Single Trapped 171Yb+ for Optical Frequency Standards

A. Roy, L. Sharma, H. Rathore, J. Saroha, Neelam, K. Kumari, S. De, S. Panja
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Abstract

An optical clock or frequency standard based on the interrogation of an atomic transition in the optical domain, operates at-1014 Hz is capable of providing orders of magnitude better accuracy than the present primary standard of frequency or time operating in the microwave range. Optical transitions of an ions, confined within a radio frequency ion trap and laser cooled to $\sim \mathrm {m}\mathrm {K}$temperature, provides better long term stability since they are free from Coulomb and intra-atomic interactions. Optical frequency standards have been realized with several ions, e.g., 199Hg+, 171Yb+, 115In+, 88Sr+, 40Ca+, 27Al+ and among those 171Y+ has multiple ultra-narrow optical transitions suitable for serving as frequency standards [1–2]
光频率标准单阱171Yb+
基于对光域原子跃迁的探测的光学时钟或频率标准,工作在1014hz,能够提供比目前在微波范围内工作的频率或时间的主要标准好几个数量级的精度。离子的光学跃迁被限制在射频离子阱和激光冷却到$\sim \ mathm {m}\ mathm {K}$温度内,提供了更好的长期稳定性,因为它们不受库仑和原子内相互作用的影响。采用199Hg+、171Yb+、115In+、88Sr+、40Ca+、27Al+等多种离子实现了光频率标准,其中171Y+具有多个适合作为频率标准的超窄光跃迁[1-2]。
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