The accuracy of state-of-the-art atomic clocks is derived from the insensitivity of narrow optical atomic resonances to environmental perturbations. Two such resonances in singly ionized lutetium have been identified with potentially lower sensitivities compared to other clock candidates. Here we report measurement of the most significant unknown atomic property of both transitions, the static differential scalar polarizability. From this, the fractional blackbody radiation shift for one of the transitions is found to be −1.36(9) × 10−18 at 300 K, the lowest of any established optical atomic clock. In consideration of leading systematic effects common to all ion clocks, both transitions compare favorably to the most accurate ion-based clocks reported to date. This work firmly establishes Lu+ as a promising candidate for a future generation of more accurate optical atomic clocks.
Development of stable and accurate time standards has historically been an important driver of both fundamental science and applied technologies. The recent decade has seen phenomenal progress in atomic clocks based on optical transitions such that several systems now demonstrate frequency inaccuracies approaching 10−181,2,3, two orders of magnitude better than state-of-the-art cesium fountain clocks that currently define the SI second4. Redefinition of the second is already under consideration5,6, but is unlikely until consensus on a best optical standard emerges. A significant technical hurdle for achieving inaccuracies below 10−18 outside of a cryogenic environment is the systematic uncertainty due to the blackbody radiation (BBR) shift7.
For an optical transition with static differential scalar polarizability Δα0 ≡ α0(e) − α0(g), where e and g refer to the excited and ground states respectively, the BBR shift, δνbbr, in Hz, is given by8
Here = (831.945 V m−1)2 is the mean-squared electric field inside a blackbody at temperature T0 = 300 K, and η(T) is a temperature dependant correction which accounts for the frequency dependence of Δα0(ν) over the blackbody spectrum8. Polarizabilities are reported in atomic units throughout which can be converted to SI units via α/h (Hz m2 V−2) = 2.48832 × 10−8α (a.u.).
Singly ionized lutetium has two candidate clock transitions with favorable clock systematics9,10, 1S0 ↔ 3D1 and 1S0 ↔ 3D2. Theoretical estimates of Δα0,1 ≡ α0(3D1) − α0(1S0) = 0.5(2.7) a.u. and Δα0,2 ≡ α0(3D2) − α0(1S0) = −0.9(2.9) a.u. have been given11,12, albeit with indeterminate sign and magnitudes limited by the error estimates. In this work, experimental measurements of both Δα0,1 and Δα0,2 are made and the BBR shifts assessed. At 300 K, the fractional BBR shifts are −1.36(9) × 10−18 and 2.70(21) × 10−17 for the 1S0 ↔ 3D1 and 1S0 ↔ 3D2 transitions, respectively. The former is the lowest among all optical clock candidates under active consideration13. Finally, the prospects for 176Lu+ as a frequency standard are discussed by comparison of its atomic properties to other leading clock candidates.
While neutral-atom clocks have performed high accuracy (2 × 10−5) measurements of Δα0 using precise dc electric fields14,15, this technique cannot be applied for ion clocks. Ion clocks have employed various methods to determine Δα0: inference from micromotion-induced stark shifts16, cancellation of second-order Doppler and Stark micromotion shifts for cases where Δα0 < 017, and extrapolation from measurements of Δα0(ν) at near infrared (NIR) laser frequencies2,18. These approaches are not suitable for measurements in 176Lu+ because, respectively: micromotion-induced Stark shifts would likely be too small to measure accurately, the signs of Δα0,1 and Δα0,2 are unknown, and extrapolation from measurements at NIR frequencies would be inconclusive given the magnitude of dynamic variation of the polarizabilties11.
The approach taken here is to measure Δα0(νm) at the mid-infrared frequency of νm = c/(10.6 μm), which is near to the peak of the blackbody spectrum at room temperature. The availability of high power CO2 laser sources ensures measurable ac Stark shifts even for small polarizabilities. In addition, a differential measurement of the clock frequency using an interleaved servo technique19 requires only one clock and eliminates uncertainties due to common-mode perturbations. This approach enables unambiguous measurement of the sign and magnitude of the polarizabilities with an accuracy limited by the determination of the CO2 laser intensity at the ion.
where is a state dependant scale factor21, α0,J(ν) and α2,J(ν) are, respectively, the dynamic scalar and tensor polarizabilities, is the mean squared electric field averaged over one optical cycle, and ϕ is the angle between the polarization and quantization axes. The quantization axis is defined by an applied magnetic field of ~ 0.2 mT and different values of ϕ are obtained by rotating this field with respect to the CO2 laser polarization. Light shifts as a function of beam position are used to characterize the beam profile and hence intensity for a given power. Light shifts at different values of ϕ for the transitions shown in Fig. 1b, are then used to determine differential scalar polarizabilities, Δα0,J, and tensor polarizabilities α2,J for the two clock transitions.
The experimental setup consists of a single 176Lu+ ion confined to a linear Paul trap with identical construction as in ref.22. The trap is operated with an rf drive frequency of Ω/2π = 20.8 MHz. Detection, cooling, and state preparation are performed on the 3D1 → 3P0 transition at 646 nm, with repump lasers at 350 and 622 nm to clear the 1S0 and 3D2 states, respectively (see Fig. 1a). The 1S0 ↔ 3D1 clock transition at 848 nm is a highly forbidden magnetic dipole (M1) transition with an estimated lifetime of 172 h23; and the 1S0 ↔ 3D2 at 804 nm is a spin-forbidden electric quadrupole (E2) transition with a measured lifetime of 17.3 s11. Both 848 and 804 nm clock lasers are frequency offset locked to the same reference cavity which has finesse of 400,000 and 30,000 at the respective wavelengths.
The 10.6 μm radiation is produced by a 10 W CO2 laser. An acousto-optic modulator is used to control the optical power at the ion and as an optical switch, demonstrating better than 30 dB extinction. Two ZnSe vacuum viewports provide optical access to the ion. Displacement of the beam in the yz-plane is achieved with mirrors on motorized translation stages, as shown schematically in Fig. 2a and detailed in Methods. The laser is linearly polarized along the z-axis. The optical power is monitored with a thermal power meter at the exit viewport and after a dichroic mirror. The measured transmissions of the ZnSe viewport and dichroic mirror at 10.6 μm are 0.990 (5) and 0.986 (5), respectively.
The light shift induced on the |3D1, 7, 0〉 ↔ |3D1, 6, 0〉 microwave transition has only a tensor contribution. This provides a useful diagnostic to determine the angle ϕ as the magnetic field is rotated: at ϕ = 90°, the light shift is at an extremum, and, at ϕ ≈ 54.7°, the light shift vanishes. At ϕ ≈ 90°, the light shift measured as a function of beam position determines the spatial profile of the laser beam. From the measured profile shown in Fig. 2b, a peak intensity relative to the incident optical power of Imax/P = 36.8 (8) mm−2 can be inferred (see Methods). The interrogation sequence for the microwave measurements is the same as in ref.22 with typical interrogation times of 10–50 ms depending on the desired Fourier limited resolution.
To determine Δα0,J(νm), the magnetic field is rotated to ϕ ≈ 54.7° where the tensor component of the light-shift vanishes. The 848 nm (804 nm) clock lasers are then stabilised to the average of the |1S0, 7, ±1〉 ↔ |3D1, 7, 0〉 (|3D2, 9, 0〉) transitions (see Fig. 1b). The light-shift is measured by interrogating alternately with and without the CO2 laser and measuring the difference frequency between the two configurations. Typical interrogation times are 10–20 ms for the 848 nm transition and 1.5 ms for the 804 nm transition. Figure 3a shows the measured light shifts on the 848 nm clock transition (green points) as a function of CO2 laser power together with interleaved measurements of the microwave transition (yellow points) for tracking the suppression of the tensor shift. The observed deviations of the microwave transition frequency are consistent with fluctuations of either 0.2 μT in the transverse magnetic field or ~ 1 mrad in the CO2 laser polarization. The residual tensor shifts implied by the interleaved microwave measurements are removed from the optical measurements to generate the corrected data plotted in purple. A linear slope of −9.60 (13) HzW−1 is deduced by a χ2 fit to the corrected data. Figure 3b shows the light shifts on the 804 nm clock transition at the same magnetic field orientation and has a fitted slope 201.3 (2.2) Hz W−1. Owing to the larger light shifts involved, corrections due to residual tensor shifts were unnecessary.
The tensor polarizabilities are separately assessed by measuring the light shifts at ϕ = 90°. Figure 3c shows the light shifts measured on the |3D1, 7, 0〉 ↔ |3D1, 6, 0〉 microwave transition with the fitted slope 530.4 (3.4) Hz W−1. Figure 3d shows the light shifts on the |1S0, 7, 0〉 ↔ |3D2, 9, 0〉 optical transition with the fitted slope 431.0 (3.2) Hz W−1, from which the 3D2 tensor polarizability can be determined by subtracting the previously determined scalar component.
From the data presented in Fig. 3, we evaluate the dynamic polarizabilities, in atomic units, to be
The largest sources of systematic uncertainty are the accuracy of the thermal power meter, specified at 5%, and an additional 6% effect which we attribute to etalon interference (see Methods). In evaluating Δα0,1(νm) we have included a 6.5% correction to account for the laser induced ac Zeeman shift (see Methods). We have not included consideration of the hyperfine mediated scalar polarizability for the 3D1 levels7,24. From estimates omitting the hyperfine corrections to the wavefunctions, it is unlikely that this would be comparable to the measurement uncertainty. Nevertheless, it would be of interest to have a more accurate assessment given the size of the measured value.
BBR shift analysis
Because the measured differential scalar polarizability on the 1S0 ↔ 3D1 transition is very small, the extrapolation to dc and the dynamic BBR shift contribution must be carefully considered. Over the BBR spectrum near room temperature, the scalar polarizability is well described by a quadratic approximation
For extrapolation to dc, we estimate the quadratic coefficient using the theoretical dipole transition matrix elements11 and experimental energies25. Assuming 5% uncertainty in the theoretical matrix elements, we find Δα0,1(0) = 0.018 (6) (a.u.). Evaluating the BBR shift by integrating the polarizability Eq. (4) over the BBR spectrum gives
where β = ≈ 0.918. Direct comparison of this expression to Eq. (1) relates our measured dynamic polarizability to the usual dynamic correction factor, η(T), up to quadratic terms. Because 10.6 μm is near to the center of the room temperature BBR spectrum, δνbbr is relatively insensitive to the dc value Δα0,1(0). At ~ 313 K, δνbbr depends only on the measured value Δα0,1(νm). The BBR shift evaluated at 300 K is −1.36(9) × 10−18.
The insensitivity of the 1S0 ↔ 3D1 clock transition to temperature is illustrated in Fig. 4. Over the full range of 270–330 K the fractional uncertainty in the BBR shift remains below 1.0 × 10−18. For more applicable laboratory conditions of 300 ± 5 K, indicated by the thin black lines, the fractional uncertainty is 2 × 10−19.
At this level one might be concerned about the shift due to the magnetic field component of the BBR7. In this case the largest contribution is due to coupling to the 3D2 state. The approximation used in ref.7 for microwave transitions does not apply in this case and a numerical integration over the BBR spectrum must be used giving an estimated contribution of 3 × 10−20 at room temperature. The hyperfine mediated scalar polarisability7,24 will also contribute at the same order of magnitude with some cancelation due to hyperfine averaging9 expected.
For the 1S0 ↔ 3D2 transition, the dynamic BBR shift is small compared to the scalar shift and we can approximate Δα0,2(0) ≈ Δα0,2(νm). The corresponding fractional BBR shift is 2.70 (21) × 10−17 at 300 K.
For ion clocks, the value of Δα0 also has implications for micromotion-induced shifts. Micromotion driven by the rf-trapping field gives rise to two correlated clock shifts: an ac Stark shift and a time dilation shift. The net micromotion shift, δνμ, to lowest order, is given by17,26:
where ν0 is the optical transition frequency in Hz, e is the electron charge, Ω is the trap drive frequency, m is the atomic mass, and is the mean squared electric field at frequency Ω. For clock transitions with Δα0 < 0, there exists a ‘magic’ drive frequency Ω0 = at which δνμ vanishes. The suppression of micromotion shifts by operating at Ω0 has been applied in both 40Ca+ and 88Sr+ clocks17,27 and is advantageous for multi-ion clock schemes10,28. An ideal clock candidate would have Δα0 < 0 which is small in magnitude to mitigate BBR shifts but sufficiently large to permit a practical value of Ω0. The 1S0 ↔ 3D2 transition is in this ideal parameter regime with the lowest BBR shift among all such ion-clock candidates and a magic drive frequency of Ω0/2π ≈ 32.9 (1.3) MHz.
With measurement of the differential scalar polarizabilities, all atomic properties of 176Lu+ required to estimate clock systematics are known with sufficient accuracy to assess its future potential. The expected clock systematics for both transitions, after elimination of tensor shifts by hyperfine averaging9, are summarized in Table 1. Achievable uncertainties in these systematic shifts are considered in reference to state-of-the-art experimental techniques. The 1S0 ↔ 3D1 transition is uniquely insensitive to the BBR shift, leaving the residual micromotion-induced time dilation shift and ac-Stark shifts from the clock laser as leading systematics. Sensitivity to motional shifts favours heavier ions where, for example, evaluation of excess micromotion to the 10−19 level has been demonstrated for 172Yb+28. Using hyper-Ramsey spectroscopy29, suppression of the probe-induced ac Stark shifts by four orders of magnitude has been demonstrated in Yb+30, for which the shift is two order of magnitude larger than in Lu+. The 1S0 ↔ 3D2 transition has negligible probe-induced ac Stark shifts and net micromotion shifts can be heavily suppressed by operating near Ω0. With improved accuracy in the polarizability measurement17 and a 1 K uncertainty in the temperature of the surroundings2, the fractional BBR shift uncertainty could be reduced to the 10−19 level. For both Lu+ transitions, second-order Doppler shifts due secular thermal motion are less than 10−19 for Doppler-limited cooling10.
The overall clock systematics compare favorably to other candidates, including 171Yb+2 and 27Al+3, the two lowest uncertainty ion clocks reported at this time. The properties of the 171Yb+ E3 clock transition offer no advantage over either Lu+ transition in any category of Table 1: the BBR shift is ~3 times larger than for Lu+ (3D2), micromotion considerations are comparable to Lu+ (3D1), and the probe ac-Stark shift is two orders of magnitude larger than for Lu+ (3D1) for the same probe time. 27Al+ has a BBR shift ~6 times larger3 than Lu+ (3D1), requires an auxiliary ion for sympathetic cooling and state detection, and motion-induced shifts present a greater technical challenge due to the relatively light mass31. For experimental control comparable to that already demonstrated in the current generation of ion-based clock experiments, the systematics of 176Lu+ suggest no significant hurdle for achieving evaluated uncertainties at the 10−18 level and beyond. Furthermore, its unique combination of atomic properties make 176Lu+ a favoured candidate for multi-ion approaches10,28 to advance the stability of ion-based atomic clocks.
Optomechanical setup for beam displacement
The CO2 laser propagates in free space and is directed onto the ion by two mirrors and a lens to focus the laser on the ion. Displacement in the z(y) - direction is achieved by translating both (one) mirrors and the lens. Motorised translation stages were characterized by detecting the position of a visible laser overlapped with the CO2 laser using a CCD camera. The two axis of the motorized stages were found to be non-orthogonal by 4 mrad and this was subsequently corrected for in software. The rms positioning error measured by the camera was 0.7 (0.6) μm in the z (y) direction for a 2d profile scan comparable to the one shown in Fig. 2b.
Analysis of the laser profile
An approximate mode function is generated by cubic spline interpolation to the measurements shown in Fig. 2b. The peak intensity relative to the incident optical power is found by dividing the maximum light shift by the integral of this mode function over the interpolation region. The largest contributor to the uncertainty is the optical power instability of 1.5%. An elliptic TEM00 gaussian model fit to the data indicates <0.5% of the light shift distribution is truncated by the finite interpolation region.
Systematic uncertainties of the polarizabilities
We observe discrete jumps in the measured light shift, monitored over the course of the day, at intervals of approximately one hour within a 6% range. These discreet jumps are not correlated with the optical power measured at the thermal detector. We attribute this predominately to frequency mode hops of the CO2 laser which alters the effective transmission of the ZnSe viewport (dichroic mirror) between the thermal detector and ion by as much as 2% (2.7%) due to etalon effects. These frequency jumps occur on timescales longer than a typical data collection window. Because the CO2 laser frequency is not controlled, we conservatively add the maximum range of variation observed in the light shift (6%) as an independent error to the power meter accuracy. Radiation reflected from the ZnSe window back to the ion contributes negligible (<0.1%) additional uncertainty in the intensity at the ion.
Laser induced ac Zeeman shift
Due to the small magnitude of Δα0,1(νm), shifts arising from the ac magnetic field of the CO2 laser should be considered. The most significant contribution arises from the magnetic dipole coupling between the 3D1 and 3D2 fine structure states, which are separated by ν0 ≈ 19.15 THz22. The quadratic Zeeman shift can be evaluated following the same treatment as for the dipole polarizability21. In the limit that the detuning is large relative to the hyperfine splitting, summation over all possible F′ results in a shift that can be broken down into scalar, vector, and tensor components. For linearly polarized light of frequency ν m the ac Zeeman shift for state |3D1, F, m F 〉 is found to be
where is the M1 reduced matrix element in Bohr magnetons, is rms magnetic field, is the same state dependant coefficient as in Eq. (2), and θ′ is the angle between the magnetic field and the quantization axis. Evaluated using the matrix element 2.05511, we find the scalar shift on the |3D1, 7, 0〉 state is 0.627 Hz W−1. This is subtracted from result shown in Fig. 3a to determine Δα0,1(νm). In this experiment the tensor component of electric field was nulled and consequently the tensor component of the orthogonal magnetic field was not cancelled. However, this magnetic tensor shift is sufficiently small that it does not impact significantly on the accuracy to which the tensor component due to the electric field was nulled. Contributions from other magnetic couplings, such as to the 1D2 state, are not statistically significant.
All data presented and analyzed this study are available from the corresponding author upon reasonable request.
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We acknowledge J.S. Chen, S. Brewer and colleagues at the National Institute for Standards and Technology (NIST) for prompting us to evaluate the laser induced ac Zeeman shift. T. R. Tan acknowledges support from the Lee Kuan Yew postdoctoral fellowship. This research is supported by the National Research Foundation, Prime Ministers Office, Singapore and the Ministry of Education, Singapore under the Research Centres of Excellence programme. It is also supported by A*STAR SERC 2015 Public Sector Research Funding (PSF) Grant (SERC Project No: 1521200080).
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