Ultra-stable laser with average fractional frequency drift rate below 5\times 10^{-19}/\mathrm{s}

Ultra-stable laser with average fractional frequency drift rate below

Christian Hagemann    Christian Grebing    Christian Lisdat    Stephan Falke    Thomas Legero    Uwe Sterr Corresponding author: uwe.sterr@ptb.de    Fritz Riehle Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, Germany
Corresponding author: uwe.sterr@ptb.de
   Michael J. Martin    Jun Ye JILA, National Institute of Standards and Technology and University of Colorado, Department of Physics, 440 UCB, Boulder, Colorado 80309, USA
Abstract

Cryogenic single-crystal optical cavities have the potential to provide highest dimensional stability. We have investigated the long-term performance of an ultra-stable laser system which is stabilized to a single-crystal silicon cavity operated at 124 K. Utilizing a frequency comb, the laser is compared to a hydrogen maser that is referenced to a primary caesium fountain standard and to the optical lattice clock at PTB. With fractional frequency instabilities of for averaging times of to and the stability of this laser, without any aid from an atomic reference, surpasses the best microwave standards for short averaging times and is competitive with the best hydrogen masers for longer times of one day. The comparison of modeled thermal response of the cavity with measured data indicates a fractional frequency drift below  /s, which we do not expect to be a fundamental limit.

pacs:
(140.3425) Laser stabilization; (140.4780) Optical resonators; (120.3940) Metrology;

Advancements in ultra-stable oscillators push forward a wide range of cutting-edge experiments such as atomic clockwork san99 (); nic12 (); hin13 (), or tests of fundamental physics eis09 (); cho10a (), and applications in deep space navigation gro10a () or very-long baseline interferometry nan11 () at shorter wavelength doe11 (). For these applications, both the short term instability on few second time scale and the long term stability over one day are essential. So far, mostly frequency standards and oscillators operating in the microwave domain, such as hydrogen masers and cryogenic microwave oscillators for improved short term stability gro10a (), are used.

Recently, oscillators operating in the optical domain have demonstrated fractional frequency instabilities with Allan deviation of at  s nic12 (); mar13 (). For most of the applications mentioned above it would be desirable if the short term stability of the oscillator could be kept also at much longer times without the need of a sophisticated optical atomic clock. However, aging in the commonly employed ultra-low expansion (ULE) glass cavities leads to a poorly predictable non-linear shrinkage of the resonator length on the order of to dub09 (), which translates to frequency drifts of the cavity resonance. Due to residual temperature fluctuations of the cavity, the day-to-day predictability of the cavity drift rate remains at dub09 (). With material creep being absent in single-crystals, crystalline reference cavities are a promising candidate for laser sources that keep their stability in the long-term. Already in 1998 dimensional stabilities of have been achieved employing a single-crystal sapphire cavity at 4.3 K sto98 () and short-term stability of see97 (). However, the automatic liquid-nitrogen refill processes led to fractional frequency excursions of every few hours.

Figure 1: Response of silicon cavity temperature inferred from the laser frequency after the temperature of the cryogenic shield was increased by  mK (black points). The red trace shows a fit of the expected response function. The inset shows the setup with the employed thermal shields represented by an equivalent electric circuit of the thermal model.

Figure 2: (a): Measured temperature deviation of the cryogenic shield. The arrows indicate when the liquid nitrogen storage Dewar of the cryostat was refilled. (b): Deviation of the cavity from zero-crossing temperature. (c): Absolute frequency of the laser stabilized to the silicon cavity with respect to the zero-crossing frequency at d. The frequency was referenced to a hydrogen maser (moving average, window:  s) which was referenced to the Cs fountain clock. The inset shows a zoom of between days 56.5 and 63 including frequency data derived from comparison with the Sr optical lattice clock (red dots).

Recently, we have set up a laser system based on a single-crystal cryogenic silicon cavity. Silicon possesses a zero-crossing in the Coefficient of Thermal Expansion (CTE) at a relatively high temperature of , which greatly reduces the technical demands of cooling. This laser system has demonstrated a short-term stability of the modified Allan deviation all81 () for averaging times of to kes12a (). The crystalline nature also lets us expect high long-term stability kes12a (). Here we present our measurements with this system obtained over an extended period of time, where the frequency of the laser system has been compared to the Sr optical lattice clock at PTB fal11 (); fal13 () and to a hydrogen maser which is referenced to a primary Cs fountain clock ger10 ().

To minimize the effect of any remaining drift of the cavity temperature on its length, operating the cavity as close as possible to the zero CTE temperature is crucial. For small deviations the length and frequency of the silicon cavity depend on its temperature according to

(1)

where is the minimum length of the cavity at  K, and is the slope of the CTE around kes12a (). A low-vibration cryostat employing cold nitrogen gas has been developed which provides a cryogenic actively controlled shield at with sub-millikelvin temperature stability. An additional passive shield further dampens residual temperature fluctuations. Adjusting the cryostat temperature to is quite cumbersome in the present setup, as no temperature sensor is attached to the silicon cavity to best preserve its vibration-insensitive mounting design and avoid local heating. Only the temperature at the bottom of the actively controlled shield was measured. As there are temperature gradients across that shield, a cavity temperature corresponds to a temperature about K below , which is taken into account in our analysis. With knowledge of and assuming that is highly constant, the cavity temperature can be estimated using Eq. (1) from the observed absolute laser frequency . Following this approach, we can use the response of the cavity frequency to a  mK step of to determine the thermal dynamics of the system (Fig. 1), which behaves as a second order thermal low-pass:

(2)
(3)

with time constants , and . From the thermal response of the cavity to a temperature step on the cryogenic shield (red curve in Fig. 1) and the known heat capacities , , we find the thermal resistivities , , and the time constants  d,  d, and  d. The thermal model allows to calculate the cavity temperature from the measured .

With the knowledge of the dynamics of the thermal system we can rapidly tune the silicon cavity to , which we did at the beginning of a frequency comparison of three months duration (Fig.2). From an initial laser frequency measurement, temperature offsets of  mK and  mK were determined. To quickly increase , was rapidly raised by 1 K and subsequently lowered by 0.9 K once has increased by 33 mK (mark A). slightly overshot its zero-crossing temperature, settling at mK within twenty days (see Fig.2(b)). At mark B a failure of the cryostat’s temperature control interrupted the thermalization of the system leading to an increased temperature 18 mK within the next days. Shortly before the frequency comb became unavailable due to maintenance, a deliberate temperature decrease of the cryo-shield by  mK (mark C) over one day was introduced to better approach . During the measurement period the temperature response of the silicon cavity was recorded via absolute frequency measurement of the laser stabilized to the cavity (see Fig.2(c)).

From these data we have estimated the stability of the system: Between the two intentional changes of the cryo-shield temperature between mark A and C, over 70 days the laser frequency remained within 600 Hz, which would correspond to an average fractional frequency drift of . A more thorough investigation confirms this rough estimate: When plotting the laser frequency as a function of the calculated cavity temperature (Fig.3) the curve shows the expected parabolic dependency once a constant frequency drift of  Hz/d (/s) is corrected in the data. Possible causes for the residual negative drift corresponding to a change of optical length of fm/d could be isothermal creep of the resonator mirror coatings or buildup of adsorbed layers from the residual gas on the mirror surfaces. The minor deviation of an exact parabolic shape may be due to mechanical relaxations of the cavity mount as a result of the cryostat failure. The lowest drift was observed between day 56 and day 63 (see inset of Fig.2(c)), where the average frequency drift of the laser was  Hz/s () due to compensation of drift and temperature variation. The frequency instability compared to the hydrogen maser (corrected for its drift by comparison to the Cs fountain clock) is shown in Fig. 4. Similar results are obtained after removal of a linear cavity drift from all other data sets, where the temperature was unperturbed. Up to  s, the instability curve follows the typical performance of such type of maser (dashed line) while the moderate increase in frequency instability from  s to  s indicates a contribution from the laser system.

Figure 3: Measured cavity frequency vs. calculated cavity temperature offset from the CTE crossing (light blue symbols) using the temporal data shown in Fig 2 that start near label A. To describe the behavior expected from the silicon thermal expansion (dashed line), a constant drift of Hz/d (Hz/s) had to be assumed (drift-removed data shown as dark blue symbols). The characters refer to the temperature perturbations indicated in Fig. 2.

Figure 4: Fractional frequency instability of the frequency data shown in the inset of Fig. 2. The red curves show the Allan deviations of the two longest continuous data sets from the comparison to the Sr clock (during days 59 and 62). The black dashed lines show the expected instabilities of a typical hydrogen maser and the Sr clock. The blue dotted line shows the Allan deviation expected from thermal noise.

The laser instability for shorter averaging times was inferred from a frequency comparison with a lattice clock which was operational for several times in this time interval (inset of Fig.2(c) red traces). The correlation with frequency excursions observed with the maser indicates that the instability observed in Fig. 4 above  s is originating from the Si-cavity laser. During these measurements the lattice clock instability was ; about a factor of two bigger than its optimal stability hag13 (), as the duty cycle of the clock was reduced to lower the systematic uncertainties during a frequency comparison fal13 (). The observed instability of the Si-cavity laser system is below for averaging times longer than one minute and reaches the -level at averaging times above  s. After that the instability varies depending on the actual frequency fluctuations of the laser that occur at the time the strontium clock was available for comparison.

The increase of laser instability between  s and  s is not yet understood and is not a property of the maser. Although Residual Amplitude Modulation (RAM) from the fiber-coupled phase modulator is actively canceled in the setup kes12a (), there might be uncompensated RAM and frequency pulling of the cavity resonance from parasitic reflections. As the finesse of the TEM-mode was poor (80 000), we employed the TEM-mode for cavity-locking kes12 (). Thus parasitic effects from beam pointing cannot be ruled out as such effects had been observed previously. Also temperature fluctuations during a day would show up at this time scale.

In conclusion, with fractional frequency instabilities of for averaging times of to and the stability of this laser surpasses the best microwave standards for short averaging times. With an average daily drift of estimated from the two frequency values at the CTE zero-crossing after points A and C, it outperforms the best cryogenic sapphire microwave oscillators showing /d tob06 () and its stability is also competitive with the best hydrogen masers for times of up to one day.

The demonstrated frequency stability of a silicon single-crystal stabilized laser in the different regimes of averaging times does not represent a fundamental limit. In a second silicon cavity system that is currently under construction, a higher finesse cavity will allow a corresponding reduction of the influence of RAM and other parasitic effects that might result from the employment of the TEM-mode for cavity-locking. It has been shown recently that the influence of the RAM on the frequency stability can be further reduced to a fraction of of a cavity linewidth zha14 (). This second cavity can be operated with reduced laser power, with less heating of the cavity from the absorbed laser power that currently amounts to mK from W absorbed power. An optimized distribution of improved temperature sensors will enable a more careful adjustment and monitoring of the cavity temperature.

With these optimizations it seems feasible to realize an ultra-stable oscillator that provides fractional frequency stabilities below from a second to a day. For example, such an ultra-stable oscillator would be useful in the comparison between optical frequency standards and primary Cs clocks, that requires averaging times of several days to reach their uncertainty of . With the improvements now under way it will also be possible to elucidate the nature of the observed temporal drift rate of about  Hz/d. Its constant value observed up to now would furthermore allow to apply a feed forward correction loop to achieve an even higher long-term stability. In the region of several days around day 60 (Fig. 2 c) where the drift rate is compensated by another – presumably temperature – effect a fractional instability of was observed. As optical clocks still lack sufficient reliability for unattended long-term operation, the very small observed long-term drift rate will allow such a laser to act as a flywheel oscillator that could bridge longer gaps in measurement and which would facilitate comparisons between optical clocks and long-term measurement with microwave time standards.

Acknowledgments

We thank A. Bauch and S. Weyers for providing the frequency data between Cs fountains and H masers. The cryogenic silicon cavity laser system employed in this work was developed jointly by the JILA Physics Frontier Center (NSF) and the National Institute of Standards and Technology (NIST), the Centre for Quantum Engineering and Space-Time Research (QUEST) and Physikalisch-Technische Bundesanstalt (PTB). We acknowledge funding from the DARPA QuASAR program, the European Community ERA-NET-Plus Programme (Grant No. 217257), the European Community 7 Framework Programme (Grant Nos. 263500) and the European Metrology Research Programme (EMRP) under IND14. The EMRP is jointly funded by the EMRP participating countries within EURAMET and the European Union. J. Y. acknowledges support from the Humboldt foundation.

References

  • (1) G. Santarelli, P. Laurent, P. Lemonde, A. Clairon, A. G. Mann, S. Chang, A. N. Luiten, and C. Salomon, ‘‘Quantum projection noise in an atomic fountain: A high stability cesium frequency standard,” Phys. Rev. Lett. 82, 4619–4622 (1999).
  • (2) T. Nicholson, M. Martin, J. Williams, B. Bloom, M. Bishof, M. Swallows, S. Campbell, and J. Ye, “Comparison of two independent Sr optical clocks with stability at  s,” Phys. Rev. Lett. 109, 230801 (2012).
  • (3) N. Hinkley, J. A. Sherman, N. B. Phillips, M. Schioppo, N. D. Lemke, K. Beloy, M. Pizzocaro, C. W. Oates, and A. D. Ludlow, “An atomic clock with instability,” Science 341, 1215–1218 (2013).
  • (4) C. Eisele, A. Y. Nevsky, and S. Schiller, “Laboratory test of the isotropy of light propagation at the level,” Phys. Rev. Lett. 103, 090401 (2009).
  • (5) C. W. Chou, D. B. Hume, T. Rosenband, and D. J. Wineland, “Optical clocks and relativity,” Science 329, 1630 – 1633 (2010).
  • (6) S. Grop, P. Y. Bourgeois, N. Bazin, Y. Kersalé, E. Rubiola, C. Langham, M. Oxborrow, D. Clapton, S. Walker, J. De Vicente, and V. Giordano, “ELISA: A cryocooled 10 GHz oscillator with frequency stability,” Rev. Sci. Instrum. 81, 025102 (2010).
  • (7) N. R. Nand, J. G. Hartnett, E. N. Ivanov, and G. Santarelli, “Ultra-stable very-low phase-noise signal source for very long baseline interferometry using a cryocooled sapphire oscillator,” IEEE Trans. Microw. Theory Tech. 59, 2978–2986 (2011).
  • (8) S. Doeleman, T. Mai, A. E. E. Rogers, J. G. Hartnett, M. E. Tobar, and N. Nand, “Adapting a cryogenic sapphire oscillator for very long baseline interferometry,” Publ. Astron. Soc. Pac. 123, 582–595 (2011).
  • (9) M. J. Martin, M. Bishof, M. D. Swallows, X. Zhang, C. Benko, J. von Stecher, A. V. Gorshkov, A. M. Rey, and J. Ye, “A quantum many-body spin system in an optical lattice clock,” Science 341, 632–636 (2013).
  • (10) P. Dubé, A. Madej, J. Bernard, L. Marmet, and A. Shiner, “A narrow linewidth and frequency-stable probe laser source for the Sr single ion optical frequency standard,” Appl. Phys. B 95, 43–54 (2009).
  • (11) R. Storz, C. Braxmaier, K. Jäck, O. Pradl, and S. Schiller, “Ultrahigh long-term dimensional stability of a sapphire cryogenic optical resonator,” Opt. Lett. 23, 1031–1033 (1998).
  • (12) S. Seel, R. Storz, G. Ruoso, J. Mlynek, and S. Schiller, “Cryogenic optical resonators: A new tool for laser frequency stabilization at the 1 Hz level,” Phys. Rev. Lett. 78, 4741–4744 (1997).
  • (13) D. W. Allan and J. Barnes, “A modified “Allan variance” with increased oscillator characterization ability,” in “Proceedings of the 35 Ann. Freq. Control Symposium,” (Electronic Industries Association, Ft. Monmouth, NJ 07703, 1981), pp. 470–475. For corrections see D. Sullivan, D. Allan, D. Howe, and F. Walls, “Characterization of clocks and oscillators,” NIST tech. note 1337, NIST, U.S Department of Commerce, National Institute of Standards and Technology (1990). Online available at http://tf.nist.gov/cgi-bin/showpubs.pl..
  • (14) T. Kessler, C. Hagemann, C. Grebing, T. Legero, U. Sterr, F. Riehle, M. J. Martin, L. Chen, and J. Ye, “A sub-40-mHz-linewidth laser based on a silicon single-crystal optical cavity,” Nature Photonics 6, 687–692 (2012).
  • (15) S. Falke, H. Schnatz, J. S. R. Vellore Winfred, T. Middelmann, S. Vogt, S. Weyers, B. Lipphardt, G. Grosche, F. Riehle, U. Sterr, and C. Lisdat, “The Sr optical frequency standard at PTB,” Metrologia 48, 399–407 (2011).
  • (16) S. Falke, N. Lemke, C. Grebing, B. Lipphardt, S. Weyers, V. Gerginov, N. Huntemann, C. Hagemann, A. Al-Masoudi, S. Häfner, S. Vogt, U. Sterr, and C. Lisdat, “A strontium lattice clock with inaccuracy and its frequency,” arXiv:1312.3419 [physics.atom-ph] (2013). Subm. to NJP.
  • (17) V. Gerginov, N. Nemitz, S. Weyers, R. Schröder, R. D. Griebsch, and R. Wynands, “Uncertainty evaluation of the caesium fountain clock PTB-CSF2,” Metrologia 47, 65–79 (2010).
  • (18) C. Hagemann, C. Grebing, T. Kessler, S. Falke, N. Lemke, C. Lisdat, H. Schnatz, F. Riehle, and U. Sterr, “Providing short-term stability of a m laser to optical clocks,” IEEE Trans. Instrum. Meas. 62, 1556–1562 (2013).
  • (19) T. Kessler, T. Legero, and U. Sterr, “Thermal noise in optical cavities revisited,” J. Opt. Soc. Am. B 29, 178–184 (2012).
  • (20) M. E. Tobar, E. N. Ivanov, C. R. Locke, P. L. Stanwix, J. G. Hartnett, A. N. Luiten, R. B. Warrington, P. T. H. Fisk, M. A. Lawn, M. J. Wouters, S. Bize, G. Santarelli, P. Wolf, A. Clairon, and P. Guillemot, “Long-term operation and performance of cryogenic sapphire oscillators,” IEEE Trans. Ultrason. Ferroelectr. Freq. Control 53, 2386–2393 (2006).
  • (21) W. Zhang, M. J. Martin, C. Benko, J. L. Hall, J. Ye, C. Hagemann, T. Legero, U. Sterr, F. Riehle, G. D. Cole, and M. Aspelmeyer, “Reduction of residual amplitude modulation to for frequency-modulation and laser stabilization,” Opt. Lett. 39, 1980–1983 (2014).
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
338543
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description