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

Published 6 Dec 2018 in physics.ins-det, physics.atom-ph, and physics.optics | (1812.03842v1)

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 Kelvin, reaching $6.5\times10{-17}$ from 0.8 to 80 seconds. We also report for the first time a clear linear dependence of the cavity frequency drift on the incident optical power. The lowest fractional frequency drift of $-3\times10{-19}$/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 $1\times10{-17}$ and fractional linear drift below $1\times10{-19}$/s.

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