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Gauge Transformations: First Encounter

Gauge transformations are changes of electromagnetic potentials that leave the electric and magnetic fields unchanged. In wave mechanics they also change the local phase convention of a charged-particle wavefunction. The physical state is not changed; the description is.

This page is a first encounter inside nonrelativistic wave mechanics. The broader structural meaning of gauge redundancy belongs to symmetry, geometry, and quantum field theory. Here the goal is practical: know how A\mathbf A, Φ\Phi, and ψ\psi transform, and know which quantities are safe to call physical.

The electromagnetic fields are

E=−∇Φ−∂A∂t,B=∇×A.\mathbf E = - \nabla\Phi - \frac{\partial\mathbf A}{\partial t}, \qquad \mathbf B = \nabla\times\mathbf A.

A gauge transformation is specified by a real scalar function χ(r,t)\chi(\mathbf r,t):

A′=A+∇χ,Φ′=Φ−∂χ∂t.\mathbf A' = \mathbf A+\nabla\chi, \qquad \Phi' = \Phi-\frac{\partial\chi}{\partial t}.

These new potentials describe the same fields. For the magnetic field,

B′=∇×A′=∇×A+∇×∇χ=B,\mathbf B' = \nabla\times\mathbf A' = \nabla\times\mathbf A + \nabla\times\nabla\chi = \mathbf B,

because the curl of a gradient vanishes. For the electric field,

E′=−∇(Φ−∂χ∂t)−∂∂t(A+∇χ)=−∇Φ−∂A∂t=E.\begin{aligned} \mathbf E' &= - \nabla\left( \Phi-\frac{\partial\chi}{\partial t} \right) - \frac{\partial}{\partial t} \left( \mathbf A+\nabla\chi \right) \\ &= - \nabla\Phi - \frac{\partial\mathbf A}{\partial t} = \mathbf E. \end{aligned}

Thus a gauge transformation changes the representative potentials, not the electromagnetic fields.

Gauge transformation changes potentials and wavefunction phase while preserving fields

A gauge transformation gives a different potential pair and a different local phase convention for the wavefunction. Gauge-invariant fields, probabilities, and currents describe the same physics.

For a particle of charge qq, minimal coupling uses

π^=−iℏ∇−qA.\hat{\boldsymbol\pi} = - i\hbar\nabla - q\mathbf A.

This kinetic momentum appears in the Hamiltonian

H^=π^ 22m+qΦ.\hat H = \frac{\hat{\boldsymbol\pi}^{\,2}}{2m} + q\Phi.

If A\mathbf A changes by ∇χ\nabla\chi, the wavefunction must change by a compensating local phase:

ψ′=exp⁡(iqχℏ)ψ.\psi' = \exp\left( \frac{iq\chi}{\hbar} \right)\psi.

This is not an optional convention. Without this phase change, the minimally coupled Schrödinger equation would not keep the same form under a gauge transformation.

The key identity is

(−iℏ∇−qA′)ψ′=exp⁡(iqχℏ)(−iℏ∇−qA)ψ.\left( -i\hbar\nabla-q\mathbf A' \right)\psi' = \exp\left( \frac{iq\chi}{\hbar} \right) \left( -i\hbar\nabla-q\mathbf A \right)\psi.

In words: the kinetic momentum acting on the transformed wavefunction gives the transformed version of the old kinetic momentum acting on the old wavefunction.

This is why π^=−iℏ∇−qA\hat{\boldsymbol\pi}=-i\hbar\nabla-q\mathbf A is called gauge-covariant. The canonical momentum −iℏ∇-i\hbar\nabla alone is not gauge-covariant.

The time-dependent part transforms similarly:

(iℏ∂∂t−qΦ′)ψ′=exp⁡(iqχℏ)(iℏ∂∂t−qΦ)ψ.\left( i\hbar\frac{\partial}{\partial t} - q\Phi' \right)\psi' = \exp\left( \frac{iq\chi}{\hbar} \right) \left( i\hbar\frac{\partial}{\partial t} - q\Phi \right)\psi.

Together these identities make the Schrödinger equation gauge-covariant.

The probability density is unchanged:

ρ′=∣ψ′∣2=∣ψ∣2=ρ.\rho' = \lvert\psi'\rvert^2 = \lvert\psi\rvert^2 = \rho.

The gauge-covariant current

j=1mRe⁡[ψ∗(−iℏ∇−qA)ψ]\mathbf j = \frac{1}{m} \operatorname{Re} \left[ \psi^* \left( -i\hbar\nabla-q\mathbf A \right)\psi \right]

is also unchanged when both A\mathbf A and ψ\psi are transformed. The local phase changes, but the vector potential changes at the same time, so the physical current agrees.

For a polar form

ψ=ReiS/ℏ,\psi = R e^{iS/\hbar},

the phase changes as

S′=S+qχ.S'=S+q\chi.

The gauge-invariant velocity field depends on the combination

∇S−qA,\nabla S-q\mathbf A,

not on ∇S\nabla S alone.

A gauge transformation maps one description to another equivalent description. A gauge choice is a decision to work in one representative.

Common examples include:

  • Coulomb gauge, ∇⋅A=0\nabla\cdot\mathbf A=0;
  • temporal gauge, Φ=0\Phi=0, when it can be imposed consistently;
  • Landau gauge for a uniform magnetic field;
  • symmetric gauge for a uniform magnetic field.

Choosing a gauge can make a calculation easier, but it should not change gauge-invariant predictions. If a computed energy, probability, or physical current depends on a gauge choice, something has been compared incorrectly or an incomplete set of states has been used.

For a uniform magnetic field

B=Bz^,\mathbf B = B\hat{\mathbf z},

two useful vector potentials are the Landau gauge

AL=Bx y^\mathbf A_L = Bx\,\hat{\mathbf y}

and the symmetric gauge

AS=B2(−y x^+x y^).\mathbf A_S = \frac{B}{2} \left( -y\,\hat{\mathbf x} + x\,\hat{\mathbf y} \right).

They differ by a gradient:

AL−AS=B2(y x^+x y^)=∇(Bxy2).\mathbf A_L-\mathbf A_S = \frac{B}{2} \left( y\,\hat{\mathbf x} + x\,\hat{\mathbf y} \right) = \nabla\left( \frac{Bxy}{2} \right).

Thus the gauge function connecting symmetric gauge to Landau gauge is

χ=Bxy2.\chi = \frac{Bxy}{2}.

If ψS\psi_S is a wavefunction in symmetric gauge, the corresponding Landau-gauge representative is

ψL=exp⁡(iqBxy2ℏ)ψS.\psi_L = \exp\left( \frac{iqBxy}{2\hbar} \right)\psi_S.

The wavefunction formulas look different, and the convenient labels are different, but the magnetic field and energy spectrum are the same.

If χ\chi is constant, the gauge transformation is just a global phase:

ψ′=eiqχ/ℏψ.\psi' = e^{iq\chi/\hbar}\psi.

If χ\chi depends on position and time, the phase is local. Local phase changes are not directly observable by themselves, but gauge-invariant phase differences around closed loops can matter. The Aharonov–Bohm effect is the standard example: a region with B=0\mathbf B=0 along the particle path can still have physically meaningful magnetic flux through an excluded region.

The lesson is not that the vector potential is itself directly observable in a gauge-dependent way. The lesson is that quantum phases, potentials, and topology must be combined into gauge-invariant quantities.

  • Changing A\mathbf A and Φ\Phi without changing the wavefunction phase.
  • Treating the canonical momentum −iℏ∇-i\hbar\nabla as the mechanical momentum in a vector potential.
  • Saying the vector potential is “unphysical” and then ignoring its role in the wave equation.
  • Comparing wavefunctions written in different gauges as if they were the same representative.
  • Expecting gauge-dependent labels, such as a particular conserved canonical momentum in a chosen gauge, to be universal observables.
  • Confusing gauge redundancy with an ordinary physical symmetry that maps one physical state to a different physical state.
  1. Verify that the gauge transformation leaves B\mathbf B unchanged.
Solution

Using

A′=A+∇χ,\mathbf A' = \mathbf A+\nabla\chi,

we find

B′=∇×A′=∇×A+∇×∇χ.\mathbf B' = \nabla\times\mathbf A' = \nabla\times\mathbf A + \nabla\times\nabla\chi.

Since ∇×∇χ=0\nabla\times\nabla\chi=0,

B′=B.\mathbf B'=\mathbf B.
  1. Show that the probability density is gauge invariant.
Solution

The transformed wavefunction is

ψ′=eiqχ/ℏψ.\psi' = e^{iq\chi/\hbar}\psi.

Since the phase has unit magnitude,

∣ψ′∣2=∣eiqχ/ℏ∣2∣ψ∣2=∣ψ∣2.\lvert\psi'\rvert^2 = \left\lvert e^{iq\chi/\hbar}\right\rvert^2 \lvert\psi\rvert^2 = \lvert\psi\rvert^2.
  1. Find the gauge function connecting AS=B2(−y x^+x y^)\mathbf A_S=\frac{B}{2}(-y\,\hat{\mathbf x}+x\,\hat{\mathbf y}) to AL=Bx y^\mathbf A_L=Bx\,\hat{\mathbf y}.
Solution

Compute the difference:

AL−AS=B2(y x^+x y^).\mathbf A_L-\mathbf A_S = \frac{B}{2} \left( y\,\hat{\mathbf x} + x\,\hat{\mathbf y} \right).

This is the gradient of

χ=Bxy2,\chi = \frac{Bxy}{2},

because

∇χ=B2(y x^+x y^).\nabla\chi = \frac{B}{2} \left( y\,\hat{\mathbf x} + x\,\hat{\mathbf y} \right).
  1. Why is the current formula with π^\hat{\boldsymbol\pi} safer than the free-particle current formula when A≠0\mathbf A\ne0?
Solution

The free-particle current uses only the phase gradient of ψ\psi. Under a local gauge transformation, that phase gradient changes. The vector potential changes at the same time, and the gauge-invariant combination is

∇S−qA.\nabla S-q\mathbf A.

Equivalently, the current should be built from

π^=−iℏ∇−qA.\hat{\boldsymbol\pi} = -i\hbar\nabla-q\mathbf A.

This makes the current transform consistently and gives the same physical current in equivalent gauges.

  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics, Wiley, 1977.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • Y. Aharonov and D. Bohm, “Significance of Electromagnetic Potentials in the Quantum Theory,” Physical Review 115, 485-491, 1959.