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Wigner’s Theorem Preview

Wigner’s theorem explains why quantum symmetries are represented on Hilbert space by unitary or antiunitary operators. The input is not a preferred basis, a Hamiltonian, or a demand that inner products themselves be fixed. The input is physical: a symmetry of pure states should preserve transition probabilities between rays.

The theorem is one of the structural reasons quantum mechanics has the symmetry language it does. Ordinary rotations, translations, parity, and internal phase symmetries are represented unitarily. Time reversal is represented antiunitarily. Projective phases appear because the physical states are rays rather than phase-chosen vectors.

For the proof and precise uniqueness statement, see Wigner’s Theorem. The short theorem statement is useful when you need only the assumptions and conclusion.

Pure states are rays in a complex Hilbert space H\mathcal H. A ray is written [ψ][\psi], meaning all nonzero scalar multiples of ∣ψ⟩\lvert\psi\rangle represent the same physical pure state.

For normalized representatives, the transition probability between two pure states is

P(ϕ,ψ)=∣⟨ϕ∣ψ⟩∣2.P(\phi,\psi) = \lvert\langle\phi|\psi\rangle\rvert^2.

Wigner’s theorem says, roughly:

If a bijective transformation of pure-state rays preserves all transition probabilities, then it can be implemented on Hilbert-space vectors by either a unitary or an antiunitary operator, up to physically irrelevant phase choices.

In symbols, if a ray map SS satisfies

P(Sϕ,Sψ)=P(ϕ,ψ)P(S\phi,S\psi) = P(\phi,\psi)

for all pure states, then one can choose a Hilbert-space operator S^\widehat S such that

S[ψ]=[S^ψ],S[\psi] = [\widehat S\psi],

where S^\widehat S is either unitary or antiunitary. Different choices of vector representatives can change S^ψ\widehat S\psi by phases without changing the ray transformation.

The transition probability is directly physical. It is the probability that a system prepared in ∣ψ⟩\lvert\psi\rangle is found in the one-dimensional projector onto ∣ϕ⟩\lvert\phi\rangle:

Prob⁡(ψ→ϕ)=∣⟨ϕ∣ψ⟩∣2.\operatorname{Prob}(\psi\to\phi) = \lvert\langle\phi|\psi\rangle\rvert^2.

This number is insensitive to independent phase choices:

∣⟨eiβϕ∣eiαψ⟩∣2=∣ei(α−β)⟨ϕ∣ψ⟩∣2=∣⟨ϕ∣ψ⟩∣2.\lvert \langle e^{i\beta}\phi|e^{i\alpha}\psi\rangle \rvert^2 = \lvert e^{i(\alpha-\beta)} \langle\phi|\psi\rangle \rvert^2 = \lvert\langle\phi|\psi\rangle\rvert^2.

The inner product ⟨ϕ∣ψ⟩\langle\phi|\psi\rangle itself is not a ray-level observable, because it changes under phase conventions. Its absolute square is the natural ray-level invariant.

This point is why the theorem starts from rays and transition probabilities. Starting instead from vectors and inner products would put in extra convention-dependent structure by hand.

A unitary operator UU is a surjective linear map that preserves inner products:

⟨Uϕ∣Uψ⟩=⟨ϕ∣ψ⟩.\langle U\phi|U\psi\rangle = \langle\phi|\psi\rangle.

Therefore it preserves transition probabilities:

∣⟨Uϕ∣Uψ⟩∣2=∣⟨ϕ∣ψ⟩∣2.\lvert\langle U\phi|U\psi\rangle\rvert^2 = \lvert\langle\phi|\psi\rangle\rvert^2.

An antiunitary operator AA is a surjective antilinear map that conjugates inner products:

A(a∣ψ⟩+b∣ϕ⟩)=a∗A∣ψ⟩+b∗A∣ϕ⟩,A(a\lvert\psi\rangle+b\lvert\phi\rangle) = a^*A\lvert\psi\rangle+b^*A\lvert\phi\rangle,

and

⟨Aϕ∣Aψ⟩=⟨ϕ∣ψ⟩∗.\langle A\phi|A\psi\rangle = \langle\phi|\psi\rangle^*.

It also preserves transition probabilities:

∣⟨Aϕ∣Aψ⟩∣2=∣⟨ϕ∣ψ⟩∗∣2=∣⟨ϕ∣ψ⟩∣2.\lvert\langle A\phi|A\psi\rangle\rvert^2 = \lvert\langle\phi|\psi\rangle^*\rvert^2 = \lvert\langle\phi|\psi\rangle\rvert^2.

Thus the two possibilities differ in what they do to phases, not in what they do to transition probabilities.

For a time-independent Hamiltonian, time reversal illustrates why the antiunitary option matters. The Schrödinger equation contains ii:

iℏddt∣ψ(t)⟩=H∣ψ(t)⟩.i\hbar \frac{d}{dt} \lvert\psi(t)\rangle = H\lvert\psi(t)\rangle.

If time reversal maps a solution to another solution by

∣ψT(t)⟩=Θ∣ψ(−t)⟩,\lvert\psi_T(t)\rangle = \Theta\lvert\psi(-t)\rangle,

then the transformed state should satisfy a Schrödinger equation with Hamiltonian ΘHΘ−1\Theta H\Theta^{-1}. This works naturally when Θ\Theta is antiunitary, because it conjugates ii:

ΘiΘ−1=−i.\Theta i\Theta^{-1} = -i.

Using the original equation at time −t-t, one finds

iℏddt∣ψT(t)⟩=ΘHΘ−1∣ψT(t)⟩.i\hbar \frac{d}{dt} \lvert\psi_T(t)\rangle = \Theta H\Theta^{-1} \lvert\psi_T(t)\rangle.

If Θ\Theta were complex-linear instead, reversing tt would produce −ΘHΘ−1-\Theta H\Theta^{-1} as the transformed Hamiltonian. The ordinary time-reversal operation preserves energy, so it uses the antiunitary alternative. A unitary operation that happens to exchange positive and negative eigenvalues of a special finite-dimensional Hamiltonian is a different spectral symmetry.

For a spinless particle with a real scalar potential and no magnetic vector potential, a suitable position-space convention is

(Θψ)(x)=ψ(x)∗.(\Theta\psi)(x) = \psi(x)^*.

For spin-1/21/2, time reversal also rotates the spinor:

Θ=−iσyK\Theta = -i\sigma_y K

in a common σz\sigma_z-basis convention. The details and the result Θ2=−I\Theta^2=-I are worked out in Time Reversal for Spin-1/2 Particles.

A continuous symmetry connected to the identity is implemented unitarily. A strongly continuous one-parameter subgroup can be lifted to a unitary group of the form

U(α)=exp⁡(−iαGℏ).U(\alpha) = \exp \left( -\frac{i\alpha G}{\hbar} \right).

The reason is structural. The identity operation is represented by the identity operator, which is linear. A continuous path of symmetry operations starting at the identity cannot jump into the antiunitary component without losing continuity in the usual operator topology. Antiunitary transformations therefore appear most naturally as discrete symmetries or as disconnected components of a larger symmetry group.

This is why translations, rotations connected to the identity, and time evolution are unitary, while time reversal is antiunitary.

Wigner’s theorem gives a lift from a ray transformation to a Hilbert-space operator, but the lift is not unique. Multiplying a representative by a phase leaves the ray unchanged:

S^∣ψ⟩andeiαS^∣ψ⟩\widehat S\lvert\psi\rangle \quad \text{and} \quad e^{i\alpha} \widehat S\lvert\psi\rangle

represent the same transformed ray. For a Hilbert space of dimension at least two, two unitary or antiunitary operators implementing the same ray map differ by one state-independent phase. Assigning arbitrary phases separately to output vectors generally destroys linearity or antilinearity; it is not a new operator implementation.

When unitary symmetry transformations form a group GG, this phase freedom leads naturally to projective representations. Instead of

U(g)U(h)=U(gh),U(g)U(h) = U(gh),

one may have

U(g)U(h)=eiω(g,h)U(gh).U(g)U(h) = e^{i\omega(g,h)} U(gh).

The phase factor does not change any single ray, but it can encode real representation-theoretic information. Spin-1/21/2 under rotations is the central elementary example. The quantum-mechanical motivation is developed in Projective Representations.

The bridge from projective phases to, but not identification with, field-theoretic anomalies is From Projective Representations to Anomalies Preview.

The theorem assumes a bijection of all pure-state rays preserving every transition probability. Norm preservation alone, or agreement on a few test states, is insufficient. It does not classify arbitrary noisy maps on density matrices.

The theorem also does not test a particular Hamiltonian. That requires the separate condition SHS−1=HSHS^{-1}=H. Once a group of symmetries is involved, compatible phase choices are a further question, developed in Projective Representations.

  1. Why is the transition probability ray-invariant?

Show that ∣⟨ϕ∣ψ⟩∣2\lvert\langle\phi|\psi\rangle\rvert^2 is unchanged under ∣ψ⟩↦eiα∣ψ⟩\lvert\psi\rangle\mapsto e^{i\alpha}\lvert\psi\rangle and ∣ϕ⟩↦eiβ∣ϕ⟩\lvert\phi\rangle\mapsto e^{i\beta}\lvert\phi\rangle.

Solution

Under the phase changes,

⟨eiβϕ∣eiαψ⟩=ei(α−β)⟨ϕ∣ψ⟩.\langle e^{i\beta}\phi|e^{i\alpha}\psi\rangle = e^{i(\alpha-\beta)} \langle\phi|\psi\rangle.

Taking the absolute square removes the phase:

∣ei(α−β)⟨ϕ∣ψ⟩∣2=∣⟨ϕ∣ψ⟩∣2.\left| e^{i(\alpha-\beta)} \langle\phi|\psi\rangle \right|^2 = \lvert\langle\phi|\psi\rangle\rvert^2.
  1. A map fixes ∣0⟩|0\rangle and ∣1⟩|1\rangle but sends ∣+⟩=(∣0⟩+∣1⟩)/2|+\rangle=(|0\rangle+|1\rangle)/\sqrt2 to i∣+⟩i|+\rangle. Can this map be linear? Does it still represent the identity on these three rays?
Solution

Linearity and the first two assignments force ∣+⟩|+\rangle to map to itself, so this chosen vector map is not linear. Each output nevertheless lies on the input ray. This separates arbitrary choices of ray representatives from the linear unitary implementation, which here is II (or a single overall phase times II).

  1. Why does time reversal conjugate ii?

Explain in one or two equations why an antiunitary Θ\Theta has ΘiΘ−1=−i\Theta i\Theta^{-1}=-i.

Solution

Antilinearity means scalar coefficients are conjugated:

Θ(c∣ψ⟩)=c∗Θ∣ψ⟩.\Theta(c\lvert\psi\rangle) = c^*\Theta\lvert\psi\rangle.

With c=ic=i,

Θ(i∣ψ⟩)=−iΘ∣ψ⟩.\Theta(i\lvert\psi\rangle) = -i\Theta\lvert\psi\rangle.

Equivalently, as an operator identity on vectors,

ΘiΘ−1=−i.\Theta i\Theta^{-1} = -i.
  1. Separate theorem implementation from Hamiltonian symmetry.

Suppose a ray transformation is implemented by a unitary operator UU. What extra condition makes it a symmetry of a time-independent Hamiltonian HH?

Solution

Wigner’s theorem supplies the unitary or antiunitary implementation of a transition-probability-preserving ray map. For UU to be a symmetry of the specific Hamiltonian HH, one also needs

UHU†=H,UHU^\dagger = H,

or equivalently [U,H]=0[U,H]=0 for a unitary UU. This is a dynamical condition, not part of the theorem by itself.

  • V. Bargmann, “Note on Wigner’s theorem on symmetry operations,” Journal of Mathematical Physics 5, 862–868 (1964). doi:10.1063/1.1704188.
  • B. C. Hall, Quantum Theory for Mathematicians, Springer, 2013. doi:10.1007/978-1-4614-7116-5.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020, chapter 4.
  • R. Simon, N. Mukunda, S. Chaturvedi, and V. Srinivasan, “Two elementary proofs of the Wigner theorem on symmetry in quantum mechanics,” arXiv:0808.0779 [quant-ph], 2008. Author manuscript.
  • E. P. Wigner, Group Theory and Its Application to the Quantum Mechanics of Atomic Spectra, Academic Press, 1959.