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Symmetry and Selection Rules Preview

A selection rule is a symmetry reason for a matrix element to vanish. The basic object is

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

where ∣i⟩\lvert i\rangle is the initial state, ∣f⟩\lvert f\rangle is the final state, and TT is the operator that tries to connect them. If symmetry says Mfi=0M_{fi}=0, then the transition, coupling, expectation value, or mixing process is forbidden in the model being used.

This page gives the continuous-symmetry logic before the full tensor-operator treatment. The detailed angular-momentum machinery belongs to Selection Rules, Irreducible Spherical Tensors, and the Wigner–Eckart Theorem.

Selection rules compare the transformation labels of the states with the transformation label of the operator. Those labels must be meaningful for the Hamiltonian and the approximation under discussion.

If a conserved observable QQ commutes with the Hamiltonian,

[H,Q]=0,[H,Q]=0,

then stationary states can often be chosen in sectors of fixed QQ. If several commuting labels are available, the transition problem can be organized by simultaneous eigenstates:

∣E,q1,…,qr,λ⟩.\lvert E,q_1,\ldots,q_r,\lambda\rangle.

The extra label λ\lambda reminds us that symmetry labels need not uniquely identify a state. The selection rule constrains the symmetry sector, not every dynamical detail inside the sector. See Simultaneous Eigenstates and Good Quantum Numbers for the label criterion.

Let UU be a unitary symmetry. Suppose the states have definite transformation phases,

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

and suppose the operator transforms by

UTU†=uTT.UTU^\dagger = u_TT.

Insert U†U=IU^\dagger U=I around the operator:

⟨f∣T∣i⟩=⟨f∣U†UTU†U∣i⟩=uf∗uTui⟨f∣T∣i⟩.\begin{aligned} \langle f|T|i\rangle &= \langle f|U^\dagger UTU^\dagger U|i\rangle \\ &= u_f^*u_Tu_i \langle f|T|i\rangle. \end{aligned}

Therefore a nonzero matrix element requires

uf∗uTui=1.u_f^*u_Tu_i=1.

If the product is not 11, the only consistent value is Mfi=0M_{fi}=0. This is the compact form of many parity, charge, and discrete-symmetry selection rules. It uses unitary UU; for an antiunitary symmetry, conjugated amplitudes require a different argument.

For a continuous one-parameter symmetry, write

U(α)=exp⁡ ⁣(−iαQℏ),U(\alpha) = \exp\!\left(-\frac{i\alpha Q}{\hbar}\right),

where QQ is the generator. Suppose

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

and suppose the operator has a definite charge under the adjoint action of QQ:

[Q,T]=qTT.[Q,T]=q_TT.

Taking a matrix element of this commutator gives

⟨f∣[Q,T]∣i⟩=(qf−qi)⟨f∣T∣i⟩=qT⟨f∣T∣i⟩.\begin{aligned} \langle f|[Q,T]|i\rangle &= (q_f-q_i)\langle f|T|i\rangle \\ &= q_T\langle f|T|i\rangle. \end{aligned}

Thus

(qf−qi−qT)Mfi=0.(q_f-q_i-q_T)M_{fi}=0.

A nonzero matrix element can occur only if

qf=qi+qT.q_f=q_i+q_T.

The operator must carry exactly the amount of quantum number needed to connect the two sectors. If TT is neutral, then qf=qiq_f=q_i.

Parity is discrete rather than continuous, but it is the cleanest first example. Let the states have definite parity

Π∣i⟩=πi∣i⟩,Π∣f⟩=πf∣f⟩,πi,πf=±1.\Pi\lvert i\rangle = \pi_i\lvert i\rangle, \qquad \Pi\lvert f\rangle = \pi_f\lvert f\rangle, \qquad \pi_i,\pi_f=\pm1.

If

ΠTΠ−1=ηTT,ηT=±1,\Pi T\Pi^{-1} = \eta_TT, \qquad \eta_T=\pm1,

then the finite test gives

πfηTπi=1.\pi_f\eta_T\pi_i=1.

An even operator, ηT=+1\eta_T=+1, connects only states of the same parity. An odd operator, ηT=−1\eta_T=-1, connects only states of opposite parity. The electric dipole operator is odd, which is why electric-dipole transitions between states of the same parity vanish in a parity-symmetric model.

For a conserved additive label, the infinitesimal test says that an operator must supply the missing charge. If

[Q,T]=qTT,[Q,T]=q_TT,

then

Δq≡qf−qi=qT\Delta q \equiv q_f-q_i = q_T

is required for a nonzero matrix element.

Common examples include particle-number-changing operators, spin ladder operators, oscillator ladder operators, and angular-momentum tensor components. For a neutral operator,

[Q,T]=0,[Q,T]=0,

the matrix element cannot connect states with different QQ eigenvalues. This is the operator form of charge conservation.

Take Q=JzQ=J_z. For a spherical tensor component Tq(k)T_q^{(k)},

[Jz,Tq(k)]=ℏq Tq(k).[J_z,T_q^{(k)}] = \hbar q\,T_q^{(k)}.

If

Jz∣ji,mi⟩=ℏmi∣ji,mi⟩,Jz∣jf,mf⟩=ℏmf∣jf,mf⟩,J_z\lvert j_i,m_i\rangle = \hbar m_i\lvert j_i,m_i\rangle, \qquad J_z\lvert j_f,m_f\rangle = \hbar m_f\lvert j_f,m_f\rangle,

then the charge-like rule gives

mf=mi+q.m_f=m_i+q.

This is the simplest angular-momentum selection rule. It follows from rotations about the chosen quantization axis alone. Full rotational covariance gives additional constraints, including the triangle condition

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

but that stronger statement uses the irreducible tensor structure developed later in the tensor-operator chapter.

The electric dipole operator is a vector under rotations and odd under parity. In spherical components it has rank k=1k=1 and component labels

q=−1,0,1.q=-1,0,1.

The magnetic rule gives

Δm=q,\Delta m=q,

where the chosen polarization selects which component appears. Rotation also imposes a rank-11 triangle rule. For orbital angular momentum this permits

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

subject to the triangle inequality, which also forbids ℓi=ℓf=0\ell_i=\ell_f=0. Since the dipole operator is odd and central-potential orbital states have parity (−1)ℓ(-1)^\ell, parity removes the Δℓ=0\Delta\ell=0 option. The familiar orbital electric-dipole rule is therefore

Δℓ=±1.\Delta\ell=\pm1.

The complete derivation, including polarization conventions and total-angular-momentum labels, is developed in Dipole Transitions.

An exact symmetry gives an exact zero for the corresponding matrix element. If the symmetry is approximate, the same matrix element is usually suppressed rather than exactly zero. If the perturbation, boundary condition, external field, environment, or measurement setup breaks the symmetry, the rule must be rederived for the new Hamiltonian and operator.

This is why “forbidden” rarely means impossible in the laboratory. It means forbidden by a specified operator under specified symmetry assumptions. An electric-dipole-forbidden transition may occur through a magnetic dipole, electric quadrupole, or two-photon process. Mixing can relax a rule only if it mixes the labels that protected the zero: ordinary spin–orbit coupling can relax a spin selection rule but preserves spatial parity, so it cannot by itself permit an electric-dipole transition between states of equal exact parity.

Selection rules are necessary tests for nonzero matrix elements. Passing a selection rule does not guarantee that the matrix element is nonzero or large.

Even if the symmetry labels match, the amplitude can still vanish because of:

  • orthogonality in additional quantum numbers;
  • a radial integral that happens to be zero;
  • destructive interference among components;
  • a missing physical coupling in the model;

A nonzero matrix element still does not guarantee an observable transition rate: energy conservation and available final states impose additional conditions.

Symmetry says which matrix elements are impossible under the assumptions. Dynamics decides the actual value of those not ruled out.

The phase test is simplest when the states are already eigenstates of the symmetry. In a degenerate subspace, an arbitrary basis vector may not have definite symmetry labels even when the subspace as a whole is symmetry invariant.

The practical instruction is: diagonalize the commuting symmetry labels before applying the rule. If the symmetry sectors are distinct, operators with definite transformation law have block-selection properties. If several copies of the same representation occur, symmetry alone may not distinguish the copies, and additional labels or dynamics are needed.

This is why selection-rule statements should name the basis and coupling scheme. After spin–orbit coupling becomes important, for example, j,mjj,m_j may be the good angular labels, while mℓ,msm_\ell,m_s are no longer exact labels of the Hamiltonian.

  1. A conserved charge QQ has eigenvalues qi=2q_i=2 and qf=5q_f=5 on the initial and final states. If [Q,T]=3T[Q,T]=3T, is ⟨f∣T∣i⟩\langle f|T|i\rangle forbidden by this charge?
Solution

The charge rule requires

qf=qi+qT.q_f=q_i+q_T.

Here qT=3q_T=3, so

qi+qT=2+3=5.q_i+q_T=2+3=5.

This matches qfq_f. The matrix element is not forbidden by this charge. It may still vanish for another symmetry or for dynamical reasons.

  1. Suppose πi=+1\pi_i=+1, πf=−1\pi_f=-1, and TT is parity even. What does parity say about MfiM_{fi}?
Solution

For a parity-even operator, ηT=+1\eta_T=+1. The nonzero condition is

πfηTπi=1.\pi_f\eta_T\pi_i=1.

Substituting the values gives

(−1)(+1)(+1)=−1.(-1)(+1)(+1)=-1.

The condition fails, so parity forces

Mfi=0.M_{fi}=0.
  1. A rank-11 spherical tensor component has q=0q=0. What magnetic quantum-number change can it produce?
Solution

The magnetic rule is

mf=mi+q.m_f=m_i+q.

For q=0q=0,

Δm=mf−mi=0.\Delta m=m_f-m_i=0.

This is often associated with the component parallel to the chosen quantization axis.

  1. Why does an exact electric-dipole selection rule not mean that the transition can never be observed?
Solution

An electric-dipole rule applies to the electric-dipole operator under a specified symmetry model. A transition forbidden at electric-dipole order may be allowed by a different operator, such as a magnetic dipole or electric quadrupole operator. It may also become weakly allowed when a perturbation mixes the particular protecting labels. For example, an electric field can mix opposite parity states; parity-preserving spin–orbit coupling cannot do that, though it can mix total-spin labels in many-electron states. The rule still matters because it explains why the leading amplitude vanishes and why the remaining process is usually weaker.

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  • A. R. Edmonds, Angular Momentum in Quantum Mechanics, Princeton University Press, 1957.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, chapters 3–5.
  • M. Tinkham, Group Theory and Quantum Mechanics, Dover, 2003 reprint of the 1964 edition.
  • E. P. Wigner, Group Theory and Its Application to the Quantum Mechanics of Atomic Spectra, Academic Press, 1959.