冷Ca原子的光缔合

G. Zinner, T. Binnewies, F. Riehle, E. Tiemann
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引用次数: 85

摘要

利用激光冷却原子的光结合光谱被证明是测定原子性质如激发态寿命和基态散射长度的有力工具。碱土中最丰富的同位素表现为非简并基态,没有超细分裂,这有望在很大程度上简化它们的光缔合光谱。这种理论描述上的优势是由光关联实验观察的困难所弥补的。激光冷却碱土的系综比目前大多数光缔合实验中使用的碱土系综更冷,密度更小。Ca的光缔合是通过将Ca的原子对激发到B/sup 1//spl Sigma//sub n//sup +/激发态来实现的,对应于大核距r的原子对4s/sup 2/ /sup 1/S/sub 0/+4s4p /sup 1/P/sub 1/。二聚体受共振偶极相互作用束缚。由于R/sup -3/-势中的加速度,在较小核距处衰变的原子通常有足够的动能离开磁光阱。通过测量依赖于/sup 1/S/sub 0/-/sup 1/P/sub 1/跃迁频率的阱损耗,我们解析了分子的振动和旋转结构。根据观测到的振动能级的位置,校正了部分未解析的旋转结构和基态原子的热能分布,得出了能级4s4p /sup 1/P/sub 1/的原子辐射衰减率/spl gamma/=2.180(11)/spl middot/10/sup 8/ s/sup -1/,其不确定度比以前的测量结果降低了近一个数量级。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Photoassociation of cold Ca atoms
Photoassociative spectroscopy using laser cooled atoms proved to be a powerful tool for the determination of atomic properties such as excited state lifetimes and ground state scattering lengths. The most abundant isotopes of alkaline earths show a non-degenerate ground state with no hyperfine splitting, which is expected to simplify their photoassociation spectra to a great extent. This advantage in the theoretical description is paid for by difficulties in the experimental observation of photoassociation. The ensembles of laser cooled alkaline earths are less cold and less dense than those of e.g. alkalines which were used in most of the photoassociation experiments until now. Photoassociation of Ca is achieved by exciting atomic pairs to the B/sup 1//spl Sigma//sub n//sup +/ excited state of Ca corresponding to an atomic pair 4s/sup 2/ /sup 1/S/sub 0/+4s4p /sup 1/P/sub 1/ at large nuclear distances R. The dimer is bound by the resonant dipole interaction. Due to acceleration in this R/sup -3/-potential, atoms decaying at a smaller nuclear distance usually have sufficient kinetic energy to leave the magneto-optical trap. By measuring the trap loss dependent on the frequency of a photoassociation laser red-detuned to the /sup 1/S/sub 0/-/sup 1/P/sub 1/ transition we resolved the vibrational and rotational structure of the molecule. From the positions of the observed vibrational levels, corrected for the partially unresolved rotational structure and the thermal energy distribution of the ground state atoms, the atomic radiation decay rate /spl gamma/=2.180(11)/spl middot/10/sup 8/ s/sup -1/ of level 4s4p /sup 1/P/sub 1/ is derived with an uncertainty reduced by nearly one order of magnitude compared to previous measurements.
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