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Toward a mercury optical lattice clock: Development of a dipole lattice trap at the magic wavelength

John J. McFerran, Sinda Mejri, L. Yi, S. Bize

Published Jun 1, 2010• 0 citations
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Abstract

We describe our work to develop an optical lattice clock using neutral mercury, which has the potential to reach accuracy near 1 part in 1018owing to its low sensitivity to black body radiation. We describe developments of our experimental setup to allow dipole lattice trapping and spectroscopy in the Lamb-Dicke regime. Specifically, we report on the implementation of a low noise imaging and detection system, on the characterization of the magneto-optic trap from which the dipole trap will be loaded, on the implementation of the dipole lattice trap itself, a challenging task given the wavelength and power requirements.

DOI
10.1109/cpem.2010.5544418

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We describe our work to develop an optical lattice clock using neutral mercury, which has the potential to reach accuracy near 1 part in 1018owing to its low sensitivity to black body radiation. We describe developments of our experimental setup to allow dipole lattice trapping and spectroscopy in the Lamb-Dicke regime. Specifically, we report on the implementation of a low noise imaging and detection system, on the characterization of the magneto-optic trap from which the dipole trap will be loaded, on the implementation of the dipole lattice trap itself, a challenging task given the wavelength and power requirements.
We are investigating the possibilities of using neutral mercury as a new species to realize a highly accurate atomic clock using the non-perturbing dipole lattice trapping scheme. Typically, accuracy below 10-17 is targeted, which would make neutral mercury an interesting candidate for a redefinition of the SI second. This paper presents our on-going work towards the realization of an optical lattice clock using neutral mercury. We will describe a 254 nm laser source delivering several hundreds of milliWatts at this wavelength with a suitably low frequency noise for laser cooling and magneto-optic trapping. We will describe our vacuum system for magneto-optic trap and report on the status of our work regarding magneto-optic trapping of mercury. We will also describe our clock laser at 266 nm.
We present details on the ultraviolet lattice spectroscopy of the (6sss2{}^{2}2) 1{}^{1}1SSS${}_{0}\ensuremath{\leftrightarrow}$ (6$s666p$) 3{}^{3}3PPP0{}_{0}0​ transition in neutral mercury, specifically 199{}^{199}199Hg. Mercury atoms are loaded into a one-dimensional vertically aligned optical lattice from a magneto-optical trap with an rms temperature of $\ensuremath{\sim}$60 $\ensuremath{\mu}$K. We describe aspects of the magneto-optical trapping, the lattice cavity design, and the techniques employed to trap and detect mercury in an optical lattice. The clock-line frequency dependence on lattice depth is measured at a range of lattice wavelengths. We confirm the magic wavelength to be 362.51(0.16) nm. Further observations to those reported by Yi et al. [Phys. Rev. Lett. 106, 073005 (2011)] are presented regarding the laser excitation of a Wannier-Stark ladder of states.
To realize a neutral mercury lattice clock, an experimental setup is in developing in SIOM. With two stable cooling lasers and a new vacuum system, an enhanced cold mercury atom source is implemented based on a two-dimensional magneto-optical trap (2D-MOT). By applying a hybrid frequency stabilization method and optimization of the 2D-MOT, about 1.3×106cold mercury atoms are obtained with a loading rate of 1.0×106atoms/s. And a high power injection-locked Ti:sapphire laser at 725 nm is developed for optical lattice at magic-wavelength.
The optical lattice clock develops fast in recent years, and its stability and accuracy has already surpassed the microwave fountain clock and the optical clock based on ion trap. The mercury (Hg) lattice clock has the possibility to make a breakthrough in the limitation of blackbody radiation shift for strontium (Sr) and ytterbium (Yb) lattice clock, and reach the uncertainty in E-18 level at room temperature. For the purposes of laser cooling of mercury atoms and interrogating of the clock transition from1S0state to3P0state, a high-power cooling laser at 253.7 nm and an ultra-stable Hz-level linewidth laser at 265.6 nm are required, respectively. Here, we report our development of these laser sources for a neutral Hg lattice clock.