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arXiv:1910.09736 · Physical Review A

Magic wavelength of the Ba+138 6s S1/22–5d D5/22 clock transition

Sapam Ranjita Chanu, V. P. W. Koh, K. J. Arnold, R. Kaewuam, Ting Rei Tan, Zhiqiang Zhang, Marianna S. Safronova, M. D. Barrett

Published Apr 22, 2020• 9 citations
arXivHTMLPDF

Abstract

The zero crossing of the dynamic differential scalar polarizability of the ${S}_{1/2}\ensuremath{-}{D}_{5/2}$ clock transition in $^{138}\mathrm{Ba}^{+}$ has been determined to be $459.1614(28)\phantom{\rule{0.28em}{0ex}}\mathrm{THz}$. Together with previously determined matrix elements and branching ratios, this tightly constrains the dynamic differential scalar polarizability of the clock transition over a large wavelength range ($\ensuremath{\gtrsim}700\phantom{\rule{0.28em}{0ex}}\mathrm{nm}$). In particular, it allows an estimate of the blackbody radiation shift of the clock transition at room temperature.

DOI
10.1103/physreva.101.042507

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The zero crossing of the dynamic differential scalar polarizability of the S1/2\ensuremath−D5/2{S}_{1/2}\ensuremath{-}{D}_{5/2}S1/2​\ensuremath−D5/2​ clock transition in 138Ba+^{138}\mathrm{Ba}^{+}138Ba+ has been determined to be 459.1614(28)THz459.1614(28)\phantom{\rule{0.28em}{0ex}}\mathrm{THz}459.1614(28)THz. Together with previously determined matrix elements and branching ratios, this tightly constrains the dynamic differential scalar polarizability of the clock transition over a large wavelength range (\ensuremath≳700nm\ensuremath{\gtrsim}700\phantom{\rule{0.28em}{0ex}}\mathrm{nm}\ensuremath≳700nm). In particular, it allows an estimate of the blackbody radiation shift of the clock transition at room temperature.
Zero crossings of the differential scalar polarizability of Ba+^++ clock transition
The differential scalar polarizability Δα0(ω)Δα_0(ω)Δα0​(ω) of the Ba+^++ S1/2_{1/2}1/2​-to-D5/2_{5/2}5/2​ clock transition has a zero crossing near 481nm, which is measured to be 623.603\,13(17)\,THz. From this measurement, we infer a ratio of reduced matrix elements ⟨P3/2∥r∥S1/2⟩/⟨P1/2∥r∥S1/2⟩=1.411 81(13)\langle P_{3/2}\|r\|S_{1/2}\rangle/\langle P_{1/2}\|r\|S_{1/2}\rangle=1.411\,81(13)⟨P3/2​∥r∥S1/2​⟩/⟨P1/2​∥r∥S1/2​⟩=1.41181(13), which provides a stringent test of atomic structure calculations and experimental determination of matrix elements. Additionally, it enables the construction of an accurate approximation to Δα0(ω)Δα_0(ω)Δα0​(ω), valid for frequencies up to 450\,THz, with only one reduced matrix element, ⟨P1/2∥r∥S1/2⟩\langle P_{1/2}\|r\|S_{1/2}\rangle⟨P1/2​∥r∥S1/2​⟩, appearing in the model's parameterization. We discuss the achievable accuracy of the model, the application to the assessment of blackbody radiation (BBR) shifts in ion-based clocks, and the applicability of the approach to other alkaline-earth ions.
It is shown that the dynamic differential scalar polarizability of the ${S}_{1/2}\ensuremath{-}{D}_{5/2}$ transition in 138Ba+^{138}\mathrm{Ba}^{+}138Ba+ can be determined to an inaccuracy below 0.50.5%0.5 across a wide wavelength range ($\ensuremath{\lambda}>700\phantom{\rule{0.28em}{0ex}}\mathrm{nm}$). This can be achieved using measurements for which accurate determination of laser intensity is not required, and most of the required measurements are already in the literature. Measurement of a laser-induced ac-Stark shift of the clock transition would then provide an in situ measurement of the laser's intensity to the same 0.50.5%0.5 level of inaccuracy, which is not easily achieved by other means. This would allow accurate polarizability measurements for clock transitions in other ions, through comparison with 138Ba+^{138}\mathrm{Ba}^{+}138Ba+. The approach would be equally applicable to Sr+{\mathrm{Sr}}^{+}Sr+ and Ca+{\mathrm{Ca}}^{+}Ca+, with the latter being immediately applicable to Al+/Ca+{\mathrm{Al}}^{+}/{\mathrm{Ca}}^{+}Al+/Ca+ quantum logic clocks.
Differential static polarizability and black body radiation (BBR) shift for Ytterbium ion (171Yb+) clock transition from ground state2S1/2to metastable state2D3/2corresponding to the wavelength 435.5 nm are calculated accurately for frequency standard applications. The values are found to be −7.5(5) × 10−40Jm2/V and −0.4(1) Hz, respectively, which are well in agreement with pre-available data and more accurate than the previous theoretical results. We further determine the values of dynamic polarizability of these states to find out the magic and tune-out wavelengths for the above mentioned clock transition.
The interaction between light and an atom causes perturbations in the atom's energy levels, known as the light shift. These light shifts are a key source of inaccuracy in atomic clocks, and can also deteriorate their precision. We present a study of light shifts and associated dynamic polarizabilities for a two-photon atomic clock based on the 5S1/25{S}_{1/2}5S1/2​--5D5/25{D}_{5/2}5D5/2​ transition in rubidium-87 over the range 770--800 nm. We determine experimental and theoretical values for a magic wavelength in this range and the electric dipole (E1) matrix element for the 5P3/25{P}_{3/2}5P3/2​--5D5/25{D}_{5/2}5D5/2​ transition. We find a magic wavelength of 776.179(5) nm (experimental) and 776.21 nm (theoretical) in the vicinity of the 5P3/25{P}_{3/2}5P3/2​--5D5/25{D}_{5/2}5D5/2​ resonance, and the corresponding reduced E1 matrix element 1.80(6)ea01.80(6)e{a}_{0}1.80(6)ea0​ (experimental) and 1.96(15)ea01.96(15)e{a}_{0}1.96(15)ea0​ (theoretical). These values resolve a previous discrepancy between theory and experiment.
Measurement of infrared magic wavelength for an all-optical trapping of 40^{40}40Ca+^{+}+ ion clock
For the first time, we experimentally determine the infrared magic wavelength for the 40^{40}40Ca+^{+}+ 4s 2 ⁣S1/2→3d 2 ⁣D5/24s\, ^{2}\!S_{1/2} \rightarrow 3d\,^{2}\!D_{5/2}4s2S1/2​→3d2D5/2​ electric quadrupole transition by observation of the light shift canceling in 40^{40}40Ca+^{+}+ optical clock. A "magic" magnetic field direction is chosen to make the magic wavelength insensitive to both the linear polarization purity and the polarization direction of the laser. The determined magic wavelength for this transition is 1056.37(9)~nm, which is not only in good agreement with theoretical predictions but also more precise by a factor of about 300. Using this measured magic wavelength we also derive the differential static polarizability to be −44.32(32)-44.32(32)−44.32(32)~a.u., which will be an important input for the evaluation of the blackbody radiation shift at room temperatures. Our work paves a way for all-optical-trapping of 40^{40}40Ca+^{+}+ optical clock.