Abstract
We apply a recently demonstrated method for precision spectroscopy on strong transitions in trapped ions to measure both fine-structure components of the 3s−3p transition in 24Mg+ and 26Mg+. We deduce absolute frequency reference data for transition frequencies, isotope shifts, and fine-structure splittings that in particular are useful for comparison with quasar absorption spectra, which test possible space-time variations of the fine-structure constant. The measurement accuracy improves previous literature values, when existing, by more than two orders of magnitude.
Originalsprache | englisch |
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Seiten (von - bis) | 022503 |
Seitenumfang | 8 |
Fachzeitschrift | Physical Review B |
Jahrgang | 80 |
DOIs | |
Publikationsstatus | Veröffentlicht - 1 Aug. 2009 |
Extern publiziert | Ja |
Fields of Expertise
- Advanced Materials Science