M Sackers, O Marchuk, D Dipti, Yu Ralchenko, S Ertmer, S Brezinsek, A Kreter
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引用次数: 0
摘要
激光吸收光谱提供了原子跃迁的高分辨率光谱,揭示了许多通常无法获得的特征。由于奇数同位素 83Kr、129Xe 和 131Xe 的超精细结构,在磁化等离子体中测量到的氪和氙的光谱线形状会受到它们的强烈影响,从而产生比偶数同位素更具挑战性的光谱。在 22.5 mT-90 mT 的磁场范围内,在线性等离子体装置 PSI-2 中测量和分析了源自氪和氙的 J = 2(Kr I 760.4 nm)和 J = 0(Kr I 785.7 nm,Xe I 764.4 nm)的瞬变水平线。对包括这些磁场强度下超频和泽曼相互作用项在内的哈密顿方程进行评估后发现,子级的线性能量移动与磁场的函数以及弱磁场公式提供的恒定相对强度存在偏差。我们证明,使用磁化等离子体中常用的弱磁场近似方法来模拟氙的跃迁,在 ≈50 mT 时变得不够充分。特别是,131Xe 同位素的光谱显示出与弱场结果的明显偏差。不过,对于氪来说,由于奇数同位素的天然丰度较低,情况没有氙那么严重。
Zeeman effect of isotopes of Kr and Xe investigated at the linear plasma device PSI-2
Laser absorption spectroscopy provides high-resolution spectra of atomic transitions that reveal many often inaccessible features. The line shapes of krypton and xenon measured in magnetized plasmas are strongly affected by the contribution of the odd-numbered isotopes 83Kr, 129Xe and 131Xe due to their hyperfine structure, creating more challenging spectra in comparison to even-numbered ones. The lines originating from metastable levels of krypton and xenon with J = 2 (Kr I 760.4 nm) and J = 0 (Kr I 785.7 nm, Xe I 764.4 nm) were measured and analyzed in the linear plasma device PSI-2 in the field range of 22.5 mT–90 mT. Evaluating the Hamiltonian, including hyperfine and Zeeman interaction terms for these magnetic field strengths, unveils a deviation from the linear energy shift of the sublevels as a function of the magnetic field and from constant relative intensities that the weak field formulas provide. We prove that modeling the transitions in Xe using the weak field approximation, frequently used in magnetized plasma, becomes inadequate at ≈50 mT. In particular, the spectra of the 131Xe isotope show pronounced deviations from the weak field results. For krypton, however, the situation is less critical compared to xenon due to the low natural abundance of the odd-numbered isotope.