22–24 févr. 2016
Paris
Fuseau horaire Europe/Paris

The 87Sr optical lattice clock at PTB

22 févr. 2016, 16:00
3h
Paris

Paris

77 avenue Denfert Rochereau 75014 Paris

Orateur

Ali Al-Masoudi (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany)

Description

We report on the implementation of a cryogenic optical lattice clock based on the ${}^{1}S_{0} \leftrightarrow {}^{3}P_{0}$ transition of ${}^{87}$Sr at PTB. While the atomic response to the blackbody radiation (BBR) field experienced by the atoms has been well characterized [1], our existing lattice clock is now limited to a total systematic uncertainty of $2 \times 10^{-17}$ [2] by our knowledge of the effective BBR field itself. Several groups [3-5] have already demonstrated approaches to control the BBR-induced frequency shifts to the level of few parts in 1018 and below, near room temperature or at cryogenic temperatures. The lattice clock at PTB is successively being upgraded to a fully cryogenic lattice clock. In a first step, we have implemented a cryogenic environment into which the atoms are transport-ed for interrogation. This has allowed us to achieve similar control of the BBR-induced fre-quency shifts and is expected to enable a total systematic uncertainty below $1 \times 10^{-17}$. A sub-sequent upgrade to a new physics package will remove the need for transporting the atoms and provide generally improved control of systematic effects to enable operation of the lattice clock at systematic uncertainties of few parts in $10^{-18}$ and better. The instability of our optical lattice clock is $1.6 \times 10^{-16} / \sqrt{\tau/\mathrm{s}}$ [6], which is limited by Dick effect. We present a novel interrogation scheme to minimize the Dick effect by interrogating the atoms longer than the coherent time of the clock laser. This work is supported by QUEST, by DFG within CRC 1128 (geo-Q) and RTG 1729, and by EMRP within ITOC and QESOCAS. The EMRP is jointly funded by the EMRP-participating countries within EURAMET and the European Union. References: [1] T. Middelmann, S. Falke, C. Lisdat, and U. Sterr, “High accuracy correction of blackbody radiation shift in an optical lattice clock”, Phys. Rev. Lett., vol. 109, p. 263004, 2012. [2] C. Lisdat, et al., “A clock network for geodesy and fundamental science”, arXiv: 1511.07735, 2015. [3] I. Ushijima, M. Takamoto, M. Das, T. Ohkubo, and H. Katori, “Cryogenic optical lattice clocks”, Nature Phot., vol. 9, p. 185, 2015. [4] T. L. Nicholson et al., “Systematic evaluation of an atomic clock at $2 \times 10^{-18}$ total uncertainty”, Nature Com., vol. 6, p. 6896, 2015. [5] K. Beloy et al., “An atomic clock with $1 \times 10^{-18}$ room-temperature blackbody Stark uncertainty”, Phys. Rev. Lett., vol. 113, p. 260801, 2014. [6] A. Al-Masoudi, S. Dörscher, S. Häfner, U. Sterr, Ch. Lisdat, Phys. Rev. A 92, 063814 (2015).

Auteur principal

Ali Al-Masoudi (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany)

Co-auteurs

Christian Lisdat (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany) Roman Schwarz (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany) Sebastian Häfner (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany) Sören Dörscher (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany) Uwe Sterr (Physikalisch-Technische Bundesanstalt, 38116 Braunschweig, Germany)

Documents de présentation

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