超正弦帕申-巴克机制下 D2 激发时^{87}$Rb 中细观结构改变的碰撞

Clare R. Higgins, Danielle Pizzey, Ifan G. Hughes
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引用次数: 0

摘要

我们研究了在 350 K 的热蒸汽中 D2 激发时,^{87}$Rb 蒸汽中的精细结构变化碰撞;将原子置于 0.6 T 的轴向磁场中,以进入超细帕申-巴克机制。在 D2 线的光激发之后,由于缓冲碰撞的结果,发生了放热转移 5P$_{3/2}$\rightarrow$5P$_{1/2}$;$^{87}$Rb 随后在 D1 转变上发射了一个光子。我们使用单光子计数仪器来监测 D1 荧光,并使用乙烯滤光片来提供高光谱分辨率。通过研究 D2 激发激光扫描时的 D1 荧光,我们发现在碰撞转移过程中,原子的量子数 $m_{J}$ 发生了变化,但是核自旋投影量子数 $m_{I}$ 却保持不变。一个简单的动力学模型结合了碰撞中的恢复系数,解释了发生碰撞的原子的速度分布变化以及由此产生的荧光线形。实验是在一个名义上 "无缓冲气 "的蒸气室中进行的;我们的结果表明,在这种介质中,细微结构变化的碰撞是很重要的,并指出了在热蒸气中进行量子光学实验可能产生的影响,这些热蒸气会产生双梯形构型的纠缠光子对,以及太阳物理磁光滤波器。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Fine-structure changing collisions in $^{87}$Rb upon D2 excitation in the hyperfine Paschen-Back regime
We investigate fine structure changing collisions in $^{87}$Rb vapour upon D2 excitation in a thermal vapour at 350 K; the atoms are placed in a 0.6 T axial magnetic field in order to gain access to the hyperfine Pashen-Back regime. Following optical excitation on the D2 line, the exothermic transfer 5P$_{3/2}$$\rightarrow$5P$_{1/2}$ occurs as a consequence of buffer-gas collisions; the $^{87}$Rb subsequently emits a photon on the D1 transition. We employ single-photon counting apparatus to monitor the D1 fluorescence, with an etalon filter to provide high spectral resolution. By studying the D1 fluorescence when the D2 excitation laser is scanned, we see that during the collisional transfer process the $m_{J}$ quantum number of the atom changes, but the nuclear spin projection quantum number, $m_{I}$, is conserved. A simple kinematic model incorporating a coefficient of restitution in the collision accounted for the change in velocity distribution of atoms undergoing collisions, and the resulting fluorescence lineshape. The experiment is conducted with a nominally ``buffer-gas free" vapour cell; our results show that fine structure changing collisions are important with such media, and point out possible implications for quantum-optics experiments in thermal vapours producing entangled photon pairs with the double ladder configuration, and solar physics magneto-optical filters.
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