Abstract

Crystalline optical cavities are the foundation of today’s state-of-the-art ultrastable lasers. Building on our previous silicon cavity effort, we now achieve the fundamental thermal-noise-limited stability for a 6 cm long silicon cavity cooled to 4 K, reaching 6.5×10−17 from 0.8 s to 80 s. We also report for the first time, to the best of our knowledge, a clear linear dependence of the cavity frequency drift on incident optical power. The lowest fractional frequency drift of −3×10−19/s is attained at a transmitted power of 40 nW, with an extrapolated drift approaching zero in the absence of optical power. These demonstrations provide a promising direction to reach a new performance domain for stable lasers, with stability better than 1×10−17 and fractional linear drift below 1×10−19/s.

Highlights

  • In this Letter, we present critical advancements in the development of a cryogenic ultrastable optical cavity

  • Short-term noise is optimized by reducing the impact of vibrations and other technical noise sources, unveiling the thermal noise floor for the first time for a 4 K optical cavity

  • The 6 cm long cavity is enclosed in a three-stage cryogenic thermal damping system formed by an outer radiation shield and two inner shields near 4 K [15]

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Summary

Introduction

In this Letter, we present critical advancements in the development of a cryogenic ultrastable optical cavity. Short-term noise is optimized by reducing the impact of vibrations and other technical noise sources, unveiling the thermal noise floor for the first time for a 4 K optical cavity. Through a frequency comparison with a reference laser (named Si3) [14], we demonstrate instability at the thermal noise floor of 6.5 × 10−17 for averaging times of 0.8 s to 80 s.

Results
Conclusion

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