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Experimental realization of an optical second with strontium lattice clocks

Nature Communications volume 4, Article number: 2109 (2013) | Download Citation

  • A Corrigendum to this article was published on 31 October 2013

This article has been updated

Abstract

Progress in realizing the SI second had multiple technological impacts and enabled further constraint of theoretical models in fundamental physics. Caesium microwave fountains, realizing best the second according to its current definition with a relative uncertainty of 2–4 × 10−16, have already been overtaken by atomic clocks referenced to an optical transition, which are both more stable and more accurate. Here we present an important step in the direction of a possible new definition of the second. Our system of five clocks connects with an unprecedented consistency the optical and the microwave worlds. For the first time, two state-of-the-art strontium optical lattice clocks are proven to agree within their accuracy budget, with a total uncertainty of 1.5 × 10−16. Their comparison with three independent caesium fountains shows a degree of accuracy now only limited by the best realizations of the microwave-defined second, at the level of 3.1 × 10−16.

Introduction

When the international system of units was formalized in 1960, the definition of the second was still derived from an astronomical reference, the Ephemeris Time. Following the measurement1 of the caesium ground state hyperfine F=3—F′=4 transition frequency (~ 9.19 GHz) in terms of the Ephemeris Time second, this transition was chosen as reference for a new definition of the SI second in 1967. The level of control on the systematic effects perturbing the clocks realizing this definition, or accuracy, has steadily progressed over the years and has now reached a level of ~2–4 × 10−16 in fractional units in the case of the best atomic fountains2. In parallel, an operational architecture was developed to establish and distribute time scales based on this microwave second, for example, via satellite systems like GPS or TWSTFT. The advent of the frequency combs3,4 in 2000 led to a revolution in the field of frequency metrology. At once, this simple and accurate way to link the optical (~1015 Hz) and the microwave domains made it possible to take full benefit from decades of progress in optical spectroscopy and laser cooling of atoms. It stimulated the development of a new generation of atomic clocks, based on optical transitions, and realizing their own unperturbed frequency with an uncertainty now surpassing the best realizations of the SI second. In this context, the term accuracy is now often used to quantify the control of systematic effects in relation to this unperturbed optical frequency, even though optical clocks are not realizing the SI second.

A few optical clocks operated with single ions feature a record control of the systematics in the 10−17 range5,6,7 or even 8.6 × 10−18 (ref.8). Research on optical lattice clocks (OLCs) is comparatively recent,9,10,11,12,13 but in less than 10 years they have reached the 10−16 level14,15,16, with excellent prospects towards the 10−17 level. The large number of probed atoms, on the order of 104, is a major asset: it already allows unprecedented statistical resolutions that translate into frequency stabilities of a few 10−16 at one second, demonstrated in some groups17,18,19,20. The key feature of this type of clocks is the trapping of neutral atoms in a deep optical potential, which allows interrogation times of several 100 ms. The decisive introduction of the magic wavelength9,21 led to a precise control of the light shift induced by the potential on the atoms, ensuring that it does not degrade the accuracy at least down to 10−17 (ref. 22). In addition to the trapping effects, other systematic effects were studied in detail in the framework of OLCs; for instance, despite the fermionic nature of atoms in most OLCs, residual atomic density effects in many-particle systems were highlighted23,24,25 and proved to be controllable below 10−18 (ref. 20). The parallel development of optical fiber links26,27,28 allows the dissemination of an optical frequency over long distances with a negligible added noise. With such a link, the possibility of comparing two remote OLCs has been demonstrated29 recently. These studies are preparing the ground for a possible redefinition of the second, and seven optical transitions have already been endorsed or recommended as secondary representations of the SI second. Nevertheless, a prerequisite before any of these candidates is chosen as new primary standard is to assess the reliability of their connection to the current SI second.

In this article, we describe the experimentation of an optical second based on an ensemble of five clocks. Firstly, we compare two optical clocks of the same nature, which is the ultimate test to validate the asserted accuracy. For the first time, two OLCs with a state-of-the-art uncertainty of 1.1 × 10−16 are proved to agree within their accuracy budget. Secondly, we demonstrate a reproducible link between these clocks and the microwave second realized by three atomic fountains. This comparison is now limited by the accuracy of the caesium fountains and constitutes the precision limit with which any frequency can be measured with respect to the current SI second. This work thus reports on a comprehensive and consistent set of optical–optical and optical–microwave clock comparisons prototyping an optical second.

Results

OLC architecture

We have built two OLCs12,22,30 based on the transition at 698 nm between the ground state 1S0 and the metastable state 3P0 of neutral 87Sr atoms, with a natural linewidth of 1 mHz. The atoms are tightly confined in a few thousand wells of an optical lattice formed by a standing wave in an optical resonator. This strong confinement regime (Lamb–Dicke regime) dramatically reduces the motional effects. The lattice induces a light shift of several 105 Hz on the energy levels, but, as anticipated in the initial proposal9, we can control the differential shift at the mHz level22 when the lattice is operated at the magic wavelength. Together with the J=0 nature of the clock states, this leads to a spectroscopy almost immune to fluctuations in trapping power or polarization. With consistent data accumulated over 2 years, we have evaluated the magic frequency canceling the differential scalar polarizability: fmagic=368,554,725 (5) MHz. As the optical lattice is the keystone of OLCs, we opted for two different trapping geometries30 to test the robustness of the clocks against technical choices (see Methods). The resonators forming the lattices allow trap depths as large as 5000 Er, Er being the recoil energy of a strontium atom absorbing a lattice photon. This provides an important leverage to explore the residual effects of the lattice22. We could thus resolve the second-order light shift, equal to 0.45 (10) μHz/ for a lattice polarization parallel to the quantization axis. These large depths, equivalent to temperatures of 0.8 mK, enable the capture of 104 atoms in 500 ms directly from the first stage 2 mK magneto-optical trap based on the 1S01P1 transition at 461 nm12. An extra cooling step is performed on the narrow line 1S03P1, before the potential is ramped down adiabatically to 100 Er. This leads to atomic temperatures of 1 μK in the strong confinement direction, and 10 μK in the transverse direction.

The large number of atoms probed simultaneously, together with the high Q-factor of the optical resonance, yields remarkable ultimate stabilities, 10−17 or below at 1 s if the quantum projection noise (QPN) limit is reached for 104 atoms. Steady work on ultrastable lasers18,19,20,31,32 and interrogation sequences17,33 has brought OLCs close to this limit17,18,19,20. Here, the two atomic clouds are probed independently by pulses delivered by an ultrastable laser (spectral width <1 Hz). These pulses can be as long as 250 ms, resulting in Fourier-limited resonances of 3.2 Hz. Then, for each clock, the laser is locked to the narrow resonance via a digital integrator acting on a frequency shifter (Fig. 1). The difference between the corrections applied to the shifters gives the instantaneous frequency difference between the two clocks. Its relative stability is 3.0 × 10−15, reaching a resolution of 3 × 10−17 after an integration time, τ, of 3 h (Fig. 2).

Figure 1: LNE-SYRTE optical to microwave measurement chain.
Figure 1

An extended cavity laser diode (ECDL) referenced to an ultrastable cavity (USC698) via a Pound–Drever–Hall (PDH) feedback loop (Int) probes the atoms trapped in the respective lattices of the two optical clocks (Sr1 and Sr2). Orange arrows represent the lattice polarizations. The green arrows materialize the magnetic fields used to control the internal state of the atoms, the quantization axis to describe this state are chosen along the same directions. The detection systems keep the laser probes independently at resonance with the two clocks via a feedback (Int) on the frequency shifters (FS1 and FS2). This feedback is asynchronous, rejecting further possible common systematic effects due to the clock laser. The frequency of the USC698 is measured by a titanium-sapphire laser-based frequency comb referenced to an auxiliary ultrastable cavity (USC1062). The division of the USC698 frequency to the microwave domain is compared (μW comp.) to a cryogenic sapphire oscillator (CSO), itself locked to a H-maser on long time scales. Finally, the frequency of the CSO is measured by the three caesium atomic fountains FO1, FO2 and FOM, independently.

Figure 2: Fractional frequency stabilities for a single acquisition.
Figure 2

This Allan s.d. gives the resolution achieved when comparing two oscillators for an integration time τ. The error bars are statistical and correspond to a white noise behavior. The blue circles and the orange triangles show the stability of the corrections applied to the frequency shifters going to each Sr clock (a predictable residual drift of the USC698 is removed). In the first seconds, these curves are dominated by the Dick effect (sampling of the high frequency noise of the clock laser by the atoms, here for a clock pulse of 110 ms and cycle times of 1 s for Sr1 and 0.7 s for Sr2). The gain of the servo loop also determines how many cycles are necessary to effectively lock the laser to the atomic frequency. After 8 s, the fundamental thermal flicker noise of the USC698 becomes predominant, at the 8 × 10−16 level. However, the direct comparison between the two devices (purple squares) shows a white noise behavior scaling as 1. Its resolution reaches 3 × 10−17 in 3 hours, equivalent to 2 × 10−17 per clock. These optical–optical comparisons already beat by more than one order of magnitude the optical–microwave comparisons (green curves), dominated by the QPN of the fountains at 4.1 × 10−14 at 1 s in the best case.

Accuracy budgets of the OLCs and direct comparisons

The optical clocks feature an accuracy budget of respectively u1=1.03 × 10−16 and u2=1.09 × 10−16, detailed in Table 1 and the Methods section. The main contribution to this budget, 7 × 10−17, is the uncertainty on the black-body radiation (BBR) shift34, due to temperature inhomogeneities (~1 K) in the environment surrounding the atoms. However, temperature-controlled environments can successfully handle this effect. Recently, the uncertainty on the atomic sensitivity to BBR was dramatically reduced by experimental measurements35,36,37, corroborated by theoretical calculations38,39,40 (previous accuracy budgets of past studies14,15,16 are also reduced accordingly). To date, no effect seems in position to prevent OLCs accuracy from progressing by at least one order of magnitude.

Table 1: Uncertainty budget.

Comparing two clocks using the same atomic species is a crucial test to corroborate the fact that no systematic has been overlooked in their individual accuracy budget. This is the only case where the frequency ratio is known in advance: it is expected to be exactly 1 within the accuracy budget. While this procedure is extensively validated on local41 and global scales2 for microwave clocks, agreement between identical optical clocks, with a total uncertainty surpassing the accuracy of the best Cs standards, was reached only for Al+ ion clocks8 (total uncertainty 2.5 × 10−17), but had so far never been achieved for OLCs.

We have conducted repeated high-resolution comparisons between our two Sr clocks. Most acquisitions lasted several hours, ensuring a statistical uncertainty in the 10−17 range for each measurement, much lower than the systematic uncertainties. The frequencies of the two devices are in agreement, with a residual difference smaller than the systematic uncertainty (Fig. 3):

Figure 3: Direct comparison of the two strontium clocks.
Figure 3

The acquisitions were carried out over 1 week, the resolution of the measurements (black error bars) is such that most of them are limited by systematics (purple error bars). The lattice frequencies were changed for the three last points to check the robustness of the results. The average frequency difference (solid purple line) between the two clocks, 1.2 × 10−16, is compatible with zero within the systematic error bar (purple-shaded area, corresponding to the combined uncertainty of two uncorrelated clocks: =1.5 × 10−16). The gray-shaded area corresponds to the stability of the cumulated data. The χ2 of this average (0.55) is <1, which is typical of systematics fluctuating less than statistics.

This agreement was reached only after several unexpected shifts, due to patch charges inducing a DC Stark effect30 and to the residual spectral background of lattice lights (see Methods), had been identified and taken into account. This illustrates that direct comparisons between clocks based on the same atomic species, but with differences in the key features, are essential tests to support the exhaustiveness of the accuracy budget. Such shifts would have been undetectable with differential frequency measurements performed on a lone clock.

Comparisons of OLCs with three primary frequency standards

Continuity at the best possible level through revisions of the definition of units is key. It is notably the case for time scales, used through decades for advanced scientific applications such as monitoring of pulsar timing or Earth rotation. In the case of OLCs, ascertaining the continuity requires absolute frequency measurements at the limit of the microwave-defined second. At LNE-SYRTE, the strontium clock frequency was measured extensively with a unique ensemble of three state-of-the-art caesium fountains41. This ensemble is operated quasi-continuously, with strong connections to the international realization of the SI second2.

The titanium-sapphire laser-based frequency comb3,4 at the heart of our measurement chain (Fig. 1) connects two frequency domains separated by 5 orders of magnitude. The comb is phase-locked with a bandwidth of 400 kHz to a laser referenced to an ultrastable auxiliary cavity at 1,062 nm (USC1062) with a thermal noise floor at 4 × 10−16. The comb reaches therefore the narrow linewidth regime, with teeth spectrally narrower than 1 Hz. The comb measures the frequency ratio between two ultrastable oscillators: in the optical domain, the Sr clock laser at 698 nm (referenced to the ultrastable cavity USC698 exhibiting a thermal noise floor of 8 × 10−16), and, in the microwave domain, a Cryogenic Sapphire Oscillator (CSO, at 11.980 GHz, exhibiting a short-term stability in the 10−15 range, and locked to a H-maser to avoid long term drifts). By dividing the Sr laser frequency, the comb generates an ultrastable microwave signal referenced to the optical domain42,43, which is then compared with the CSO. This approach covers an important aspect of a possible redefinition of the second: this microwave signal could feed directly any conventional or satellite system in need of a frequency reference, the existing infrastructure would thus need no modification. At the same time, the absolute frequency of the CSO is simultaneously and independently measured by the three Cs fountains, while, at the other end of the chain, the frequency difference between the Sr clock transition and the USC698 is given by the corrections applied to the frequency shifter. These measurements are combined to provide the absolute frequency of Sr against each fountain.

We demonstrate the best frequency stability between an optical clock and a microwave clock ever reported to the best of our knowledge, at 4 × 10−14 at one second (Fig. 2). This number is solely limited by the QPN of the fountains, which constitutes a fundamental limitation. On 11 non-consecutive days, the absolute frequency of the 87Sr clock transition was measured against the three caesium fountains simultaneously (Fig. 4a). The independent averages are shown in Table 2. The large number of acquisitions ensured a statistical uncertainty lower than the systematic effects for each fountain. Furthermore, these three measurements agree within the systematic error bar, showing the consistency between fountains. The total average (Fig. 4b) yields:

Figure 4: Measurements of the absolute 87Sr clock frequency.
Figure 4

(a) The 11 LNE-SYRTE acquisitions, equivalent to 30 h of measurement, are scattered over 6 months. For each acquisition, the strontium clocks are compared to the 3 LNE-SYRTE fountains (FO1, FO2, FOM). The total error bars represented with each point are dominated by the statistical uncertainty. (b) Average per fountain of the points is shown in a. For each fountain, the statistical error bar (thin gray lines) is smaller than the systematic uncertainty (thick colored lines), thus giving three independent measurements of the 87Sr clock frequency limited by the fountain accuracy. The Sr systematic budget (gray background) is negligible. These three values are in excellent agreement, reinforcing the confidence in our final average (blue diamond, total statistical error bar and systematic error bar of the fountain contributing the most). (c) Worldwide history of the 87Sr clock frequency measurements reported by five different groups with their total error bar,42,16,47,48 modified accordingly to the BBR sensitivity from other studies36,40. Data points corresponding to a are shown in light green, the blue diamond represent the final average of b. The purple fit (straight line together with a sinusoidal yearly variation) takes into account all the points weighted by their respective total error bar: the measurement campaign presented here enables us to improve by a factor 8 the bound on the hypothetical time and spatial variations of the Sr/Cs frequency ratio.

Table 2: Per fountain measurements of the absolute 87Sr clock frequency.

As a fundamental progress of the microwave clocks no longer seems possible, we anticipate that this result borders on the ultimate accuracy at which any optical frequency can be measured in units of caesium-defined Hz.

Five groups worldwide have reported absolute frequency measurements of the 87Sr clock transition in the last 7 years (Fig. 4c). In this context, the data points presented by us strengthen the overall consistency, with an increased accuracy at 3.1 × 10−16. Our measurements, spanning over 6 months, enable us to track a change of the Sr/Cs frequency ratio due to possible variations of fundamental constants, which would reveal physics beyond the standard model. All the measured strontium frequencies are fitted by a linear drift (−3.3 × 10−16±3.0 × 10−16 per year) superimposed on a yearly sinusoidal contribution (1.2 × 10−16±4.4 × 10−16) modeling a hypothetical coupling of the constants with the sun’s gravitational potential, which would reflect a violation of the ‘local position invariance’ principle (Fig. 4c). This fit is still compatible with no variation of the constants, but with an eight-fold increased resolution compared to the previous measurements44. These laboratory tests of fundamental physics involve optical–microwave as well as optical–optical5 and microwave–microwave45 frequency ratios. They complement, on very different time scales and length scales, astronomical evidences in order to constrain theories in the ongoing quest for a unified description of gravitation and quantum mechanics. They are all the more topical in view of recent results reporting a spatial variation of the fine structure constant from observations of quasars46.

Discussion

The five state-of-the-art clocks of our architecture, two strontium OLCs and three caesium fountains, are ticking with an unprecedented consistency. The link between the optical frequency domain and the microwave second is demonstrated to be reproducible and now hindered by the hard limits the fountains are facing in accuracy (2.6 × 10−16) and stability (4 × 10−14 at 1 s due to the QPN). Direct comparisons between the two OLCs were necessary to show a level of agreement (1.2 × 10−16±1.5 × 10−16) better than what can be resolved by three of the best caesium fountains. Our study shows that strontium OLCs provide a reproducible frequency with a trustworthy connection to the current SI second, and therefore to the various time scales established in the last 50 years.

Several steps are nevertheless still required in order to demonstrate that OLCs are suited to a new definition of the second. Their accuracy continues to progress swiftly since the initial proposal9, it is therefore necessary to further explore their fundamental limits, instead of choosing a definition that would be rapidly overrun. Ongoing efforts aiming at controlling the BBR shift by means of temperature-regulated environments raise the prospect of accuracies at 1 × 10−17 or below for OLCs in a near future, thus possibly matching the performances of single-ion clocks, which have taken the lead in terms of control of the systematics5,6,7,8.

Finally, further comparisons, on a larger scale and between optical clocks designed and built in different institutes, are required to fully explore the potential of the various approaches. This process is crucial in order to confirm that all systematics have been comprehended, irrespective of experimental choices or local environment considerations. As an illustration, long-term comparisons between state-of-the-art caesium fountains sometimes showed discrepancies exceeding the individual accuracy budgets in the past. This highlights the complexity of establishing a universal time unit. Any redefinition of the SI second would require an international consensus through due process, under the supervision of the CIPM. The ongoing development of coherent long-distance fiber links and the associated dissemination of ultra-pure optical carrier let us contemplate the possibility of an all-optical clocks network. These links will soon enable comparisons between remote optical clocks, with a level of performance taking full advantage of the record stabilities recently permitted by OLCs20, thus allowing the exploration of clock’s physics at the <10−18 level. Such an extended network of clocks opens up new horizons for fundamental physics, such as testing of Einstein’s equivalence principle and of the gravitational redshift. Further, clock-based geodesy with ultimate precision already raises new prospects in Earth science47,48.

Methods

Geometry of the lattices

In order to demonstrate the level of control on the trapping effects, the two cavities forming the optical lattices have been designed in two different ways. The waist of the first lattice is 90 μm, and the intracavity power is 7 W, ensuring a maximum depth of 1,000 Er. With a waist of 56 μm and an intracavity power of 14 W, the second clock features potentials as deep as 5000 Er. The magic frequency, fmagic=368,554,725 (5) MHz, ensures only the cancellation of the scalar part of the differential polarizability; a tensor correction22 depending on the angle α between the lattice polarization and the quantization axis defined along the magnetic field can shift noticeably the effective magic point (from fmagic−268 MHz to fmagic+134 MHz). This angle also defines the sensitivity of the clocks to residual lattice polarization fluctuations. In the second lattice cavity, the absence of polarization selective element makes it difficult to ensure a perfectly linear polarization: α is thus chosen to minimize the sensitivity of this clock (α=12°±5°). In the first clock cavity, on the other hand, an intracavity mirror selects a highly stable linear polarization (> 99.9% in field), α is adjusted to almost maximize the sensitivity (α=51.5°±1°).

Zeeman shift

In order to control the influence of the magnetic field on the clock frequency, we optically pump the atoms alternately into the extreme Zeeman ground states mF=9/2 or −9/2, the axis being defined along an orientation field of 1 Gauss used to display the Zeeman structure. We then interleave measurements on the internal transitions |1S0, F=9/2, mF=9/2→|3P0, F′=9/2, mF′=9/2 and |1S0, F=9/2, mF=−9/2→|3P0, F′=9/2, mF′=−9/2, with no change of the quantum numbers describing the motion of the atoms in the lattice. The average of the two measured frequencies leads to a cancelation of the linear Zeeman shift and of the vector light shift. The difference of the two frequencies gives a real-time monitoring of the magnetic field B and of the ellipticity of the lattice polarization22. On long time-scales (104 s), B is constant at a level of 0.1%, thus the uncertainty on the second-order Zeeman shift correction (2 × 10−17) is limited by the knowledge of the sensitivity coefficient at the 1% level.

The experiment was designed to avoid any bias on the clock frequency due to a perturbing magnetic field that would be sequentially switched between two different values when measurements are performed either on the 9/2→9/2 or on the −9/2→−9/2 transitions. No component producing a magnetic field is switched differently between the mF=9/2 and the mF=−9/2 configurations. The ellipticity of the optical pumping light polarization is rather controlled by addressing alternately different AOMs.

Transients due to the switching of the MOT coils and of the orientation field were checked to take place in less than a few 100 μs, affecting the atomic populations at an insignificant level of 10−6. More generally, the clocks were shown to be immune to other transients by introducing various delays prior to the clock pulse. No frequency shift could be resolved and no loss of stability was observed.

Motional and lattice-induced effects

The motional effects are dramatically suppressed in an OLC by the strong confinement of the atoms. The main residual motional effect is the pulling of the clock resonance by the transitions corresponding to a change of motional quantum number. Together with the pulling by the neighboring Zeeman transitions (for example, mF=7/2→mF′=7/2 and mF=−7/2→mF′=−7/2), the uncertainty due to this effect is at most 5 × 10−17. A possible sliding of the lattice cavity, and therefore of the atoms, during the spectroscopy phase must also be taken into account. This effect was checked to happen at a maximum velocity of v=6 × 10−9 m s−1, inducing frequency shifts <2 × 10−17 in relative value.

The lattices are operated close to their respective magic configuration, and their frequencies are stabilised via a transfer cavity to the |1S0→|3P1 transition. The residual first-order light shifts induced on the atoms are controlled at a level better than 2 × 10−17, whereas the second-order light shifts will not compromise the accuracy of the OLCs down to <1 × 10−17.

Clock laser

The power of the clock pulse is typically a few nW, and the light shift induced by the far-detuned coupling of the clock states with the other atomic levels was shown to be limited to 1.9 × 10−17. The pulse is delivered by an AOM, the initial and final-phase transients are limited to π in <20 μs, inducing a negligible fractional excitation of 10−7 on the atoms. Phase drifts due to slow thermal effects in the AOM in the course of the pulse are observed, but they scale down with the RF power that is used. In our experimental configuration, we use 8 dBm of RF power, and we characterized that this induces a frequency bias of at most 5 × 10−18.

Collisional effects

Atomic density effects in fermionic lattice clocks have drawn attention in the recent years, and it was demonstrated they could be as high as several 10−16 for 1011 atoms cm−3 in some configurations23,25. The atomic density in our lattices is considerably lower (109 atoms  cm−3), and our measurements have confirmed the effect was not a concern at this stage: by measuring differentially the clock frequency in a nominal density configuration (~5 atoms per site) and in a low-density configuration (~0.5 atoms per site), we have put an upper bound of 5 × 10−17 on this effect (Fig. 5). According to the density ratio compared to a previous study,23 the effect is projected to be <10−17.

Figure 5: Study of a possible collisional frequency shift on the strontium clocks.
Figure 5

A possible effect of the atomic density in the lattice is studied by alternating a high (5 atomspersite) and a low (0.5 atompersite) density configuration and by measuring the clock frequency. The data points for Sr1 (blue) and for Sr2 (orange) are represented with their statistical error bars. The averages (blue and orange lines, together with shadings corresponding to the cumulated statistics) show that no effect is resolved at least down to 5 × 10−17.

BBR shift

The frequency response of strontium atoms to the BBR was measured recently36 and validated theoretically40, reducing considerably the corresponding uncertainty to 0.5 × 10−17. The uncertainty on the BBR shift due to the imperfect control of the effective temperature experienced by the atoms is presently the main limitation to the clock accuracy budget. Temperature sensors were distributed around each of the vacuum chambers, and inhomogeneities of 1 K around the temperature of the first chamber (301 K) and of the second chamber (298 K) were observed in the course of the integrations. This results in a −2,310±32 mHz (resp. −2,216±31 mHz) shift on the Sr1 (resp. Sr2) clock.

The thermal radiation of the ovens can possibly affect the atoms, but it is considerably clipped by narrow differential pumping tubes interleaved between the ovens and the atoms. The residual effect was estimated to be at most 3 mHz. This is therefore negligible in relation to the above-mentioned uncertainties of ~30 mHz (7.5 × 10−17).

DC Stark shift

Static charges were trapped on the surface of the mirrors under vacuum, forming the short 60-mm lattice cavity for the Sr2 clock. This induced a DC Stark shift on the atoms inducing a slowly decaying frequency shift on the order of 10−13. The charges were eventually removed from the coatings by photoelectric effect by shining UV light through an optical access of this chamber, the residual effect was characterized to be compatible with 0, with an uncertainty of 1.5 × 10−18 (ref.30).

Optical amplifier spectrum

The residual spontaneous emission background of the tapered amplifiers (TAs) generating the light for the lattices was shown to induce a fluctuating discrepancy in the order of 10−15 between the two clocks. We carried out tests with various TAs and with different ways to control the optical power in the lattices (feedback on the current of the TA, feedback on an acousto-optic modulator or on a setup liquid crystal waveplate+polarization beamsplitter interleaved between the TA and the lattice cavity), and they yielded very different results for the two clocks.

The Sr1 frequency was demonstrated to be immune to the TA choice or to the way to control the lattice depth; we attribute this feature to the geometry of the lattice cavity and particularly to the polarization purity.

On the other hand, the Sr2 provided discrepant results. The unwanted shift induced by a given TA for the clock operated at a given depth was calibrated by differential measurements between two configurations: one configuration with the lattice run with light stemming from the TA, the other configuration with the lattice run with light stemming from the ECDL seeding the TA in the first configuration. The TA is therefore completely bypassed during the spectroscopy phase in the second configuration. The shift was calibrated to be 110±15 mHz at a lattice depth of 100 Er, introducing therefore a 3.5 × 10−17 additional uncertainty in the accuracy budget of Sr2.

Contribution of the absolute frequency measurement chain

The relative height of the different clocks was measured with a precision better than a few 10 cm, thus inducing an uncertainty of at most a few 10−17 on the comparison. The accuracy of the compensated fiber link transferring the signal of the CSO has also been evaluated to be at the 10−17 level. Finally, the measurement of the frequency of the same cavity (USC1062) simultaneously with the titanium-sapphire laser-based comb and with two erbium-fiber-based combs showed that the uncertainty of the frequency transfer by the combs is at most 3 × 10−17.

Remark on uncertainties

Except for the BBR contribution, all the uncertainties have been conservatively evaluated. Once temperature-controlled environments are in place in state-of-the-art OLCs, there seems to be no effect prohibiting their accuracy from progressing by at least one order of magnitude.

Additional information

How to cite this article: Le Targat, R. et al. Experimental realization of an optical second with strontium lattice clocks. Nat. Commun. 4:2109 doi: 10.1038/ncomms3109 (2013).

Change history

  • 31 October 2013

    A correction has been published and is appended to both the HTML and PDF versions of this paper. The error has not been fixed in the paper.

References

  1. 1.

    & Frequency of cesium in terms of ephemeris time. Phys. Rev. Lett. 1, 105–107 (1958).

  2. 2.

    Long-term comparison of caesium fountain primary frequency standards. Metrologia 47, 1–10 (2010).

  3. 3.

    Nobel Lecture: passion for precision. Rev. Mod. Phys. 78, 1297–1309 (2006).

  4. 4.

    Nobel Lecture: defining and measuring optical frequencies. Rev. Mod. Phys. 78, 1279–1295 (2006).

  5. 5.

    et al. Frequency Ratio of Al+ and Hg+ single-ion optical clocks: metrology at the 17th decimal place. Science 319, 1808–1812 (2008).

  6. 6.

    et al. High-accuracy optical clock based on the octupole transition in 171Yb+. Phys. Rev. Lett. 108, 090801 (2012).

  7. 7.

    & 88Sr+ 445-THz single-ion reference at the 10−17 level via control and cancellation of systematic uncertainties and its measurement against the SI Second. Phys. Rev. Lett. 109, 203002 (2012).

  8. 8.

    & Frequency comparison of two high-accuracy Al+ optical clocks. Phys. Rev. Lett. 104, 070802 (2010).

  9. 9.

    & Ultrastable optical clock with neutral atoms in an engineered light shift trap. Phys. Rev. Lett. 91, 173005 (2003).

  10. 10.

    & An optical lattice clock. Nature. 435, 321–324 (2005).

  11. 11.

    et al. Systematic study of the 87Sr clock transition in an optical lattice. Phys. Rev. Lett. 96, 033003 (2006).

  12. 12.

    et al. Accurate optical lattice clock with 87Sr atoms. Phys. Rev. Lett. 97, 130801 (2006).

  13. 13.

    et al. Direct excitation of the forbidden clock transition in neutral 174Yb atoms confined to an optical lattice. Phys. Rev. Lett. 96, 083002 (2006).

  14. 14.

    et al. Sr lattice clock at 1 × 10–16 fractional uncertainty by remote optical evaluation with a Ca clock. Science. 319, 1805–1808 (2008).

  15. 15.

    et al. Spin-1/2 optical lattice clock. Phys. Rev. Lett. 103, 063001 (2009).

  16. 16.

    et al. The 87Sr optical frequency standard at PTB. Metrologia. 48, 399–407 (2011).

  17. 17.

    & Frequency comparison of optical lattice clocks beyond the Dick limit. Nat Photon. 5, 288–292 (2011).

  18. 18.

    et al. Making optical atomic clocks more stable with 10−16-level laser stabilization. Nat Photon. 5, 158–161 (2011).

  19. 19.

    et al. Providing 10−16 short-term stability of a 1.5 μm laser to optical clocks. IEEE Trans. Instrum. Meas. 99, 1–7 (2013).

  20. 20.

    et al. Comparison of two independent Sr optical clocks with 1 × 10−17 stability at 103 s. Phys. Rev. Lett. 109, 230801 (2012).

  21. 21.

    & Quantum state engineering and precision metrology using state-insensitive light traps. Science 320, 1734–1738 (2008).

  22. 22.

    et al. Lattice-induced frequency shifts in Sr optical lattice clocks at the 10−17 level. Phys. Rev. Lett 106, 210801 (2011).

  23. 23.

    et al. Suppression of collisional shifts in a strongly interacting lattice clock. Science 331, 1043–1046 (2011).

  24. 24.

    et al. p-wave cold collisions in an optical lattice clock. Phys. Rev. Lett. 107, 103902 (2011).

  25. 25.

    Decoherence and collisional frequency shifts of trapped bosons and fermions. Phys. Rev. Lett. 103, 113202 (2009).

  26. 26.

    & Coherent transfer of an optical carrier over 251 km. Opt. Lett. 32, 3056–3058 (2007).

  27. 27.

    et al. A 920-kilometer optical fiber link for frequency metrology at the 19th decimal place. Science 336, 441–444 (2012).

  28. 28.

    et al. Ultra-stable long distance optical frequency distribution using the internet fiber network. Opt. Express 20, 23518–23526 (2012).

  29. 29.

    et al. Direct comparison of distant optical lattice clocks at the 10−16 uncertainty. Appl. Phys. Expr. 4, 082203 (2011).

  30. 30.

    & Observation and cancellation of a perturbing dc stark shift in strontium optical lattice clocks. IEEE Trans. Ultr. Ferr. Freq. Contr. 59, 411–415 (2012).

  31. 31.

    & Frequency stabilization to 6 × 10−16 via spectral-hole burning. Nat. Photon. 5, 688–693 (2011).

  32. 32.

    et al. A sub-40-mHz-linewidth laser based on a silicon single-crystal optical cavity. Nat. Photon. 6, 687–692 (2012).

  33. 33.

    & Nondestructive measurement of the transition probability in a Sr optical lattice clock. Phys. Rev. A 79, 061401 (2009).

  34. 34.

    & Shift of 2S1/2 hyperfine splittings due to blackbody radiation. Phys. Rev. A 25, 1233–1235 (1982).

  35. 35.

    et al. High-accuracy measurement of atomic polarizability in an optical lattice clock. Phys. Rev. Lett. 108, 153002 (2012).

  36. 36.

    & High accuracy correction of blackbody radiation shift in an optical lattice clock. Phys. Rev. Lett. 109, 263004 (2012).

  37. 37.

    et al. Determination of the 5d6s 3D1 state lifetime and blackbody-radiation clock shift in Yb. Phys. Rev. A 86, 051404 (2012).

  38. 38.

    & Multipolar theory of blackbody radiation shift of atomic energy levels and its implications for optical lattice clocks. Phys. Rev. A 74, 020502 (2006).

  39. 39.

    & Ytterbium in quantum gases and atomic clocks: van der Waals interactions and blackbody shifts. Phys. Rev. Lett. 109, 230802 (2012).

  40. 40.

    & Blackbody radiation shift in the Sr optical atomic clock. Phys. Rev. A 87, 012509 (2013).

  41. 41.

    et al. Progress in atomic fountains at LNE-SYRTE. IEEE Trans. Ultr. Ferr. Freq. Contr. 59, 391–410 (2012).

  42. 42.

    et al. The stability of an optical clock laser transferred to the interrogation oscillator for a Cs fountain. IEEE Trans. Instr. 58, 1258–1262 (2009).

  43. 43.

    et al. Ultralow noise microwave generation with fiber-based optical frequency comb and application to atomic fountain clock. Appl. Phys. Lett 94, 141105 (2009).

  44. 44.

    et al. New limits on coupling of fundamental constants to gravity using 87Sr optical lattice clocks. Phys. Rev. Lett. 100, 140801 (2008).

  45. 45.

    et al. Improved tests of local position invariance using 87Rb and 133Cs fountains. Phys. Rev. Lett. 109, 080801 (2012).

  46. 46.

    et al. Spatial variation in the fine-structure constant—new results from VLT/UVES. Mon. Not. R. Astron. Soc. 422, 3370–3414 (2012).

  47. 47.

    et al. Geophysical applicability of atomic clocks: direct continental geoid mapping. Geophys. J. Int. 191, 78–82 (2012).

  48. 48.

    & Geodesy and relativity. J. Geod. 82, 133–145 (2008).

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Acknowledgements

SYRTE is CNRS UMR 8630. We acknowledge funding by LNE, CNES, IFRAF, DGA, EMRP project T1 J2.1 OCS, ESA project SOC1, FP7 project SOC2. We thank Christophe Salomon and Thomas Udem for fruitful discussions on the manuscript.

Author information

Affiliations

  1. LNE-SYRTE, CNRS, UPMC, Observatoire de Paris, 61 Avenue de l’Observatoire, 75014 Paris, France

    • R. Le Targat
    • , L. Lorini
    • , Y. Le Coq
    • , M. Zawada
    • , J. Guéna
    • , M. Abgrall
    • , M. Gurov
    • , P. Rosenbusch
    • , D. G. Rovera
    • , B. Nagórny
    • , R. Gartman
    • , P. G. Westergaard
    • , M. Lours
    • , G. Santarelli
    • , A. Clairon
    • , S. Bize
    • , P. Laurent
    • , P. Lemonde
    •  & J. Lodewyck
  2. Istituto Nazionale di Ricerca Metrologica, Strada delle Cacce 91, 10135 Torino, Italy

    • L. Lorini
  3. Institute of Physics, Nicolaus Copernicus University, Grudziadzka 5, PL-87-100 Toruń, Poland

    • M. Zawada
    • , B. Nagórny
    •  & R. Gartman
  4. School of Physics (M013), The University of Western Australia, 35 Stirling Highway, Crawley 6009, Western Australia, Australia

    • M. E. Tobar

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All authors contributed extensively to the work presented in this paper.

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The authors declare no competing financial interests.

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Correspondence to J. Lodewyck.

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https://doi.org/10.1038/ncomms3109

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