Short-term stability improvements of an optical frequency standard based on free Ca atoms

POSTER

Abstract

Compared to optical frequency standards featuring trapped ions or atoms in optical lattices, the strength of a standard using freely expanding neutral calcium atoms is not ultimate accuracy but rather short-term stability and experimental simplicity. Recently, a fractional frequency instability of $4 \times 10^{-15}$ at 1 second was demonstrated for the Ca standard at 657 nm~[1]. The short cycle time ($\sim$2 ms) combined with only a moderate interrogation duty cycle ($\sim$15 \%) is thought to introduce excess, and potentially critically limiting technical noise due to the Dick effect---high-frequency noise on the laser oscillator is not averaged away but is instead down-sampled by aliasing. We will present results of two strategies employed to minimize this effect: the reduction of clock laser noise by filtering the master clock oscillator through a high-finesse optical cavity~[2], and an optimization of the interrogation cycle to match our laser's noise spectrum.\\[4pt] [1] Oates et al., \emph{Optics Letters}, \textbf{25}(21), 1603--5 (2000)\\[0pt] [2] Nazarova et al., \emph{J.\ Opt.\ Soc.\ Am.\ B}, \textbf{5}(10), 1632--8 (2008)

Authors

  • Jeff Sherman

    NIST-Boulder

  • Chris Oates