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A selection rule is a symmetry statement that makes a matrix element vanish. In transition problems the relevant matrix element often has the form

Mfi=⟨f∣O∣i⟩,M_{fi} = \langle f|O|i\rangle,

where OO is the perturbing operator, coupling operator, or observable being tested. If symmetry forces Mfi=0M_{fi}=0, the corresponding transition, coupling, or mixing is forbidden at that order and under those assumptions.

An exact zero is stronger than a small rate. To decide which is meant, identify the states, operator, and approximation used in the calculation.

The argument needs definite transformation laws for the states and operator. A symmetry of the Hamiltonian often supplies suitable energy eigenstates, but the matrix-element identity also holds for deliberately prepared symmetry eigenstates. Mixing those states or changing the interaction can change the rule.

Let UU be a unitary symmetry. Suppose

U∣i⟩=ui∣i⟩,U∣f⟩=uf∣f⟩,U|i\rangle = u_i|i\rangle, \qquad U|f\rangle = u_f|f\rangle,

and suppose the operator transforms as

UOU†=uOO.UOU^\dagger = u_O O.

Then

⟨f∣O∣i⟩=⟨f∣U†UOU†U∣i⟩=uf∗uOui ⟨f∣O∣i⟩.\begin{aligned} \langle f|O|i\rangle &= \langle f|U^\dagger UOU^\dagger U|i\rangle \\ &= u_f^*u_Ou_i\, \langle f|O|i\rangle. \end{aligned}

Therefore a nonzero matrix element requires

uf∗uOui=1.u_f^*u_Ou_i=1.

If this condition fails, the matrix element must vanish. Parity rules, charge-conservation rules, and many discrete symmetry rules are versions of this simple argument.

The focused derivation and common parity examples are collected in Parity Selection Rules. The compact version is as follows.

For parity, the eigenvalues are

πi,πf=±1.\pi_i,\pi_f=\pm1.

If the operator has parity πO\pi_O, then

ΠOΠ−1=πOO.\Pi O\Pi^{-1} = \pi_O O.

The nonzero condition becomes

πfπOπi=1.\pi_f\pi_O\pi_i=1.

Thus:

  • an even operator connects states of the same parity;
  • an odd operator connects states of opposite parity.

For example, the electric dipole operator is odd under parity. In a parity-symmetric atom or molecule, an electric-dipole matrix element between two states of the same parity vanishes.

For a continuous U(1)U(1) symmetry with conserved generator QQ, states may be labeled by charge:

Q∣i⟩=qi∣i⟩,Q∣f⟩=qf∣f⟩.Q|i\rangle = q_i|i\rangle, \qquad Q|f\rangle = q_f|f\rangle.

An operator carries charge qOq_O when [Q,O]=qOO[Q,O]=q_OO. Taking this commutator between charge eigenstates gives

(qf−qi)⟨f∣O∣i⟩=qO⟨f∣O∣i⟩.(q_f-q_i)\langle f|O|i\rangle=q_O\langle f|O|i\rangle.

A nonzero matrix element therefore requires

qf=qi+qO.q_f=q_i+q_O.

If OO is neutral, then qf=qiq_f=q_i. This is the selection-rule form of charge conservation. In nonrelativistic quantum mechanics the same logic appears for particle number, magnetic quantum numbers, oscillator number under special ladder operators, and other additive labels when the operator has a definite charge under the symmetry.

Angular momentum selection rules use the fact that operators can transform as irreducible spherical tensors. A rank-kk tensor component Tq(k)T_q^{(k)} carries magnetic label qq.

The Wigner–Eckart theorem gives the rotational selection rules

mf=mi+q,m_f=m_i+q,

and

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

The first rule is a magnetic quantum-number rule. The second is a triangle rule, with jfj_f advancing in integer steps from ∣ji−k∣|j_i-k|. It expresses whether jij_i and the operator rank kk can couple to jfj_f. A rank-11 operator excludes 0→00\to0, even though the shorthand Δj=0,±1\Delta j=0,\pm1 might seem to include it.

For a vector operator, k=1k=1, so

Δm=q=0,±1,\Delta m=q=0,\pm1,

and

jf=ji−1, ji, ji+1j_f=j_i-1,\ j_i,\ j_i+1

where the values are allowed by nonnegative angular momentum and the triangle condition.

Many familiar rules combine more than one symmetry. Electric dipole transitions in central-potential orbital states are the standard example.

The position operator is a vector, so angular momentum allows

ℓf=ℓi−1,ℓi,ℓi+1.\ell_f=\ell_i-1,\ell_i,\ell_i+1.

But position is odd under parity, and orbital parity is

πℓ=(−1)ℓ.\pi_\ell=(-1)^\ell.

The parity rule requires opposite parity:

(−1)ℓf=−(−1)ℓi.(-1)^{\ell_f} = -(-1)^{\ell_i}.

Combining both statements gives

Δℓ=±1.\Delta\ell=\pm1.

The Δℓ=0\Delta\ell=0 option is allowed by rotations for a vector operator but forbidden by parity in this setting.

Spin selection rules depend on the operator. If an operator acts only on spatial variables and commutes with total spin, then spin labels are preserved:

Δs=0,Δms=0\Delta s=0, \qquad \Delta m_s=0

in the basis where those labels are meaningful.

In atomic spectroscopy, electric dipole transitions often satisfy an approximate ΔS=0\Delta S=0 rule in an LSLS-coupling description because the leading electric dipole operator does not act on spin. But this is not a universal law. Spin-dependent interactions can mix different SS sectors or introduce an operator with a different spin transformation law. Spin-independent electrostatic configuration mixing preserves SS and cannot alone open a ΔS≠0\Delta S\ne0 line. Likewise, the leading atomic M1 operator proportional to L+gsS\mathbf L+g_s\mathbf S preserves SS in pure LSLS coupling.

Check whether the particular interaction commutes with S2S^2 before attributing a weak line to spin mixing.

“Forbidden” usually means forbidden in a specified approximation. A transition can become weakly allowed when:

  • a different multipole operator contributes;
  • a higher-order perturbative process is included;
  • spin–orbit or hyperfine mixing changes the state labels;
  • an external field breaks the symmetry;
  • the environment or boundary conditions no longer respect the symmetry;
  • the initial or final state is only approximately a symmetry eigenstate.

For example, an electric-dipole forbidden transition may occur through magnetic dipole or electric quadrupole multipoles, two-photon processes, or symmetry-breaking mechanisms. The selection rule still matters: it tells which leading mechanism vanishes and why the observed process is weaker.

Selection rules constrain amplitudes. Rates require additional physics. In a golden-rule calculation,

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

Here MfiM_{fi} is the relevant interaction matrix element and ρ\rho is the density per unit energy at the energy allowed by the process, including photon energy for absorption or emission. For isolated discrete levels, finite-time amplitudes or a line profile replace a naive continuum density. If symmetry gives Mfi=0M_{fi}=0, the leading rate vanishes. If MfiM_{fi} is allowed, the actual rate still depends on the reduced matrix element, density of final states, linewidths, populations, polarization, and experimental geometry.

The transition-rate machinery belongs to Selection Rules in Transition Rates. The electric-dipole specialization is derived in Dipole Transitions, while Atomic Selection Rules applies the hierarchy to fine and hyperfine labels, polarization, metastability, and perturbative mixing. This page explains the general symmetry zeros.

  • Calling a transition forbidden without naming the symmetry and operator.
  • Treating “allowed” as meaning “large.”
  • Applying parity rules when the system is not parity symmetric.
  • Forgetting that angular momentum rules and parity rules are separate constraints.
  • Using weak-field quantum numbers in a strong-field regime where the coupling scheme has changed.
  • Treating spin selection rules as exact when spin-dependent interactions mix the states.
  • Forgetting that a higher-order or different-multipole process can bypass a leading selection rule.
  1. Two states have parity πi=+1\pi_i=+1 and πf=+1\pi_f=+1. Can an odd operator connect them?
Solution

For an odd operator, πO=−1\pi_O=-1. The nonzero condition is

πfπOπi=1.\pi_f\pi_O\pi_i=1.

Here

(+1)(−1)(+1)=−1,(+1)(-1)(+1)=-1,

so the matrix element must vanish.

  1. Let QQ count excitations and let [Q,O]=2O[Q,O]=2O. Can OO connect a state with qi=3q_i=3 to one with qf=4q_f=4? What about qf=5q_f=5?
Solution

The commutator requires (qf−qi−2)⟨f∣O∣i⟩=0(q_f-q_i-2)\langle f|O|i\rangle=0. Thus 3→43\to4 vanishes, while 3→53\to5 is not excluded by this rule. The latter can still vanish for another symmetry or because of the detailed matrix element.

  1. Why does the electric dipole orbital rule exclude Δℓ=0\Delta\ell=0 even though a vector operator can satisfy the triangle rule with ℓf=ℓi\ell_f=\ell_i?
Solution

The vector nature of the dipole operator gives the triangle rule

ℓf=ℓi−1,ℓi,ℓi+1\ell_f=\ell_i-1,\ell_i,\ell_i+1

where allowed. But the electric dipole operator is odd under parity. Orbital states have parity (−1)ℓ(-1)^\ell, so a dipole matrix element requires opposite parity between the initial and final orbital states. The case ℓf=ℓi\ell_f=\ell_i has the same parity and is therefore forbidden. The remaining options are

Δℓ=±1.\Delta\ell=\pm1.
  1. Give one mechanism that can make a forbidden transition weakly allowed.
Solution

For an opposite-parity pair with an E1 spin-forbidden amplitude, spin–orbit mixing can admix the required spin character. If the admixture is ϵ\epsilon and the borrowed allowed amplitude is M0M_0, then M≃ϵM0M\simeq\epsilon M_0 and the rate is of order ∣ϵ∣2∣M0∣2|\epsilon|^2|M_0|^2, apart from phase-space factors. Spin–orbit coupling preserves parity, so it cannot by itself open an E1 line between two same-parity states.

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