allows a symmetry of the related comparison with previous studies looking for cosmological variations of  using spectra from Quasi Stellar Objects (QSOs). In this way, we can expect higher sensitivity from white-dwarf spectra than QSO spectra. Therefore, this study should have orders-of-magnitude higher sensitivity per system than previous quasar studies, and we should reduce statistical and systematic errors. The results of this study place a more stringent limit on  than previous studies using the same data.