The Sodium Doublet钠双线
The magnitude of the spin-orbit interaction has the form μzB = μBSzLz. In the case of the sodium doublet, the difference in energy for the 3p3/2 and 3p1/2 comes from a change of 1 unit in the spin orientation with the orbital part presumed to be the same. The change in energy is of the form 自旋-轨道相互作用的幅度形式为 μ z B = μ B S z L z 。在钠双重态的情况下,3p 3/2 和 3p 1/2 的能量差来自于自旋方向的变化为 1 单位,而轨道部分被假定相同。能量的变化形式为
ΔE = μBgB = 0.0021 eV ΔE = μ B gB = 0.0021 eV(专名或术语) where μB is the Bohr magneton and g is the electron spin g-factor with value very close to 2. This gives an estimate of the internal magnetic field needed to produce the observed splitting: 其中 μ_B 是玻尔磁子,g 是电子自旋 g 因子,其值非常接近 2。这给出了产生观察到的分裂所需的内部磁场的估计值:
μBgB = (5.79 x 10-5 eV/T)2B = 0.0021 eV μ B gB = (5.79 × 10⁻⁵ eV/T)²B = 0.0021 eV B = 18 Tesla B = 18特斯拉 This is a very large magnetic field by laboratory standards. Large magnets with dimensions over a meter, used for NMR and ESR experiments, have magnetic fields on the order of a Tesla. 这在实验室标准下是一个非常大的磁场。用于核磁共振和电子自旋共振实验的大尺寸磁体,其磁场强度通常在特斯拉量级。
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Index Other spectra References Thornton & Rex Sec 9.2 Serway, Moses, Moyer Sec 8.3 索引 其他光谱 参考文献 Thornton & Rex 第9章第2节 Serway, Moses, Moyer 第8章第3节 | ||||
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The Sodium Zeeman Effect钠塞曼效应
The sodium spectrum is dominated by the bright doublet known as the Sodium D-lines at 588.9950 and 589.5924 nanometers. From the energy level diagram it can be seen that these lines are emitted in a transition from the 3p to the 3s levels. 钠的光谱主要由两条明亮的双线主导,称为钠D线,波长分别为588.9950纳米和589.5924纳米。从能级图可以看出,这些线是由3p能级向3s能级跃迁发出的。
The size of the magnetic energy contribution depends upon a geometrical factor called the Lande' g-factor. The values for the relevant quantum numbers and the associated values for the Lande' g-factor are shown in the table below. 磁能贡献的大小取决于一个称为兰德 g 因子的几何因子。相关量子数的值及其对应的兰德 g 因子值如下面的表格所示。
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Sodium Zeeman Effect: Early Observations钠塞曼效应:早期观测
The splitting of the sodium doublet in the presence of an external magnetic field was observed by Pieter Zeeman in 1896, and the effect was subsequently named the Zeeman effect. It is remarkable that so much detailed spectroscopy was done long before the Bohr theory, and perhaps even more remarkable that Zeeman's first study of the sodium Zeeman splitting was done the year before J. J.Thomson's discovery of the electron in 1897. 在外部磁场存在的情况下,钠双线的分裂现象是由皮特·塞曼于1896年观测到的,这一效应随后被命名为塞曼效应。令人惊讶的是,在波尔理论提出之前就已经进行了如此详细的光谱学研究,也许更令人惊讶的是,塞曼对钠塞曼分裂的第一项研究是在1897年汤姆森发现电子的前一年进行的。
After Thomson's work, Zeeman and Lorentz did further study of the influence of magnetic fields on the spectral emissions from atoms. By analysis of the splitting of the sodium doublet, they were able to demonstrate that the charge to mass ratio of the charge responsible for the splitting was the same as Thomson's electron. This was the first direct demonstration that electrons were involved in the production of the spectral line emissions. 在汤姆森的研究之后, Zeeman 和 Lorentz 进一步研究了磁场对原子发射光谱的影响。通过分析钠双线的分裂,他们证明了导致分裂的电荷的电荷与质量比与汤姆森发现的电子的电荷与质量比相同。这是首次直接证明电子参与了光谱线的产生。
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Index Reference Leighton Ch 2 索引参考莱顿第二章 | ||
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