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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Mejri, S. Yi, L. McFerran, J.J. Bize, S. |
| Copyright Year | 2011 |
| Description | Author affiliation: LNE-SYRTE, Observatoire de Paris, CNRS UMR 8630, UMPC, 61 Avenue de l'Observatoire, 75014 Paris, France (Mejri, S.; Yi, L.; McFerran, J.J.; Bize, S.) |
| Abstract | Optical lattice clocks offer the possibility to combine accuracy in the $10^{−18}$ range together with exquisite short stability, $10^{−16}$ for a measurement time of 1 second or even better [7]. Clocks with such level of accuracy and stability largely outperform the existing primary frequency standard based on the laser-cooled atomic fountain geometry and on an atomic transition in the microwave domain. Optical clocks allow fundamental physics tests with unprecedented accuracy [11] and open the way to new applications such as Earth gravitation potential mapping [12]. The ultimate limitation to the performance of optical lattice clock is still under investigation. Nonetheless, one limiting systematic shifts is clearly identified already: the blackbody radiation shift, the shift of the clock frequency due to the interaction of atoms with the ambient thermal electromagnetic background. At the temperature of 300 K and in fractional terms, this frequency shift is of the order of $−5.5×10^{−15}$ for strontium (Sr) and $−2.6×10^{−15}$ for ytterbium (Yb). Consequently, this effect must be controlled to much better than the percent level for an accuracy of $10^{−17},$ a highly challenging task. One motivation for considering mercury (Hg) is its low susceptibility to blackbody radiation [8]. At 300 K, the corresponding fractional frequency shift is only $−1.6×10^{−16},$ ∼16 times smaller than for Yb and ∼34 times smaller than for Sr. Hg is also interesting for its high sensitivity to a putative variation of the fine structure constant. Hg has 7 natural isotopes, 6 of them with abundance above 6%, 2 fermions and 5 bosons, which are all candidates for an optical lattice clock. Using Hg for an optical lattice clock remains however a significant technical challenge given that most of the laser wavelengths necessary to manipulate atoms and to probe the clock transition are in the deep ultraviolet range of the electromagnetic spectrum. |
| Starting Page | 1 |
| Ending Page | 2 |
| File Size | 144698 |
| Page Count | 2 |
| File Format | |
| ISBN | 9781424451173 |
| e-ISBN | 9781424460519 |
| DOI | 10.1109/URSIGASS.2011.6050321 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 2011-08-13 |
| Publisher Place | Turkey |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Atomic measurements Lattices Measurement by laser beam Laser transitions Mercury (metals) Atomic clocks |
| Content Type | Text |
| Resource Type | Article |
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