Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autorschaft

  • S. Dörscher
  • N. Huntemann
  • R. Schwarz
  • R. Lange
  • E. Benkler
  • B. Lipphardt
  • U. Sterr
  • E. Peik
  • C. Lisdat

Externe Organisationen

  • Physikalisch-Technische Bundesanstalt (PTB)
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer015005
FachzeitschriftMETROLOGIA
Jahrgang58
Ausgabenummer1
PublikationsstatusVeröffentlicht - Feb. 2021
Extern publiziertJa

Abstract

We report direct measurements of the frequency ratio of the 642 THz 2S1/2(F = 0)-2F7/2(F = 3) electric octupole transition in 171Yb+ and the 429 THz 1S0 -3P0 transition in 87Sr. A series of 107 measurements has been performed at the Physikalisch-Technische Bundesanstalt between December 2012 and October 2019. Long-term variations of the ratio are larger than expected from the individual measurement uncertainties of few 1017. The cause of these variations remains unknown. Even taking these into account, we find a fractional uncertainty of the frequency ratio of 2.5 × 1017, which improves upon previous knowledge by one order of magnitude. The average frequency ratio is νYb+ /νSr = 1.495 991 618 544 900 537(38). This represents one of the most accurate measurements between two different atomic species to date.

ASJC Scopus Sachgebiete

Zitieren

Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock. / Dörscher, S.; Huntemann, N.; Schwarz, R. et al.
in: METROLOGIA, Jahrgang 58, Nr. 1, 015005, 02.2021.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Dörscher, S, Huntemann, N, Schwarz, R, Lange, R, Benkler, E, Lipphardt, B, Sterr, U, Peik, E & Lisdat, C 2021, 'Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock', METROLOGIA, Jg. 58, Nr. 1, 015005. https://doi.org/10.1088/1681-7575/abc86f
Dörscher, S., Huntemann, N., Schwarz, R., Lange, R., Benkler, E., Lipphardt, B., Sterr, U., Peik, E., & Lisdat, C. (2021). Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock. METROLOGIA, 58(1), Artikel 015005. https://doi.org/10.1088/1681-7575/abc86f
Dörscher S, Huntemann N, Schwarz R, Lange R, Benkler E, Lipphardt B et al. Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock. METROLOGIA. 2021 Feb;58(1):015005. doi: 10.1088/1681-7575/abc86f
Dörscher, S. ; Huntemann, N. ; Schwarz, R. et al. / Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock. in: METROLOGIA. 2021 ; Jahrgang 58, Nr. 1.
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title = "Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock",
abstract = "We report direct measurements of the frequency ratio of the 642 THz 2S1/2(F = 0)-2F7/2(F = 3) electric octupole transition in 171Yb+ and the 429 THz 1S0 -3P0 transition in 87Sr. A series of 107 measurements has been performed at the Physikalisch-Technische Bundesanstalt between December 2012 and October 2019. Long-term variations of the ratio are larger than expected from the individual measurement uncertainties of few 10−17. The cause of these variations remains unknown. Even taking these into account, we find a fractional uncertainty of the frequency ratio of 2.5 × 10−17, which improves upon previous knowledge by one order of magnitude. The average frequency ratio is νYb+ /νSr = 1.495 991 618 544 900 537(38). This represents one of the most accurate measurements between two different atomic species to date.",
keywords = "Frequency ratio, Optical clocks, Strontium lattice clock, Ytterbium ion clock",
author = "S. D{\"o}rscher and N. Huntemann and R. Schwarz and R. Lange and E. Benkler and B. Lipphardt and U. Sterr and E. Peik and C. Lisdat",
note = "Funding information: [ We thank T Legero, D Matei, and S H{\"a}fner for operating the Si-2 laser system, C Grebing for operating one of the optical frequency combs during the first few measurements, and N Lemke, S Falke, A Al-Masoudi, M Abdel Hafiz, and C Sanner for their contributions to operating the clocks during some measurements. We acknowledge support by the project 18SIB05 ROCIT, which has received funding from the EMPIR programme co-financed by the Participating States and from the European Union's Horizon 2020 Research and Innovation Programme, and by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany's Excellence Strategy-EXC-2123 QuantumFrontiers-390837967 and CRC 1227 DQ-mat within project B02. We thank T Legero, D Matei, and S H{\"a}fner for operating the Si-2 laser system, C Grebing for operating one of the optical frequency combs during the first few measurements, and N Lemke, S Falke, A Al-Masoudi, M Abdel Hafiz, and C Sanner for their contributions to operating the clocks during some measurements. We acknowledge support by the project 18SIB05 ROCIT, which has received funding from the EMPIR programme co-financed by the Participating States and from the European Union{\textquoteright}s Horizon 2020 Research and Innovation Programme, and by the Deutsche Forschungs-gemeinschaft (DFG, German Research Foundation) under Germany{\textquoteright}s Excellence Strategy—EXC-2123 QuantumFron-tiers—390837967and CRC 1227 DQ-mat within project B02",
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T1 - Optical frequency ratio of a 171Yb+ single-ion clock and a 87Sr lattice clock

AU - Dörscher, S.

AU - Huntemann, N.

AU - Schwarz, R.

AU - Lange, R.

AU - Benkler, E.

AU - Lipphardt, B.

AU - Sterr, U.

AU - Peik, E.

AU - Lisdat, C.

N1 - Funding information: [ We thank T Legero, D Matei, and S Häfner for operating the Si-2 laser system, C Grebing for operating one of the optical frequency combs during the first few measurements, and N Lemke, S Falke, A Al-Masoudi, M Abdel Hafiz, and C Sanner for their contributions to operating the clocks during some measurements. We acknowledge support by the project 18SIB05 ROCIT, which has received funding from the EMPIR programme co-financed by the Participating States and from the European Union's Horizon 2020 Research and Innovation Programme, and by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany's Excellence Strategy-EXC-2123 QuantumFrontiers-390837967 and CRC 1227 DQ-mat within project B02. We thank T Legero, D Matei, and S Häfner for operating the Si-2 laser system, C Grebing for operating one of the optical frequency combs during the first few measurements, and N Lemke, S Falke, A Al-Masoudi, M Abdel Hafiz, and C Sanner for their contributions to operating the clocks during some measurements. We acknowledge support by the project 18SIB05 ROCIT, which has received funding from the EMPIR programme co-financed by the Participating States and from the European Union’s Horizon 2020 Research and Innovation Programme, and by the Deutsche Forschungs-gemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy—EXC-2123 QuantumFron-tiers—390837967and CRC 1227 DQ-mat within project B02

PY - 2021/2

Y1 - 2021/2

N2 - We report direct measurements of the frequency ratio of the 642 THz 2S1/2(F = 0)-2F7/2(F = 3) electric octupole transition in 171Yb+ and the 429 THz 1S0 -3P0 transition in 87Sr. A series of 107 measurements has been performed at the Physikalisch-Technische Bundesanstalt between December 2012 and October 2019. Long-term variations of the ratio are larger than expected from the individual measurement uncertainties of few 10−17. The cause of these variations remains unknown. Even taking these into account, we find a fractional uncertainty of the frequency ratio of 2.5 × 10−17, which improves upon previous knowledge by one order of magnitude. The average frequency ratio is νYb+ /νSr = 1.495 991 618 544 900 537(38). This represents one of the most accurate measurements between two different atomic species to date.

AB - We report direct measurements of the frequency ratio of the 642 THz 2S1/2(F = 0)-2F7/2(F = 3) electric octupole transition in 171Yb+ and the 429 THz 1S0 -3P0 transition in 87Sr. A series of 107 measurements has been performed at the Physikalisch-Technische Bundesanstalt between December 2012 and October 2019. Long-term variations of the ratio are larger than expected from the individual measurement uncertainties of few 10−17. The cause of these variations remains unknown. Even taking these into account, we find a fractional uncertainty of the frequency ratio of 2.5 × 10−17, which improves upon previous knowledge by one order of magnitude. The average frequency ratio is νYb+ /νSr = 1.495 991 618 544 900 537(38). This represents one of the most accurate measurements between two different atomic species to date.

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DO - 10.1088/1681-7575/abc86f

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VL - 58

JO - METROLOGIA

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