Details
Original language | English |
---|---|
Article number | 015005 |
Journal | METROLOGIA |
Volume | 58 |
Issue number | 1 |
Publication status | Published - Feb 2021 |
Externally published | Yes |
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
ASJC Scopus subject areas
- Engineering(all)
- General Engineering
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In: METROLOGIA, Vol. 58, No. 1, 015005, 02.2021.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
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.
KW - Frequency ratio
KW - Optical clocks
KW - Strontium lattice clock
KW - Ytterbium ion clock
UR - http://www.scopus.com/inward/record.url?scp=85099239392&partnerID=8YFLogxK
U2 - 10.1088/1681-7575/abc86f
DO - 10.1088/1681-7575/abc86f
M3 - Article
AN - SCOPUS:85099239392
VL - 58
JO - METROLOGIA
JF - METROLOGIA
SN - 0026-1394
IS - 1
M1 - 015005
ER -