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arXiv · 1907.10805

Frequency Shifts due to Stark Effects on a Rb two-photon transition

Kyle W Martin·Benjamin Stuhl·Jon Eugenio·Marianna S. Safronova·Gretchen Phelps·John H. Burke·Nathan D. Lemke
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Abstract

The $5S_{1/2}\rightarrow 5D_{5/2}$ two-photon transition in Rb is of interest for the development of a compact optical atomic clock. Here we present a rigorous calculation of the 778.1~nm ac-Stark shift ($2.30(4) \times10^{-13}$(mW/mm$^2$)$^{-1}$) that is in good agreement with our measured value of $2.5(2) \times10^{-13}$(mW/mm$^2$)$^{-1}$. We include a calculation of the temperature-dependent blackbody radiation shift, we predict that the clock could be operated either with zero net BBR shift ($T=495.9(27)$~K) or with zero first-order sensitivity ($T=368.1(14)$~K). Also described is the calculation of the dc-Stark shift of 5.5(1)$\times 10^{-15}$/(V/cm$^2$) as well as clock sensitivities to optical alignment variations in both a cat's eye and flat mirror retro-reflector. Finally, we characterize these Stark effects discussing mitigation techniques necessary to reduce final clock instabilities.

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Kyle W Martin, Benjamin Stuhl, Jon Eugenio, Marianna S. Safronova, Gretchen Phelps, John H. Burke, Nathan D. Lemke. 2019-07-25. Frequency Shifts due to Stark Effects on a Rb two-photon transition. https://doi.org/10.1103/physreva.100.023417

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