2017
DOI: 10.1364/ao.56.005436
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Medium-finesse optical cavity for the stabilization of Rydberg lasers

Abstract: We describe the design, construction, and characterization of a medium-finesse Fabry-Pérot cavity for simultaneous frequency stabilization of two lasers operating at 960 and 780 nm wavelengths, respectively. The lasers are applied in experiments with ultracold rubidium Rydberg atoms, for which a combined laser linewidth similar to the natural Rydberg linewidth (≈ 10 kHz) is desired. The cavity, with a finesse of ≈ 1500, is used to reduce the linewidth of the lasers to below this level. By using a spacer made o… Show more

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Cited by 20 publications
(18 citation statements)
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“…Finally, we have demonstrated excellent long-term stability with a linear drift of ∼ 1 Hz/s relative to an atomic reference. These measurement are competitive against doubly-stabilized optical clocks [32,37] and offer an order of magnitude improvement compared to similar cavity stabilized Rydberg laser systems [35,36].…”
Section: Discussionmentioning
confidence: 99%
“…Finally, we have demonstrated excellent long-term stability with a linear drift of ∼ 1 Hz/s relative to an atomic reference. These measurement are competitive against doubly-stabilized optical clocks [32,37] and offer an order of magnitude improvement compared to similar cavity stabilized Rydberg laser systems [35,36].…”
Section: Discussionmentioning
confidence: 99%
“…respectively). The excitation lasers are stabilized using a reference cavity and have a linewidth of typically 10 kHz [40]. The 780-nm beam is sent through a combination of a mechanical shutter and an acousto-optical modulator for excellent contrast and fast switching times, respectively.…”
Section: Collective Onset and Rydberg Blockadementioning
confidence: 99%
“…6(a) shows an improvement of four orders of magnitude in the normalized spectral density of optical fluctuation √ S ν /ν 0 compared to its value at room temperature. However, even if the spectral density of noise is largely reduced by working at cryogenic temperature, the Q of Si 3 N 4 rings such as those we study is generally too low to consider them as viable candidates for reference cavities [32]. Going forward, recent improvements in the Q of thick Si 3 N 4 [33][34][35] resonators, as well as earlier work on thin Si 3 N 4 resonators with quality factors approaching 10 8 [36], suggest future potential to combine such higher Q with cryogenic operation towards reference cavity applications.…”
mentioning
confidence: 90%