Narrow-line Cooling and Determination of Magic Wavelength of Cd
arXiv:1909.07931 · doi:10.1103/PhysRevLett.123.113201
Abstract
We experimentally and theoretically determine the magic wavelength of the (5)(55) clock transition of Cd to be 419.88(14) nm and 420.1(7) nm. To perform Lamb-Dicke spectroscopy of the clock transition, we use narrow-line laser cooling on the transition to cool the atoms to 6 K and load them into an optical lattice. Cadmium is an attractive candidate for optical lattice clocks because it has a small sensitivity to blackbody radiation and its efficient narrow-line cooling mitigates higher order light shifts. We calculate the blackbody shift, including the dynamic correction, to be fractionally 2.83(8)10 at 300 K, an order of magnitude smaller than that of Sr and Yb. We also report calculations of the Cd lifetime and the ground state coefficient.
6 pages 5 figures 1 table + supplemental material 3 pages 2 tables
References in corpus (10)
- An Al quantum-logic clock with systematic uncertainty below
- Improved limit on a temporal variation of from comparisons of Yb and Cs atomic clocks
- Multipolar theory of black-body radiation shift of atomic energy levels and its implications for optical lattice clocks
- Real-time geopotentiometry with synchronously linked optical lattice clocks
- A transportable optical lattice clock with uncertainty
- Development of a configuration-interaction + all-order method for atomic calculations
- Operational Magic Intensity for Sr Optical Lattice Clocks
- Magneto-optical Trapping of Cadmium
- Optical clock sensitive to variation of the fine structure constant based on the Ho ion
- Relativistic calculations of and coefficients for strontium dimers
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