[1] Gill P. Optical frequency standards[J]. Metrologia, 42, S125-S137(2005).

[2] Ludlow A D, Boyd M M, Ye J et al. Optical atomic clocks[J]. Reviews of Modern Physics, 87, 637701(2015).

[3] Eisele C, Nevsky A Y, Schiller S. Laboratory test of the isotropy of light propagation at the 10-17 level[J]. Physical Review Letters, 103, 090401(2009).

[4] Godun R M, Nisbet-Jones P B R, Jones J M et al. Frequency ratio of two optical clock transitions in 171Yb+ and constraints on the time variation of fundamental constants[J]. Physical Review Letters, 113, 210801(2014).

[5] LIGO Scientific Collaboration. LIGO: The laser interferometer gravitational-wave observatory[J]. Reports on Progress in Physics, 72, 076901(2009).

[6] LIGO scientific collaboration and VIRGO Collaboration. Observation of gravitational waves from a binary black hole merger[J]. Physical Review Letters, 116, 061102(2016).

[7] Hanes G R, Baird K M, Deremigis J. Stability, reproducibility, and absolute wavelength of a 633-nm He-Ne laser stabilized to an iodine hyperfine component[J]. Applied Optics, 12, 1600-1605(1973).

[8] Hall J L, Ma L S, Taubman M et al. Stabilization and frequency measurement of the I2-stabilized Nd : YAG laser[J]. IEEE Transactions on Instrumentation and Measurement, 48, 583-586(1999).

[9] Drever R W P, Hall J L, Kowalski F V et al. Laser phase and frequency stabilization using an optical resonator[J]. Applied Physics B, 31, 97-105(1983).

[10] Numata K, Kemery A, Camp J. Thermal-noise limit in the frequency stabilization of lasers with rigid cavities[J]. Physical Review Letters, 93, 250602(2004).

[11] Zhang J, Wu W, Shi X H et al. Design verification of large time constant thermal shields for optical reference cavities[J]. Review of Scientific Instruments, 87, 023104(2016).

[12] Dai X J, Jiang Y Y, Hang C et al. Thermal analysis of optical reference cavities for low sensitivity to environmental temperature fluctuations[J]. Optics Express, 23, 5134-5146(2015).

[13] Sanjuan J, Gürlebeck N, Braxmaier C. Mathematical model of thermal shields for long-term stability optical resonators[J]. Optics Express, 23, 17892-17908(2015).

[14] Chen L S, Hall J L, Ye J et al. Vibration-induced elastic deformation of Fabry-Perot cavities[J]. Physical Review A, 74, 053801(2006).

[15] Millo J, Magalhães D V, Mandache C et al. Ultrastable lasers based on vibration insensitive cavities[J]. Physical Review A, 79, 053829(2009).

[16] Nazarova T, Riehle F, Sterr U. Vibration-insensitive reference cavity for an ultra-narrow-linewidth laser[J]. Applied Physics B, 83, 531-536(2006).

[17] Webster S A, Oxborrow M, Gill P. Vibration insensitive optical cavity[J]. Physical Review A, 75, 011801(2007).

[18] Ludlow A D, Huang X, Notcutt M et al. Compact, thermal-noise-limited optical cavity for diode laser stabilization at 1 × 10-15[J]. Optics Letters, 32, 641-643(2007).

[19] Webster S, Gill P. Force-insensitive optical cavity[J]. Optics Letters, 36, 3572-3574(2011).

[20] Xiao R, Xu Y Q, Wang Y et al. Transportable 30 cm optical cavity based ultrastable lasers with beating instability of 2 × 10-16[J]. Applied Physics B, 128, 220(2022).

[21] Antonini P, Okhapkin M, Göklü E et al. Test of constancy of speed of light with rotating cryogenic optical resonators[J]. Physical Review A, 71, 050101(2005).

[22] Robinson J M, Oelker E, Milner W R et al. Crystalline optical cavity at 4 K with thermal-noise-limited instability and ultralow drift[J]. Optica, 6, 240-243(2019).

[23] Jin L. Development of Lasers with 10-16 Frequency Instability and Theoretical Exploration on 10-18 Laser Frequency Instability via Four-wave Mixing[D](2019).

[24] Jiang C H. Research on Key Technologies of 698 nm Ultra-stable Laser Based on 30 cm Long Cavity[D](2019).

[25] Sebastian H, Stephan F, Christian G et al. 8 × 10-17 fractional laser frequency instability with a long room-temperature cavity[J]. Optics Letters, 40, 2112-2115(2015).