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Antiunitary Time Reversal

Time reversal in quantum mechanics is represented by an antiunitary operator, not by an ordinary unitary operator. This is not a matter of convention. It is forced by the sign of ii in the Schrödinger equation, by the canonical commutation relations, and by the requirement that time reversal relate forward evolution to backward evolution.

Write the time-reversal operator as Θ\Theta. Antiunitarity means two things:

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

and

⟨Θϕ∣Θψ⟩=⟨ϕ∣ψ⟩∗.\langle \Theta\phi|\Theta\psi\rangle = \langle \phi|\psi\rangle^*.

The first line is antilinearity; the second says transition probabilities are preserved. In particular,

ΘiΘ−1=−i.\Theta i\Theta^{-1}=-i.

That one sign is the algebraic heart of time reversal.

There are two closely related questions that are often blended together:

  • What operator represents time reversal on Hilbert space?
  • When is a Hamiltonian invariant under that operator?

The first question is answered by antiunitarity and the transformation of observables such as position, momentum, orbital angular momentum, and spin. The second question is dynamical:

ΘHΘ−1=H\Theta H\Theta^{-1}=H

for a time-independent Hamiltonian with no external parameters held fixed in a time-reversal-odd way. A Hamiltonian can fail the second test even though the time-reversal operator itself is perfectly well defined.

The conceptual overview is Time Reversal. This page gives the working derivation of antiunitarity.

Start with a state satisfying

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

The time-reversed candidate is the state

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

Let τ=−t\tau=-t. Since

ddτ∣ψ(τ)⟩=−iℏH∣ψ(τ)⟩,\frac{d}{d\tau}\lvert\psi(\tau)\rangle = -\frac{i}{\hbar}H\lvert\psi(\tau)\rangle,

we get

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

Now apply Θ\Theta. Because Θ\Theta is antilinear, the scalar ii becomes −i-i:

ddt∣ψT(t)⟩=Θ(iℏH∣ψ(−t)⟩)=−iℏΘH∣ψ(−t)⟩=−iℏ(ΘHΘ−1)∣ψT(t)⟩.\begin{aligned} \frac{d}{dt}\lvert\psi_T(t)\rangle &= \Theta\left( \frac{i}{\hbar}H\lvert\psi(-t)\rangle \right) \\ &= -\frac{i}{\hbar} \Theta H\lvert\psi(-t)\rangle \\ &= -\frac{i}{\hbar} (\Theta H\Theta^{-1}) \lvert\psi_T(t)\rangle. \end{aligned}

Therefore

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 ΘHΘ−1=H\Theta H\Theta^{-1}=H, the transformed state obeys the same Schrödinger equation. The antilinear conjugation of ii is exactly what makes the sign come out correctly.

What Would Go Wrong for a Unitary Operator

Section titled “What Would Go Wrong for a Unitary Operator”

Suppose one tried to represent time reversal by a unitary operator UTU_T that leaves position fixed and reverses momentum:

UTXUT−1=X,UTPUT−1=−P.U_T X U_T^{-1}=X, \qquad U_T P U_T^{-1}=-P.

Apply this to the canonical commutator. The transformed left-hand side is

[X,−P]=−iℏI.[X,-P] = -i\hbar I.

But if UTU_T were unitary, it would leave the scalar ii untouched:

UT[X,P]UT−1=UT(iℏI)UT−1=iℏI.U_T[X,P]U_T^{-1} = U_T(i\hbar I)U_T^{-1} = i\hbar I.

These two answers contradict each other. For an antiunitary operator Θ\Theta, the same calculation is consistent because

Θ(iℏI)Θ−1=−iℏI.\Theta(i\hbar I)\Theta^{-1} = -i\hbar I.

Thus the antiunitary sign is already forced by the basic position-momentum algebra.

The same point appears in the time-evolution operator

U(t)=e−iHt/ℏ.U(t)=e^{-iHt/\hbar}.

For an antiunitary Θ\Theta, the exponential transforms as

Θe−iHt/ℏΘ−1=e+i(ΘHΘ−1)t/ℏ.\Theta e^{-iHt/\hbar}\Theta^{-1} = e^{+i(\Theta H\Theta^{-1})t/\hbar}.

This follows term by term from the power series: each scalar coefficient is complex-conjugated. If HH is time-reversal invariant, then

ΘU(t)Θ−1=e+iHt/ℏ=U(−t).\Theta U(t)\Theta^{-1} = e^{+iHt/\hbar} = U(-t).

This is the clean operator statement that time reversal maps forward time evolution to backward time evolution.

In a chosen orthonormal basis, any antiunitary operator can be written as

Θ=UK,\Theta=UK,

where UU is unitary and KK complex-conjugates components in that basis. This formula is useful, but it must be read with care:

  • KK depends on the chosen basis.
  • UU carries the physical part not supplied by plain conjugation.
  • The product Θ=UK\Theta=UK is the meaningful symmetry operator.

For a spinless particle in a standard position representation, one often has Θ=K\Theta=K; the concrete scalar-particle consequences are collected in Time Reversal for Spinless Particles. For a spin-1/21/2 degree of freedom in the usual SzS_z basis, a common convention is

Θ=−iσyK.\Theta=-i\sigma_yK.

The spinor convention and the proof of Θ2=−I\Theta^2=-I are developed in Time Reversal for Spin-1/2 Particles.

Time reversal leaves position even and makes momenta odd:

ΘXΘ−1=X,ΘPΘ−1=−P.\Theta\mathbf X\Theta^{-1} = \mathbf X, \qquad \Theta\mathbf P\Theta^{-1} = -\mathbf P.

Orbital angular momentum is odd because L=X×P\mathbf L=\mathbf X\times\mathbf P:

ΘLΘ−1=−L.\Theta\mathbf L\Theta^{-1} = -\mathbf L.

Spin is also time-reversal odd:

ΘSΘ−1=−S.\Theta\mathbf S\Theta^{-1} = -\mathbf S.

The antiunitary nature of Θ\Theta is not a separate decorative feature added after these sign rules. It is what makes the sign rules compatible with the algebra of quantum observables.

For a spinless particle in a real scalar potential,

H=P22m+V(X),H = \frac{P^2}{2m}+V(X),

time reversal is a symmetry because P2P^2 and V(X)V(X) are unchanged. In a basis where Θ=K\Theta=K, this Hamiltonian is real in the position representation.

With magnetic fields, the test is more delicate. A Zeeman term

HZ=−γS⋅BH_Z = -\gamma\mathbf S\cdot\mathbf B

transforms as

ΘHZ(B)Θ−1=HZ(−B).\Theta H_Z(\mathbf B)\Theta^{-1} = H_Z(-\mathbf B).

The family of Hamiltonians is covariant if the magnetic field is also reversed. A single Hamiltonian with a fixed nonzero external B\mathbf B is not time-reversal invariant. This distinction is essential in applications to spin dynamics, Kramers degeneracy, and symmetry classification.

Antiunitarity alone does not determine Θ2\Theta^2. Depending on the Hilbert-space sector,

Θ2=+IorΘ2=−I\Theta^2=+I \qquad\text{or}\qquad \Theta^2=-I

can occur. Spinless systems often have Θ2=+I\Theta^2=+I. A single spin-1/21/2 degree of freedom has Θ2=−I\Theta^2=-I. More generally, a pure angular-momentum multiplet with quantum number jj has the familiar pattern

Θ2=(−1)2jI.\Theta^2=(-1)^{2j}I.

The sign cannot be changed by multiplying Θ\Theta by a phase. If Θ′=eiχΘ\Theta'=e^{i\chi}\Theta, then antilinearity gives

(Θ′)2=eiχe−iχΘ2=Θ2.(\Theta')^2 = e^{i\chi}e^{-i\chi}\Theta^2 = \Theta^2.

This invariant square is what makes Kramers Degeneracy possible when Θ2=−I\Theta^2=-I.

  • Treating Θ\Theta as a unitary operator that happens to reverse momenta.
  • Forgetting that Θ(a∣ψ⟩)=a∗Θ∣ψ⟩\Theta(a\lvert\psi\rangle)=a^*\Theta\lvert\psi\rangle.
  • Saying “time reversal means t↦−tt\mapsto -t” without specifying the Hilbert-space operator.
  • Treating KK as basis-independent.
  • Testing a magnetic-field Hamiltonian while keeping a time-reversal-odd external field fixed.
  • Assuming that antiunitary time reversal always has the same square in every physical sector.
  • E. P. Wigner, Group Theory and Its Application to the Quantum Mechanics of Atomic Spectra, Academic Press, 1959.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • L. E. Ballentine, Quantum Mechanics: A Modern Development, 2nd ed., World Scientific, 2014.
  • A. Messiah, Quantum Mechanics, Dover, 1999.
  • M. Tinkham, Group Theory and Quantum Mechanics, Dover, 2003.
  1. Use the canonical commutator to show that a unitary operator cannot leave XX fixed while reversing PP.
Solution

If UTU_T were unitary with UTXUT−1=XU_TXU_T^{-1}=X and UTPUT−1=−PU_TPU_T^{-1}=-P, then

UT[X,P]UT−1=[X,−P]=−iℏI.U_T[X,P]U_T^{-1} = [X,-P] = -i\hbar I.

But unitary conjugation leaves the scalar ii unchanged, so the same expression is

UT(iℏI)UT−1=iℏI.U_T(i\hbar I)U_T^{-1} = i\hbar I.

This contradiction is removed when the operator is antiunitary, because antiunitarity sends ii to −i-i.

  1. Prove the propagator identity
Θe−iHt/ℏΘ−1=e+i(ΘHΘ−1)t/ℏ\Theta e^{-iHt/\hbar}\Theta^{-1} = e^{+i(\Theta H\Theta^{-1})t/\hbar}

for antiunitary Θ\Theta.

Solution

Expand the exponential:

e−iHt/ℏ=∑n=0∞1n!(−itℏ)nHn.e^{-iHt/\hbar} = \sum_{n=0}^\infty \frac{1}{n!} \left(-\frac{it}{\hbar}\right)^n H^n.

Antiunitarity conjugates the scalar coefficient and conjugates the operator product:

Θ[(−itℏ)nHn]Θ−1=(+itℏ)n(ΘHΘ−1)n.\Theta \left[ \left(-\frac{it}{\hbar}\right)^nH^n \right] \Theta^{-1} = \left(+\frac{it}{\hbar}\right)^n (\Theta H\Theta^{-1})^n.

Summing the series gives the stated identity.

  1. A single spin-1/21/2 in a fixed magnetic field has Hamiltonian H=−γS⋅BH=-\gamma\mathbf S\cdot\mathbf B. Is this Hamiltonian time-reversal invariant?
Solution

Spin is time-reversal odd:

ΘSΘ−1=−S.\Theta\mathbf S\Theta^{-1} = -\mathbf S.

If the external field is kept fixed, then

ΘH(B)Θ−1=γS⋅B≠H(B)\Theta H(\mathbf B)\Theta^{-1} = \gamma\mathbf S\cdot\mathbf B \neq H(\mathbf B)

unless B=0\mathbf B=0. The family is covariant under B↦−B\mathbf B\mapsto-\mathbf B, since

ΘH(B)Θ−1=H(−B).\Theta H(\mathbf B)\Theta^{-1} = H(-\mathbf B).

So a fixed nonzero magnetic field breaks time-reversal symmetry, while the field-reversed comparison is time-reversal covariant.