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Updated Constraints on the Variations of the Fine-Structure 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, α = e 2 4 π ε 0 ℏ c . The analysis was combined with laboratory-measured and astronomically observed lines in [Ni V] to find Δ α / α = ( − 0.003 ± 0.072 ) × 10...
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Published in: | Symmetry (Basel) 2019-07, Vol.11 (7), p.936 |
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Main Author: | |
Format: | Article |
Language: | English |
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Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | I fused observed spectra from the white-dwarf star G191-B2B to constrain the spatial and temporal variation of the fine-structure constant, α = e 2 4 π ε 0 ℏ c . The analysis was combined with laboratory-measured and astronomically observed lines in [Ni V] to find Δ α / α = ( − 0.003 ± 0.072 ) × 10 − 6 . The obtained result allows a symmetry of the related comparison with previous studies looking for cosmological variations of α 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 Δ α / α than previous studies using the same data. |
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ISSN: | 2073-8994 2073-8994 |
DOI: | 10.3390/sym11070936 |