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AN OPTICAL FREQUENCY STANDARD WITH ULTRACOLD Ca-ATOMS

机译:具有Ultracold CA-Atoms的光学频率标准

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Optical frequency standards utilizing narrow atomic transitions with Q≈ 10~(12) and low sensitivities to external fields offer the possibility to reach relative uncertainties below 10~(-15). Using ensembles of more than 10~7 neutral alkaline earth atoms laser cooled in a magneto-optical trap, excellent short time stabilities below 10~(-16) in 1 s seem possible. In our optical Ca-frequency standard with an ensemble Doppler cooled to a temperature of 3 mK we have realized a relative uncertainty of 2·10~(-14) limited mainly by a residual Doppler effect of the atomic motion and by the effect of cold collisions. With a new quench cooling method we were able to reduce the temperature to below 10μK. First measurements showed the potential for a reduced uncertainty and an improved stability in utilizing these ultracold atoms in the frequency standard.
机译:光学频率标准利用Q≈10〜(12)的窄原子过渡,对外场的低灵敏度提供了达到10〜(-15)的相对不确定性的可能性。 在磁光阱中冷却超过10〜7中性碱土原子激光的集合,在1 s中优异的短时间稳定率低于10〜( - 16)。 在我们的光学CA频率标准中,通过集合多普勒冷却至3 mk的温度,我们已经实现了2·10〜(-14)的相对不确定性,主要是由原子运动的残留多普勒效应和冷的效果 碰撞。 通过新的淬火冷却方法,我们能够将温度降低至10μk。 首先测量显示出降低不确定性的可能性和在频率标准中利用这些超自然原子的提高稳定性。

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