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Selection Rules in Transition Rates

A selection rule is a symmetry statement that makes a transition matrix element vanish. In transition calculations, the rate is often proportional to a squared matrix element, so a symmetry zero suppresses the transition before any density-of-states or resonance factor matters.

For a weak perturbation V(t)V(t), the first-order transition amplitude contains

⟨f∣VI(t)∣i⟩.\langle f|V_I(t)|i\rangle.

In the golden-rule regime, a typical rate has the form

Γi→f=2πℏ∣Vfi∣2ρ(Ef).\Gamma_{i\to f} = \frac{2\pi}{\hbar} |V_{fi}|^2 \rho(E_f).

If Vfi=0V_{fi}=0 by symmetry, the leading transition rate vanishes. A nonzero matrix element permitted by symmetry may still be small or vanish through radial cancellation; selection rules give necessary conditions, not guaranteed strengths.

Required background. Parity gives symmetry labels, and Fermi’s Golden Rule explains how a channel amplitude enters a rate.

Selection rules are not guesses about smallness. They are exact zeros under stated assumptions:

  • the Hamiltonian has the relevant symmetry;
  • the states are chosen with definite symmetry labels;
  • the perturbing operator transforms in a definite way;
  • the symmetry is not broken by the environment, boundary conditions, or approximations.

If any assumption fails, the selection rule may be weakened or removed.

Let Π\Pi be the parity operator. Suppose

Π∣i⟩=πi∣i⟩,Π∣f⟩=πf∣f⟩,\Pi\lvert i\rangle = \pi_i\lvert i\rangle, \qquad \Pi\lvert f\rangle = \pi_f\lvert f\rangle,

where πi,πf=±1\pi_i,\pi_f=\pm1. Let OO be an operator with parity πO\pi_O:

ΠOΠ−1=πOO.\Pi O\Pi^{-1} = \pi_O O.

Then

⟨f∣O∣i⟩=πfπOπi⟨f∣O∣i⟩.\langle f|O|i\rangle = \pi_f\pi_O\pi_i \langle f|O|i\rangle.

Therefore the matrix element can be nonzero only if

πfπOπi=1.\pi_f\pi_O\pi_i=1.

For an odd operator, πO=−1\pi_O=-1, transitions connect states of opposite parity. For an even operator, transitions connect states of the same parity.

In the electric dipole approximation, the perturbation is proportional to

d⋅ϵ,\mathbf d\cdot\boldsymbol\epsilon,

where d\mathbf d is odd under parity. Thus electric dipole transitions require opposite parity between initial and final states:

πf=−πi.\pi_f=-\pi_i.

For central-potential orbital states, the position operator transforms as a vector. The familiar orbital angular-momentum rule is

Δℓ=±1.\Delta \ell=\pm1.

For a spherical operator component dqd_q, the magnetic quantum number changes by qq:

Δm=0,±1.\Delta m=0,\pm1.

In the interaction −d⋅E=−∑q(−1)qdqE−q-\mathbf d\cdot\mathbf E=-\sum_q(-1)^q d_qE_{-q}, the component of the applied field is paired with dqd_q through E−qE_{-q}. State the spherical-basis and propagation conventions before identifying qq with a polarization helicity.

These are electric-dipole rules in the simplest nonrelativistic setting. Spin, fine structure, identical particles, and many-body structure add further labels.

Angular momentum selection rules come from rotational symmetry. A perturbing operator that transforms as a spherical tensor of rank kk can connect angular-momentum states only when angular momenta can couple consistently:

∣ji−k∣≤jf≤ji+k.|j_i-k| \le j_f \le j_i+k.

The magnetic quantum numbers satisfy

mf=mi+q,q=−k,…,k.m_f=m_i+q, \qquad q=-k,\ldots,k.

For a vector operator, k=1k=1, so q=0,±1q=0,\pm1 and j=0→j=0j=0\to j=0 is excluded by the triangle condition. Clebsch–Gordan coefficients determine which allowed couplings have nonzero angular factors. The systematic theorem behind this factorization is the Wigner–Eckart Theorem.

A selection rule first constrains the amplitude. The transition rate then inherits that constraint:

Vfi=0⟹Γi→f=0V_{fi}=0 \quad \Longrightarrow \quad \Gamma_{i\to f}=0

at the order being computed. Higher-order processes may still occur. For example, a one-photon electric dipole transition may be forbidden while a two-photon process, magnetic dipole process, or symmetry-breaking perturbation gives a much smaller nonzero rate.

Selection rules therefore classify leading mechanisms. They do not imply that a transition is impossible under all physical perturbations.

For continuum processes, the symmetry-allowed matrix element must still be combined with the correctly normalized final-state measure; see Density of States in Transition Rates.

Let ∣i⟩|i\rangle and ∣f⟩|f\rangle have the same parity, so ⟨f∣dq∣i⟩=0\langle f|d_q|i\rangle=0. Suppose a weak static parity-breaking perturbation mixes an opposite-parity state ∣o⟩|o\rangle into the final state:

∣f~⟩=∣f⟩+ϵ∣o⟩+O(ϵ2),ϵ=⟨o∣δH∣f⟩Ef−Eo.|\widetilde f\rangle=|f\rangle+\epsilon|o\rangle+O(\epsilon^2), \qquad \epsilon=\frac{\langle o|\delta H|f\rangle}{E_f-E_o}.

Assuming the initial state is unchanged at this order,

⟨f~∣dq∣i⟩=ϵ∗⟨o∣dq∣i⟩+O(ϵ2).\langle\widetilde f|d_q|i\rangle =\epsilon^*\langle o|d_q|i\rangle+O(\epsilon^2).

The borrowed transition strength scales as ∣ϵ∣2|\epsilon|^2 times the allowed strength, at fixed frequency and final-state measure. Near an ff–oo degeneracy, the mixing coefficient need not be small; diagonalize the pair before estimating the rate. If the initial state also mixes, its amplitude correction must be added coherently.

Allowed angular labels, zero angular factor

Section titled “Allowed angular labels, zero angular factor”

Can a rank-one q=0q=0 operator connect ji=jf=1j_i=j_f=1, mi=mf=0m_i=m_f=0? Compare the triangle and magnetic conditions with the actual angular coefficient.

Solution

The triangle and magnetic conditions allow these labels, but the coefficient is proportional to the Wigner symbol (111000)=0\left(\begin{smallmatrix}1&1&1\\0&0&0\end{smallmatrix}\right)=0. Interchanging the first and third columns leaves all entries unchanged while multiplying the symbol by (−1)1+1+1=−1(-1)^{1+1+1}=-1, so it must vanish. Necessary angular-label rules do not replace evaluation of the angular factor.

Suppose the final-state mixing above contributes amplitude ϵ∗Df\epsilon^*D_f and initial-state mixing contributes ηDi\eta D_i. Write the strength through quadratic order in the mixing coefficients. Can two nonzero contributions cancel?

Solution

The strength is ∣ϵ∗Df+ηDi∣2|\epsilon^*D_f+\eta D_i|^2, including the interference term 2Re⁡(ϵηDf∗Di)2\operatorname{Re}(\epsilon\eta D_f^*D_i). Equal and opposite amplitudes give zero even though each mixing pathway is individually nonzero. Adding their squared magnitudes would discard coherence.

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