Crystalline optical cavity at 4  K with thermal-noise-limited instability and ultralow drift

John Robinson, E. Oelker, William R. Milner, Wei Zhang, Thomas Legero, Dan Matei, F. Riehle, Uwe Sterr, Jun Ye

Optica · 2019 · 168 citations · 17 references

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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.

References

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