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In an experimental system of 87Sr atomic optical lattice clock, the free-running 698 nm diode laser is locked in an ultra-stable optical reference cavity to obtain the ultra-stable narrow linewidth laser with good short-term frequency stability. The ultra-stable optical reference cavity, which is usually composed of glass material doped with titanium dioxide for ultra-low thermal expansion coefficient and two highly reflective fused quartz mirrors, is called ULE cavity. The cavity length is prone to being affected by mechanical vibration, temperature change, airflow, etc. The stability of the cavity length determines the stability of the final laser frequency. Near the room temperature, there exists a special temperature point for the ultra-low expansion glass material, at which temperature its thermal expansion coefficient becomes zero, which is called the zero-crossing temperature. At the zero-crossing temperature, the length of the ULE cavity is not sensitive to the temperature fluctuation, reaching a minimum value, and the laser locked to the ULE cavity has a minimum frequency drift. In order to reduce the influence of temperature on the laser frequency instability, the zero-crossing temperature of the ultra-stable optical reference cavity of 698 nm ultra-stable narrow linewidth laser system is measured by using the clock transition spectrum of the strontium atomic optical lattice clock. The frequency drift and frequency instability of the 698 nm ultra-stable narrow linewidth laser system at zero-crossing temperature are measured by using the change of the in-loop locked clock frequency of strontium atomic optical lattice clock. By scanning the atomic clock transition frequencies at different temperatures, the clock transition spectra at different temperatures are obtained. The second order polynomial fitting of the central frequency of the clock transition spectrum with the change curve of temperature is carried out, and the zero-crossing temperature of the 698 nm ultra-stable narrow linewidth laser system ULE cavity is measured to be 30.63 ℃. At the zero-crossing temperature, the 698 nm ultra-stable narrow linewidth laser frequency is used for in-loop locking of 87Sr atomic optical lattice clock. The linear drift rate of the ULE cavity in the 698 nm ultra-stable narrow linewidth laser system is measured to be 0.15 Hz/s, and the frequency instability of the 698 nm ultra-stable narrow linewidth laser system is 1.6 × 10–15 at an average time of 3.744 s. The determination of ULE cavity zero-crossing temperature for the 698 nm ultra-stable narrow linewidth laser system is of great significance in helping to not only improve the instability of the laser system, but also increase the instability of 87Sr optical lattice clock system. In the future, we will improve the temperature control system of the ULE cavity in the 698 nm clock laser system, enhancing the temperature control accuracy of the ULE cavity and reducing the measurement error, thus achieving a more accurate zero-crossing temperature and further improving the frequency instability of the 698 nm ultra-stable narrow linewidth laser system.
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Keywords:
- ultra-stable optical reference cavity /
- frequency drift /
- clock transition spectra /
- zero-crossing temperature
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图 1 测量零温漂点的实验装置
Figure 1. Schematic setup for zero-crossing temperature measurement.
图 2 归一化钟跃迁谱线
Figure 2. Normalized excitation spectra of clock transition.
图 3 698 nm超稳窄线宽激光系统ULE腔零漂温点的测量
Figure 3. Measurements at different controlled temperatures clock transition spectra.
图 4 (a) 698 nm激光频率随时间的漂移; (b) 698 nm激光系统的频率不稳定度
Figure 4. (a) 698 nm laser frequency drift with the time; (b) fractional frequency instability of the 698 nm laser.
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[1] Ludlow A D, Boyd M M, Ye J, Peik E, Schmidt P O 2015 Rev. Mod. Phys. 87 637
Google Scholar
[2] Blatt S, Ludlow A D, Campbell G K, et al. 2008 Phys. Rev. Lett. 100 140801
Google Scholar
[3] Godun R M, Nisbet-Jones P B R, Jones J M, King S A, Johnson L A, Margolis H S, Szymaniec K, Lea S N, Bongs K, Gill P 2014 Phys. Rev. Lett. 113 210801
Google Scholar
[4] Huntemann N, Lipphardt B, Tamm C, Gerginov V, Weyers S, Peik E 2014 Phys. Rev. Lett. 113 210802
Google Scholar
[5] Derevianko A, Pospelov M 2014 Nat. Phys. 10 933
Google Scholar
[6] Wcisło P, Morzyński P, Bober M, Cygan A, Lisak D, Ciuryło R, Zawada M 2016 Nat. Astron. 1 0009
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Google Scholar
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Google Scholar
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Google Scholar
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Google Scholar
[12] Jiang Y Y, Ludlow A D, Lemke N D, Fox R W, Sherman J A, Ma L S, Oates C W 2011 Nat. Photonics 5 158
Google Scholar
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Google Scholar
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Google Scholar
Lin Y G, Fang Z J 2018 Acta Phys. Sin. 67 160604
Google Scholar
[15] Muller H, Peters A, Chu S 2010 Nature 463 926
Google Scholar
[16] Wang C, Ji Z, Gong T, et al. 2019 J. Phys. D: Appl. Phys. 52 455104
Google Scholar
[17] Thomas L, Thomas K, Uwe S 2010 J. Opt. Soc. Am. B 27 914
Google Scholar
[18] Zhang J, Luo Y X, Ouyang B, Deng K, Lu Z H, Luo J 2013 Eur. Phys. J. D 67 46
Google Scholar
[19] Berthold J W, Jacobs S F 1976 Appl. Opt. 15 2334
[20] 卢晓同, 李婷, 孔德欢, 王叶兵, 常宏 2019 物理学报 68 233401
Google Scholar
Lu X T, Li T, Kong D H, Wang Y B, Chang H 2019 Acta Phys. Sin. 68 233401
Google Scholar
[21] Lu X T, Yin M J, Li T, Wang Y B, Chang H 2020 Appl. Sci. 10 1440
Google Scholar
[22] 高峰, 刘辉, 许鹏, 王叶兵, 田晓, 常宏 2014 物理学报 63 140704
Google Scholar
Gao F, Liu H, Xu P, Wang Y B, Tian X, Chang H 2014 Acta Phys. Sin. 63 140704
Google Scholar
[23] Drever R W P, Hall J L, Kowalski F V, Hough J, Ford G M, Munley A J, Ward H 1983 Appl. Phys. B 31 97
[24] Wang Y B, Yin M J, Ren J, Xu Q F, Lu B Q, Han J X, Guo Y, Chang H 2018 Chin. Phys. B 27 023701
Google Scholar
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