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Free Physics Study Material for CSIR NET, IIT JAM, GATE, JEST & TIFR

by Pravegaa Education
Chapter 3

Spectroscopic Notation, L–S Coupling, j–j Coupling and Hyperfine Structure

What this chapter covers
  • Orbital and spin magnetic moments, the Bohr magneton, and the \(g\) factors.

  • Larmor precession and space quantization.

  • The vocabulary of spectroscopy: state, level, sublevel, term, configuration, statistical weight.

  • The atomic Hamiltonian, and which of its terms decides whether an atom follows L–S or j–j coupling.

  • Building term symbols \(^{2S+1}L_J\) for non-equivalent and equivalent electrons, the latter via Breit's scheme.

  • Hund's rules, the Landé interval rule, and the selection rules.

  • j–j coupling, and how its level count agrees with L–S.

3.1 Orbital Magnetic Dipole Moment: the Bohr Magneton

An electron in orbit is a current loop. If the orbital period is \(T\), the orbital current is \begin{equation} i = -\frac{e}{T} = -\frac{e v}{2\pi r} , \label{eq:orbital-current} \end{equation} and if \(A = \pi r^{2}\) is the area enclosed, the orbital magnetic moment is \begin{equation} \mu_{\ell} = i A = -\frac{e v r}{2} . \label{eq:mu-orbital} \end{equation} The orbital angular momentum is \(L = m v r\), so \begin{equation} \boxed{\;\frac{\mu_{\ell}}{L} = -\frac{e}{2m}\;} \label{eq:gyromag-ratio} \end{equation}

The ratio of magnetic moment to angular momentum is independent of the parameters of the orbit — \(v\) and \(r\) have cancelled. The quantity \(e/2m\) is the gyromagnetic ratio of the electron, exactly half the charge-to-mass ratio \(e/m = 1.76\times 10^{11}\,\mathrm{C}\,\mathrm{kg}^{-1}\).

Note

The electron is negatively charged, so its magnetic dipole moment points opposite to its angular momentum. Every sign in this chapter follows from that one fact.

Written as a vector relation, \begin{equation} \vec\mu_{\ell} = -\,g_{\ell}\,\frac{\mu_{\mathrm B}}{\hbar}\,\vec L , \qquad g_{\ell} = 1 , \label{eq:mu-vec-orbital} \end{equation} where the Bohr magneton is \begin{equation} \mu_{\mathrm B} = \frac{e\hbar}{2m} = 9.274\times 10^{-24}\,\mathrm{J}\,\mathrm{T}^{-1} = 5.788\times 10^{-5}\,\mathrm{eV}\,\mathrm{T}^{-1} . \label{eq:bohr-magneton} \end{equation} The orbital \(g\) factor \(g_{\ell}=1\) is introduced only to preserve symmetry with the spin and Landé \(g\) factors that follow; it is not equal to \(g_{s}\).

From quantum mechanics \(\lvert\vec L\rvert = \sqrt{\ell(\ell+1)}\,\hbar\), so the magnitude of the orbital moment is \begin{equation} \lvert\vec\mu_{\ell}\rvert = g_{\ell}\,\mu_{\mathrm B}\sqrt{\ell(\ell+1)} , \qquad \mu_{\ell,z} = -g_{\ell}\,\mu_{\mathrm B}\, m_{\ell} . \label{eq:mu-magnitude} \end{equation}

3.2 Larmor Precession

A magnetic dipole in an external field \(\vec B\) experiences a torque \begin{equation} \vec\tau = \vec\mu \times \vec B , \label{eq:torque} \end{equation} and since \(\vec\tau = \dd\vec L/\dd t\), combining with \(\eqref{eq:mu-vec-orbital}\) gives \[ \frac{\dd \vec L}{\dd t} = -\frac{e}{2m}\,\vec L \times \vec B . \] This is the equation of a vector precessing about \(\vec B\) at constant angle, with angular frequency \begin{equation} \boxed{\;\omega_{L} = \frac{eB}{2m} = \frac{g_{\ell}\mu_{\mathrm B}B}{\hbar}\;} \qquad \nu_{L} = \frac{eB}{4\pi m} . \label{eq:larmor} \end{equation} This is the Larmor precession frequency. Note that the magnitude of \(\vec L\) and its angle to \(\vec B\) are unchanged — only the azimuth advances.

Exam Tip

For spin, \(g_{s}=2\) doubles this: \(\omega_{s} = eB/m\). The factor-of-two difference between orbital and spin precession is the origin of the anomalous Zeeman effect in Chapter 4.

3.3 Space Quantization

Since \(L_{z} = m_{\ell}\hbar\) while \(\lvert\vec L\rvert = \sqrt{\ell(\ell+1)}\,\hbar\), the angular momentum vector can only make certain discrete angles with the field direction: \begin{equation} \cos\theta = \frac{L_{z}}{\lvert\vec L\rvert} = \frac{m_{\ell}}{\sqrt{\ell(\ell+1)}} , \qquad m_{\ell} = -\ell,\dots,+\ell . \label{eq:space-quant} \end{equation}

Figure 3.1. Space quantization of the orbital angular momentum: (a) \(\ell = 2\), (b) \(\ell = 3\). The vector \(\vec L\) has the fixed length \(\sqrt{\ell(\ell+1)}\,\hbar\) — the radius of the semicircle — but its projection on the field axis is restricted to the \(2\ell+1\) values \(L_{z} = m_{\ell}\hbar\) marked by the dashed lines. Note that the arrow can never lie along the axis: since \(\sqrt{\ell(\ell+1)} > \ell\), even the extreme state \(m_{\ell} = \ell\) leaves \(\vec L\) tilted away from \(z\). This is a purely quantum feature, and it is the reason \(\vec L\) must be pictured as precessing about the axis rather than standing still.
Exam Tip

The minimum angle for given \(\ell\) is at \(m_{\ell} = \ell\): \[ \cos\theta_{\min} = \frac{\ell}{\sqrt{\ell(\ell+1)}} = \sqrt{\frac{\ell}{\ell+1}} . \] For a \(2p\) electron (\(\ell=1\)) this gives \(\cos\theta = 1/\sqrt2\), so \(\theta_{\min} = 45^{\circ}\) — asked verbatim in GATE 2023.

3.4 Electron Spin and its Magnetic Moment

The electron behaves as though it were a charged sphere spinning about its own axis, carrying an intrinsic angular momentum and hence an intrinsic magnetic dipole moment. In terms of the Pauli matrices, \begin{equation} \vec S = \frac{\hbar}{2}\,\vec\sigma , \qquad \lvert\vec S\rvert = \sqrt{s(s+1)}\,\hbar = \frac{\sqrt3}{2}\hbar , \qquad S_{z} = m_{s}\hbar = \pm\frac{\hbar}{2} , \label{eq:spin-operators} \end{equation} with \(s = \tfrac12\) and \(m_{s} = \pm\tfrac12\); the kets \(\lvert s, m_{s}\rangle\) form a complete two-dimensional basis.

Space quantization for spin follows \(\eqref{eq:space-quant}\) with \(\ell \to s\): \begin{equation} \cos\theta = \frac{m_{s}}{\sqrt{s(s+1)}} = \pm\frac{1}{\sqrt3} \quad\Longrightarrow\quad \theta = 54.7^{\circ} \ \text{or}\ 125.3^{\circ} . \label{eq:spin-angles} \end{equation}

The associated magnetic moment is \begin{equation} \vec\mu_{s} = -\,g_{s}\,\frac{\mu_{\mathrm B}}{\hbar}\,\vec S , \qquad g_{s} = 2.0023 \approx 2 , \label{eq:mu-spin3} \end{equation} so that \begin{equation} \lvert\vec\mu_{s}\rvert = g_{s}\mu_{\mathrm B}\sqrt{s(s+1)} = \sqrt3\,\mu_{\mathrm B} , \qquad \mu_{s,z} = -g_{s}\mu_{\mathrm B}m_{s} = \mp\mu_{\mathrm B} . \label{eq:mu-spin-z} \end{equation}

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