4.8 Article

Intercontinental comparison of optical atomic clocks through very long baseline interferometry

期刊

NATURE PHYSICS
卷 17, 期 2, 页码 223-+

出版社

NATURE PORTFOLIO
DOI: 10.1038/s41567-020-01038-6

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资金

  1. European Metrology Program for Innovation and Research (EMPIR) [15SIB03 OC18, 15SIB05 OFTEN, 17IND14 WRITE, 18SIB05 ROCIT]
  2. Italian Ministry of Education, University and Research
  3. Horizon 2020 Marie Skodowska-Curie Research and Innovation Staff Exchange (MSCA-RISE) project Q-SENSE [691156]
  4. European Union's Horizon 2020 research and innovation programme
  5. EMPIR Participating States
  6. French National Research Agency under the LABEX Cluster of Excellence FIRST-TF [ANR-10-LABX-48-01]
  7. high-speed research network JGN
  8. high-speed research network Internet2
  9. high-speed research network TransPAC
  10. high-speed research network APAN
  11. high-speed research network GEANT
  12. high-speed research network GARR
  13. Research Coordination Committee
  14. National Astronomical Observatory of Japan (NAOJ)
  15. National Institutes of Natural Sciences (NINS)
  16. Marie Curie Actions (MSCA) [691156] Funding Source: Marie Curie Actions (MSCA)

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The study demonstrates that very long baseline interferometry (VLBI) can be used to compare intercontinental optical clocks by observing extragalactic radio sources, overcoming limitations of satellite transfer techniques. The new system's performance surpasses satellite techniques, paving the way for future stable international clock comparisons.
The comparison of distant atomic clocks is foundational to international timekeeping, global positioning and tests of fundamental physics. Optical-fibre links allow the most precise optical clocks to be compared, without degradation, over intracontinental distances up to thousands of kilometres, but intercontinental comparisons remain limited by the performance of satellite transfer techniques. Here we show that very long baseline interferometry (VLBI), although originally developed for radio astronomy and geodesy, can overcome this limit and compare remote clocks through the observation of extragalactic radio sources. We developed dedicated transportable VLBI stations that use broadband detection and demonstrate the comparison of two optical clocks located in Italy and Japan separated by 9,000 km. This system demonstrates performance beyond satellite techniques and can pave the way for future long-term stable international clock comparisons. Very long baseline interferometry is used to compare two optical clocks located in Japan and Italy through the observation of extragalactic radio sources. This approach overcomes limitations of the performance of satellite transfer techniques.

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