Zugriffsnummer 50399
Dokumenttyp Zeitschriftenartikel Open Access Gold
Peer Review mit Peer Review
Sprache Englisch
Titel Evaluation of a 88Sr+ optical clock with a direct measurement of the blackbody radiation shift and determination of the clock frequency
Autor(in); Institution
Steinel, Martin; 4.4, Zeit und Frequenz, PTB-Braunschweig
Shao, Hu; 4.4, Zeit und Frequenz, PTB-Braunschweig
Filzinger, Melina; 4.4, Zeit und Frequenz, PTB-Braunschweig
Lipphardt, Burghard; 4.4, Zeit und Frequenz, PTB-Braunschweig
Brinkmann, Malte; QUEST, FG 2, Quantenuhren und komplexe Systeme, PTB-Braunschweig
Didier, Alexandre; QUEST, FG 2, Quantenuhren und komplexe Systeme, PTB-Braunschweig
Mehlstäubler, Tanja E.; QUEST, FG 2, Quantenuhren und komplexe Systeme, PTB-Braunschweig; Leibniz Universität Hannover, Hannover, GERMANY
Lindvall, Thomas; VTT Technical Research Centre of Finland, VTT, FINLAND
Peik, Ekkehard; 4.4, Zeit und Frequenz, PTB-Braunschweig
Huntemann, Nils; 4.4, Zeit und Frequenz, PTB-Braunschweig
Quelle/Jahr Physical Review Letters: 131 (2023), 8, 083002-1 - 083002-6
Artikelnummer 083002
ISSN 1079-7114 (online) ; 0031-9007 (print)
DOI
URL
Verlag College Park, Md.: American Physical Society (APS)
Freie Schlagworte atom and ion cooling ; atomic, optical and lattice clocks ; laser spectroscopy ; quantum sensing ; relativistic and quantum electrodynamic effects in atoms ; molecules and ions ; Stark effect ; Zeeman effect
Zusammenfassung We report on an evaluation of an optical clock that uses the 2S1/2→2D5/2 transition of a single 88Sr+ ion as the reference. In contrast to previous work, we estimate the effective temperature of the blackbody radiation that shifts the reference transition directly during operation from the corresponding frequency shift and the well-characterized sensitivity to thermal radiation. We measure the clock output frequency against an independent 171Yb+ ion clock, based on the 2S1/2(F≡0) → 2F7/2 (F. ident. 3) electric octupole (E3) transition, and determine the frequency ratio with a total fractional uncertainty of 2.3 ×10-17. Relying on a previous measurement of the 171Yb+ (E3) clock frequency, we find the absolute frequency of the 88Sr+ clock transition to be 444 779 044 095 485.277(59) Hz. Our result reduces the uncertainty by a factor of 3 compared with the previously most accurate measurement and may help to resolve so far inconsistent determinations of this value. We also show that for three simultaneously interrogated 88Sr+ ions, the increased number causes the expected improvement of the short-term frequency instability of the optical clock without degrading its systematic uncertainty.
Kostenfreier Zugang Open Access Gold
Rechteinformation CC BY 4.0 ; Creative Commons Attribution 4.0 License
Themenbereich der Metrologie Zeit und Frequenz
Innovationscluster Quantentechnologie
Geschäftsfelder Grundlagen der Metrologie
Förderinformationen (1) Förderername: European Commission (EC)
Förderer ID: 0000 0001 2242 8989
Förderer ID Typ: ISNI
Förderprogramm: EMPIR 2020 Fundamental
Titel der Förderung: 20FUN01: TSCAC: Two-species composite atomic clocks
Förderungsnummer: 20FUN01
Förderinformationen (2) Förderername: European Commission (EC)
Förderer ID: 0000 0001 2242 8989
Förderer ID Typ: ISNI
Förderprogramm: EMPIR 2017 Fundamental
Titel der Förderung: 17FUN07: CC4C: Coulomb Crystals for Clocks
Förderungsnummer: 17FUN07
Förderinformationen (3) Förderername: Deutsche Forschungsgemeinschaft (DFG)
Förderer ID: 0000 0001 2096 9829
Förderer ID Typ: ISNI
Förderprogramm: SFB 1227 DQ-mat
Titel der Förderung: Project B02
Förderungsnummer: 274200144
Förderinformationen (4) Förderername: Max-Planck, RIKEN, PTB Center for Time, Constants, and Fundamental Symmetries (C-TCFS)

Zitierung

Steinel, M., Shao, H., Filzinger, M., Lipphardt, B., Brinkmann, M., Didier, A., Mehlstäubler, T. E., Lindvall, T., Peik, E., & Huntemann, N. (2023). Evaluation of a ⁸⁸Sr⁺ optical clock with a direct measurement of the blackbody radiation shift and determination of the clock frequency. Physical Review Letters, 131(8), 083002-1–083002-6. https://doi.org/10.1103/PhysRevLett.131.083002

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