The space optical clocks project: Development of high-performance transportable and breadboard optical clocks and advanced subsystems

S. Schiller, A. Görlitz, A. Nevsky, S. Alighanbari, S. Vasilyev, C. Abou-Jaoudeh, G. Mura, T. Franzen, U. Sterr, S. Falke, C. Lisdat, E. Rasel, A. Kulosa, S. Bize, J. Lodewyck, G. Tino, N. Poli, M. Schioppo, K. Bongs, Y. Singh, P. Gill, G. Barwood, Yuri B. Ovchinnikov, J. Stuhler, W. Kaenders, C. Braxmaier, R. Holzwarth, A. Donati, S. Lecomte, D. Calonico, F. Levi
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引用次数: 43

Abstract

The use of ultra-precise optical clocks in space (“master clocks”) will allow for a range of new applications in the fields of fundamental physics (tests of Einstein's theory of General Relativity, time and frequency metrology by means of the comparison of distant terrestrial clocks), geophysics (mapping of the gravitational potential of Earth), and astronomy (providing local oscillators for radio ranging and interferometry in space). Within the ELIPS-3 program of ESA, the “Space Optical Clocks” (SOC) project aims to install and to operate an optical lattice clock on the ISS towards the end of this decade, as a natural follow-on to the ACES mission, improving its performance by at least one order of magnitude. The payload is planned to include an optical lattice clock, as well as a frequency comb, a microwave link, and an optical link for comparisons of the ISS clock with ground clocks located in several countries and continents. Undertaking a necessary step towards optical clocks in space, the EU-FP7-SPACE-2010-1 project no. 263500 (SOC2) (2011–2015) aims at two “engineering confidence“, accurate transportable lattice optical clock demonstrators having relative frequency instability below 1×10−15 at 1 s integration time and relative inaccuracy below 5×10−17. This goal performance is about 2 and 1 orders better in instability and inaccuracy, respectively, than today's best transportable clocks. The devices will be based on trapped neutral ytterbium and strontium atoms. One device will be a breadboard. The two systems will be validated in laboratory environments and their performance will be established by comparison with laboratory optical clocks and primary frequency standards. In order to achieve the goals, SOC2 will develop the necessary laser systems - adapted in terms of power, linewidth, frequency stability, long-term reliability, and accuracy. Novel solutions with reduced space, power and mass requirements will be implemented. Some of the laser systems will be developed towards particularly high compactness and robustness levels. Also, the project will validate crucial laser components in relevant environments. In this paper we present the project and the results achieved during the first year.
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空间光学时钟项目:开发高性能可移动和面包板光学时钟和先进子系统
在空间使用超精密光学钟("主钟")将在基础物理学(检验爱因斯坦的广义相对论、通过比较遥远的地面时钟进行时间和频率计量)、地球物理学(绘制地球引力势)和天文学(为空间无线电测距和干涉测量提供本地振荡器)等领域实现一系列新的应用。在ESA的ELIPS-3计划中,“空间光学时钟”(SOC)项目的目标是在本十年末在国际空间站上安装和运行一个光学晶格时钟,作为ACES任务的自然后续,将其性能提高至少一个数量级。有效载荷计划包括一个光学晶格时钟、一个频率梳、一个微波链路和一个光学链路,用于将国际空间站时钟与位于几个国家和大陆的地面时钟进行比较。EU-FP7-SPACE-2010-1项目向太空光学时钟迈出了必要的一步。263500 (SOC2)(2011-2015)的目标是两个“工程信心”,精确的可移动晶格光钟演示,在1 s积分时间的相对频率不稳定性低于1×10−15,相对不准确性低于5×10−17。这种目标性能在不稳定性和不准确性方面分别比当今最好的可移动时钟好2个和1个数量级。该装置将基于捕获的中性钇和锶原子。一个设备是面包板。这两个系统将在实验室环境中进行验证,并通过与实验室光钟和主要频率标准进行比较来确定其性能。为了实现目标,SOC2将开发必要的激光系统-在功率,线宽,频率稳定性,长期可靠性和精度方面进行调整。减少空间、功率和质量要求的新颖解决方案将被实施。一些激光系统将朝着特别高的紧凑性和坚固性水平发展。此外,该项目将在相关环境中验证关键的激光组件。在本文中,我们介绍了该项目和第一年取得的成果。
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