Physical Review Letters · 2003 · 297 citations · 16 references
Natural SciencesPhysicsInstrumentationQuantum MechanicsSpectroscopyAtomic ClocksFrequency MetrologyLaser CoolingLaser SpectroscopyPrecision SpectroscopyAtomic Clock ExperimentsAtomic Frequency StandardsAtomic Transition FrequenciesFrequency Ratio MeasurementsFundamental Physical ConstantsGround State PropertiesHyperfine Transition FrequenciesSystematic Frequency Shifts
Over five years, we have compared the hyperfine frequencies of $^{133}\mathrm{C}\mathrm{s}$ and $^{87}\mathrm{R}\mathrm{b}$ atoms in their electronic ground state using several laser-cooled $^{133}\mathrm{C}\mathrm{s}$ and $^{87}\mathrm{R}\mathrm{b}$ atomic fountains with an accuracy of $\ensuremath{\sim}{10}^{\ensuremath{-}15}$. These measurements set a stringent upper bound to a possible fractional time variation of the ratio between the two frequencies: $\frac{d}{dt}\mathrm{ln}[({\ensuremath{\nu}}_{\mathrm{R}\mathrm{b}})/({\ensuremath{\nu}}_{\mathrm{C}\mathrm{s}})]=(0.2\ifmmode\pm\else\textpm\fi{}7.0)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}16}\text{ }{\mathrm{y}\mathrm{r}}^{\ensuremath{-}1}$ ($1\ensuremath{\sigma}$ uncertainty). The same limit applies to a possible variation of the quantity $({\ensuremath{\mu}}_{\mathrm{R}\mathrm{b}}/{\ensuremath{\mu}}_{\mathrm{C}\mathrm{s}}){\ensuremath{\alpha}}^{\ensuremath{-}0.44}$, which involves the ratio of nuclear magnetic moments and the fine structure constant.
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Natural Sciences, Physics, Cosmology +16