Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

The Sodium Doublet

钠双线
The well known bright doublet which is responsible for the bright yellow light from a sodium lamp may be used to demonstrate several of the influences which cause splitting of the emission lines of atomic spectra. The transition which gives rise to the doublet is from the 3p to the 3s level, levels which would be the same in the hydrogen atom. The fact that the 3s (orbital quantum number = 0) is lower than the 3p (l=1) is a good example of the dependence of atomic energy levels on angular momentum. The 3s electron penetrates the 1s shell more and is less effectively shielded than the 3p electron, so the 3s level is lower (more tightly bound). The fact that there is a doublet shows the smaller dependence of the atomic energy levels on the total angular momentum . The 3p level is split into states with total angular momentum j=3/2 and j=1/2 by the magnetic energy of the electron spin in the presence of the internal magnetic field caused by the orbital motion. This effect is called the spin-orbit effect. In the presence of an additional externally applied magnetic field, these levels are further split by the magnetic interaction, showing dependence of the energies on the z-component of the total angular momentum. This splitting gives the Zeeman effect for sodium.
众所周知的明亮双线,它负责钠灯发出的明亮黄色光,可用于演示几种导致原子光谱发射线分裂的影响。产生双线的跃迁是从3p到3s能级,这些能级在氢原子中会是相同的。3s(轨道量子数=0)比3p(l=1)低,这是原子能级对角动量依赖性的良好例子。3s电子更深入地穿透1s壳层,因此比3p电子更不被有效屏蔽,所以3s能级更低(更紧密地结合)。双线的存在表明原子能级对总角动量的依赖性较小。在内部磁场(由轨道运动引起)的作用下,3p能级被电子自旋的磁能分裂成总角动量j=3/2和j=1/2的态。这种效应称为自旋-轨道效应。在存在额外外部施加的磁场时,这些能级进一步被磁相互作用分裂,显示出能量对总角动量z分量的依赖性。这种分裂导致钠的塞曼效应。

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。
More on sodium spectrum
钠光谱的更多内容
Sodium Zeeman effect
钠塞曼效应
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 sodium doublet is further spit by the application of an external magnetic field ( Zeeman effect). Using the vector model for total angular momentum, the splitting is seen to produce one level for each possible value of the z-component of the total angular momentum J.
钠双线进一步被外加磁场(塞曼效应)分裂。利用总角动量的矢量模型,分裂现象显示出每个可能的总角动量J的z分量对应一个电平。

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。
Term
术语
JLSgL
3p3/23/211/24/3
3p1/21/211/22/3
3s1/21/201/22

Examination of the size of the Lande g-factor gL for the three levels will show why the splittings of the different levels are different in magnitude. The selection rules explain why the transitions shown are allowed and others not.

考察三个能级的兰德-盖尔因子g_L的大小,将说明不同能级分裂幅度不同的原因。选择定则解释了为何所示的跃迁是允许的,而其他跃迁则不允许。
Some history
一些历史
Index
索引
 
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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。
Index

Reference
Leighton
Ch 2
索引参考莱顿第二章
 
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