Quantum correlations between light and the kilogram-mass mirrors of LIGO

Abstract

The measurement of minuscule forces and displacements with ever greater precision is inhibited by the Heisenberg uncertainty principle, which imposes a limit to the precision with which the position of an object can be measured continuously, known as the standard quantum limit1,2,3,4. When light is used as the probe, the standard quantum limit arises from the balance between the uncertainties of the photon radiation pressure applied to the object and of the photon number in the photoelectric detection. The only way to surpass the standard quantum limit is by introducing correlations between the position/momentum uncertainty of the object and the photon number/phase uncertainty of the light that it reflects5. Here we confirm experimentally the theoretical prediction5 that this type of quantum correlation is naturally produced in the Laser Interferometer Gravitational-wave Observatory (LIGO). We characterize and compare noise spectra taken without squeezing and with squeezed vacuum states injected at varying quadrature angles. After subtracting classical noise, our measurements show that the quantum mechanical uncertainties in the phases of the 200-kilowatt laser beams and in the positions of the 40-kilogram mirrors of the Advanced LIGO detectors yield a joint quantum uncertainty that is a factor of 1.4 (3 decibels) below the standard quantum limit. We anticipate that the use of quantum correlations will improve not only the observation of gravitational waves, but also more broadly future quantum noise-limited measurements.

Access options

Rent or Buy article

Get time limited or full article access on ReadCube.

from$8.99

All prices are NET prices.

Fig. 1: Simplified schematic of the experimental setup.
Fig. 2: Spectral density measurements revealing sub-SQL quantum noise.
Fig. 3: Quantum noise spectra at additional squeezing angles of 7°, 24° and 46°.

Data availability

Source data for Figs. 2, 3, Extended Data Figs. 13 and other data pertaining to this study are available from the corresponding authors upon reasonable request.

References

  1. 1.

    Caves, C. M. Quantum-mechanical noise in an interferometer. Phys. Rev. D 23, 1693–1708 (1981).

    ADS  Article  Google Scholar 

  2. 2.

    Braginsky, V. B. & Khalili, F. Y. Quantum nondemolition measurements: the route from toys to tools. Rev. Mod. Phys. 68, 1–11 (1996).

    ADS  MathSciNet  Article  Google Scholar 

  3. 3.

    Braginsky, V. B., Khalili, F. Y. & Thorne, K. S. Quantum Measurement (Cambridge University Press, 1992).

  4. 4.

    Kimble, H. J., Levin, Y., Matsko, A. B., Thorne, K. S. & Vyatchanin, S. P. Conversion of conventional gravitational-wave interferometers into quantum nondemolition interferometers by modifying their input and/or output optics. Phys. Rev. D 65, 022002 (2001).

    ADS  Article  Google Scholar 

  5. 5.

    Unruh, W. G. Quantum Optics, Experimental Gravitation, and Measurement Theory (Plenum, 1982).

  6. 6.

    Buonanno, A. & Chen, Y. Quantum noise in second generation, signal-recycled laser interferometric gravitational-wave detectors. Phys. Rev. D 64, 042006 (2001).

    ADS  Article  Google Scholar 

  7. 7.

    Kwee, P., Miller, J., Isogai, T., Barsotti, L. & Evans, M. Decoherence and degradation of squeezed states in quantum filter cavities. Phys. Rev. D 90, 062006 (2014).

    ADS  Article  Google Scholar 

  8. 8.

    Danilishin, S. et al. Creation of a quantum oscillator by classical control. Preprint at https://arxiv.org/abs/0809.2024 (2008).

  9. 9.

    Purdue, P. & Chen, Y. Practical speed meter designs for quantum nondemolition gravitational-wave interferometers. Phys. Rev. D 66, 122004 (2002).

    ADS  Article  Google Scholar 

  10. 10.

    Møller, C. B. et al. Quantum back-action-evading measurement of motion in a negative mass reference frame. Nature 547, 191–195 (2017).

    ADS  Article  Google Scholar 

  11. 11.

    Purdy, T. P., Peterson, R. W. & Regal, C. A. Observation of radiation pressure shot noise on a macroscopic object. Science 339, 801–804 (2013).

    ADS  CAS  Article  Google Scholar 

  12. 12.

    Suh, J. et al. Mechanically detecting and avoiding the quantum fluctuations of a microwave field. Science 344, 1262–1265 (2014).

    ADS  CAS  Article  Google Scholar 

  13. 13.

    Wilson, D. J. et al. Measurement-based control of a mechanical oscillator at its thermal decoherence rate. Nature 524, 325–329 (2015).

    ADS  CAS  Article  Google Scholar 

  14. 14.

    Teufel, J., Lecocq, F. & Simmonds, R. Overwhelming thermomechanical motion with microwave radiation pressure shot noise. Phys. Rev. Lett. 116, 013602 (2016).

    ADS  CAS  Article  Google Scholar 

  15. 15.

    Cripe, J. et al. Measurement of quantum back action in the audio band at room temperature. Nature 568, 364–367 (2019).

    ADS  CAS  Article  Google Scholar 

  16. 16.

    Sudhir, V. et al. Quantum correlations of light from a room-temperature mechanical oscillator. Phys. Rev. X 7, 031055 (2017).

    Google Scholar 

  17. 17.

    Purdy, T. P., Grutter, K. E., Srinivasan, K. & Taylor, J. M. Quantum correlations from a room-temperature optomechanical cavity. Science 356, 1265–1268 (2017).

    ADS  MathSciNet  CAS  Article  Google Scholar 

  18. 18.

    Mason, D., Chen, J., Rossi, M., Tsaturyan, Y. & Schliesser, A. Continuous force and displacement measurement below the standard quantum limit. Nat. Phys. 15, 745–749 (2019).

    CAS  Article  Google Scholar 

  19. 19.

    Tse, M. et al. Quantum-enhanced advanced LIGO detectors in the era of gravitational-wave astronomy. Phys. Rev. Lett. 123, 231107 (2019).

    ADS  CAS  Article  Google Scholar 

  20. 20.

    Abbott, B. P. et al. Gw150914: the advanced LIGO detectors in the era of first discoveries. Phys. Rev. Lett. 116, 131103 (2016).

    ADS  MathSciNet  CAS  Article  Google Scholar 

  21. 21.

    Sun, L. et al. Characterization of systematic error in advanced LIGO calibration. Preprint at https://arxiv.org/abs/2005.02531 (2020).

  22. 22.

    Kiwamu, I. Time domain implementation of dcpd cross correlation. Technical Note T1700131 (LIGO Virgo, 2017); https://dcc.ligo.org/LIGO-T1700131/public.

Download references

Acknowledgements

LIGO was constructed by the California Institute of Technology and the Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under Cooperative Agreement number PHY-1764464. Advanced LIGO was built under grant number PHY-0823459. The authors gratefully acknowledge the support of the Australian Research Council under the ARC Centre of Excellence for Gravitational Wave Discovery grant number CE170100004, Linkage Infrastructure, Equipment and Facilities grant number LE170100217 and Discovery Early Career Award number DE190100437; the National Science Foundation Graduate Research Fellowship under grant number 1122374; the Science and Technology Facilities Council of the United Kingdom; and the LIGO Scientific Collaboration Fellows programme.

Author information

Affiliations

Authors

Consortia

Contributions

The measurements presented in this paper were performed with the 4-km detector at the LIGO Livingston Observatory using a novel squeezed light source. Haocun Yu performed all of the measurements. Haocun Yu and L.M. carried out the analysis of the data. M. Tse, Haocun Yu and N.K. built and commissioned the squeezed-light sources. L.B. led the squeezed-light upgrade of the LIGO detectors, involving contributions from a large number of people within the LIGO Laboratory, the Australian National University and other members of the LIGO Scientific Collaboration. N.M. led the experimental campaign to measure sub-SQL quantum noise in the Advanced LIGO detector. Haocun Yu, L.M., M. Tse, L.B. and N.M. contributed directly to the preparation of the manuscript.

Corresponding authors

Correspondence to Haocun Yu or L. McCuller.

Ethics declarations

Competing interests

The authors declare no competing interests.

Additional information

Peer review information Nature thanks Albert Schliesser, Valeria Sequino and Kentaro Somiya for their contribution to the peer review of this work.

Publisher’s note Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Extended data figures and tables

Extended Data Fig. 1 Spectral density measurements revealing sub-SQL quantum noise of the interferometer with uncertainties.

The black and brown traces show the measured total noise level of the interferometer with the unsqueezed vacuum state (the reference) and injected squeezing at 35°, respectively. The grey curve shows the classical noise contribution to the total noise of the interferometer, which is independent of the squeezer state. The solid blue curve shows the quantum noise model and includes the 5% uncertainty in the arm power, compensated by the output optical loss to maintain the calibrated sensing function. The inferred quantum noise (green curve) and error bars include all uncertainty terms present in equation (12), as estimated in Methods, including the frequency dependence. The quantum noise model with 35° squeezing (purple line) is shown with the 5% arm power uncertainty (purple shading) and the 0.5-dB uncertainty of the squeezing generated by the squeezer (pink shading). The free-mass SQL is shown by the dashed red line, and the pure QRPN contribution of the interferometer with the unsqueezed vacuum state is shown by the dashed blue line and includes the uncertainty in the arm power.

Extended Data Fig. 2 Squeezing level of the interferometer over the full range of squeezing angles.

Contour plot of squeezing level S*(ϕθψ) detected in the interferometer as a function of the frequency and squeezing angle ϕ (top) and the corresponding theoretical model (bottom). The dashed lines indicate cross-sections in other figures. The green dashed line shows ϕ = 35° in Fig. 2, and the magenta, navy and orange lines correspond to the angles shown in Fig. 3.

Extended Data Fig. 3 Individual and combined estimates of non-stationary noise between measurement segments.

The two upper plots show the relative time variation of noise between each pair of reference and squeezing measurement segments, respectively. The black lines show 2σ or a 95% confidence level. The bottom plot shows the combined non-stationary power defined by equation (14).

Extended Data Table 1 Interferometer and squeezer parameters used for modelling the Advanced LIGO detector in Livingston

Supplementary information

Rights and permissions

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Yu, H., McCuller, L., Tse, M. et al. Quantum correlations between light and the kilogram-mass mirrors of LIGO. Nature 583, 43–47 (2020). https://doi.org/10.1038/s41586-020-2420-8

Download citation

Comments

By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.