Skip to content

Aharonov–Bohm Effect

The Aharonov–Bohm effect is the standard example where quantum phase sees more than the local electromagnetic field along a particle’s path. A charged particle can move through a region with B=0\mathbf B=\mathbf 0 and still acquire a measurable interference phase from magnetic flux enclosed by its path.

The geometric statement is sharper than “the vector potential is physical.” The vector potential is gauge dependent. The observable quantity is the gauge-invariant holonomy

exp⁡(iqℏ∮CA⋅dr),\exp \left( \frac{iq}{\hbar} \oint_C \mathbf A\cdot d\mathbf r \right),

for a closed loop CC in the accessible configuration space. When CC winds around an excluded flux tube, this holonomy can be nontrivial even though ∇×A=0\nabla\times\mathbf A=0 everywhere on the accessible path.

The wave-mechanics derivation and ring-spectrum first encounter are in Aharonov–Bohm Effect: First Encounter. This page owns the gauge, holonomy, and topology interpretation.

The magnetic version uses an inaccessible region carrying flux, such as an idealized long solenoid or a shielded flux tube. Coherent charged-particle beams travel through the exterior region and recombine. In the ideal limit:

  • the accessible region excludes the flux-carrying core;
  • the magnetic field vanishes along the particle paths;
  • the vector potential has nonzero circulation around loops that wind around the core;
  • the observed interference pattern shifts as the enclosed flux changes.

Two paths around an excluded magnetic flux region acquire an Aharonov–Bohm phase difference

Two paths enclose an inaccessible flux region. The field can vanish along both paths while the closed-loop phase ΔφAB=(q/ℏ)∮A⋅dr\Delta\varphi_{\mathrm{AB}}=(q/\hbar)\oint\mathbf A\cdot d\mathbf r remains measurable through interference.

The effect is not a claim that a hidden Lorentz force acts along the exterior paths. In the ideal magnetic setup, the local force law sees E=0\mathbf E=\mathbf 0 and B=0\mathbf B=\mathbf 0 where the particle travels. The interference pattern sees the relative phase of amplitudes that wind differently around an excluded region.

For a particle of charge qq minimally coupled to a vector potential, the Hamiltonian contains

p^⟼p^−qA.\hat{\mathbf p} \longmapsto \hat{\mathbf p}-q\mathbf A.

Along a path Γ\Gamma, the magnetic contribution to the quantum phase is

φΓ=qℏ∫ΓA⋅dr.\varphi_\Gamma = \frac{q}{\hbar} \int_\Gamma \mathbf A\cdot d\mathbf r.

For two paths Γ1\Gamma_1 and Γ2\Gamma_2 with common endpoints, the observable phase difference is the closed-loop integral over C=Γ1−Γ2C=\Gamma_1-\Gamma_2:

ΔφAB=qℏ(∫Γ1A⋅dr−∫Γ2A⋅dr)=qℏ∮CA⋅dr.\begin{aligned} \Delta\varphi_{\mathrm{AB}} &= \frac{q}{\hbar} \left( \int_{\Gamma_1}\mathbf A\cdot d\mathbf r - \int_{\Gamma_2}\mathbf A\cdot d\mathbf r \right)\\ &= \frac{q}{\hbar} \oint_C \mathbf A\cdot d\mathbf r. \end{aligned}

If the loop encloses magnetic flux ΦB\Phi_B with the chosen orientation, then

∮CA⋅dr=ΦB,\oint_C \mathbf A\cdot d\mathbf r = \Phi_B,

so

ΔφAB=qΦBℏmod⁡2π.\Delta\varphi_{\mathrm{AB}} = \frac{q\Phi_B}{\hbar} \quad \operatorname{mod} 2\pi.

The interference pattern is periodic under

ΦB↦ΦB+Φ0,Φ0=h∣q∣.\Phi_B \mapsto \Phi_B+\Phi_0, \qquad \Phi_0 = \frac{h}{\lvert q\rvert}.

For electrons, q=−eq=-e, so the sign of the phase depends on the loop orientation and charge convention. The physical fringe shift is the phase modulo 2π2\pi.

A gauge transformation changes the vector potential by

A↦A+∇χ,\mathbf A \mapsto \mathbf A+\nabla\chi,

and the wavefunction by a compensating local phase. With the convention p↦p−qAp\mapsto p-qA,

ψ↦exp⁡(iqχℏ)ψ.\psi \mapsto \exp \left( \frac{iq\chi}{\hbar} \right) \psi.

For an open path, the line integral changes by an endpoint term:

∫Γ(A+∇χ)⋅dr=∫ΓA⋅dr+χ(b)−χ(a).\int_\Gamma \left( \mathbf A+\nabla\chi \right)\cdot d\mathbf r = \int_\Gamma \mathbf A\cdot d\mathbf r + \chi(b)-\chi(a).

That is why a single open-path phase is not separately gauge invariant. In an interference experiment the endpoint phase changes are also carried by the transformed wavefunctions, so the physical relative phase is unchanged.

For a closed loop and a single-valued gauge function,

∮C∇χ⋅dr=0.\oint_C \nabla\chi\cdot d\mathbf r = 0.

Thus the phase factor

W(C)=exp⁡(iqℏ∮CA⋅dr)W(C) = \exp \left( \frac{iq}{\hbar} \oint_C \mathbf A\cdot d\mathbf r \right)

is gauge invariant. This loop phase is the abelian Wilson loop of the electromagnetic connection in nonrelativistic quantum mechanics.

The essential geometry is not that B\mathbf B is nonzero on the particle path. It is that the accessible configuration space has a hole. In the idealized planar setup, the particle moves in the punctured plane

M=R2∖{0},M = \mathbb R^2\setminus\{0\},

or, more realistically, in the complement of a finite-radius flux tube. Loops in MM are labeled by an integer winding number around the excluded region.

A convenient exterior vector potential for a thin flux tube is

A=ΦB2πrθ^.\mathbf A = \frac{\Phi_B}{2\pi r} \hat{\boldsymbol\theta}.

For r>0r>0,

∇×A=0,\nabla\times\mathbf A = \mathbf 0,

but a counterclockwise circle of radius rr has

∮A⋅dr=∫02πΦB2πr(r dθ)=ΦB.\begin{aligned} \oint \mathbf A\cdot d\mathbf r &= \int_0^{2\pi} \frac{\Phi_B}{2\pi r} \left( r\,d\theta \right)\\ &= \Phi_B. \end{aligned}

For a loop with winding number ww,

∮CA⋅dr=wΦB,ΔφAB=qwΦBℏ.\oint_C \mathbf A\cdot d\mathbf r = w\Phi_B, \qquad \Delta\varphi_{\mathrm{AB}} = \frac{qw\Phi_B}{\hbar}.

This is the simplest quantum-mechanical example of a flat connection with nontrivial holonomy. Locally, the connection can look pure gauge. Globally, a loop that winds around the removed region cannot be shrunk to a point without leaving the accessible space.

The phrase “topological” needs some care. The winding number is topological, and the phase is insensitive to smooth deformations of the paths that preserve the winding and avoid the flux. The phase is not quantized by topology alone; it varies continuously with ΦB\Phi_B and becomes physically periodic only modulo the flux quantum.

A common paradox is to combine ∇×A=0\nabla\times\mathbf A=0 outside the solenoid with Stokes theorem and conclude that the loop integral must vanish. The missing assumption is the existence of a smooth surface in the accessible region whose boundary is the loop and on which the same smooth vector potential is defined.

For a loop that winds around the excluded flux tube, every spanning disk crosses the removed region. If one allows a surface that cuts through the solenoid, then the magnetic field through the excluded core contributes:

∮CA⋅dr=∫ΣB⋅dS=ΦB.\oint_C \mathbf A\cdot d\mathbf r = \int_\Sigma \mathbf B\cdot d\mathbf S = \Phi_B.

If one restricts to the accessible region, no such disk exists for a winding loop. That is the topology. Stokes theorem is not failing; its hypotheses are being violated by the puncture or by the need for multiple patches.

The Aharonov–Bohm phase and Berry phase are both closed-loop phases, but their connections live over different spaces.

In the Aharonov–Bohm effect, the connection is the electromagnetic vector potential over the particle’s configuration space. The loop is a real-space loop around excluded flux:

γAB[C]=qℏ∮CA⋅dr.\gamma_{\mathrm{AB}}[C] = \frac{q}{\hbar} \oint_C \mathbf A\cdot d\mathbf r.

In Berry phase, the connection is built from parameter-dependent eigenvectors:

An(R)=i⟨n(R)∣∇Rn(R)⟩,γn[C]=∮CAn(R)⋅dR.\mathbf A_n(R) = i\langle n(R)|\nabla_R n(R)\rangle, \qquad \gamma_n[C] = \oint_C \mathbf A_n(R)\cdot dR.

The shared word is holonomy: a phase remains after transporting around a closed loop. The difference is physical origin. Aharonov–Bohm phase is electromagnetic gauge holonomy in configuration space; Berry phase is eigenstate-bundle holonomy in parameter space under adiabatic evolution.

There is also a useful contrast in curvature. In many Berry examples, a nonzero local Berry curvature contributes to the phase through a surface flux. In the ideal magnetic Aharonov–Bohm exterior, the local magnetic field strength vanishes on the accessible region, but the space is not simply connected. This makes the Aharonov–Bohm effect a clean reminder that zero local curvature does not always imply trivial global holonomy.

The effect was proposed by Aharonov and Bohm in 1959 and observed in electron interference experiments soon after. Later experiments with improved shielding addressed the worry that stray magnetic fields or forces were responsible for the fringe shift.

The modern lesson is not that gauge choices themselves are observable. It is that electromagnetic gauge potentials encode global phase information whose gauge-invariant content can appear in interference. This lesson reappears in mesoscopic rings, persistent currents, superconducting flux quantization, quantum Hall systems, and topological phases of matter.

The electric Aharonov–Bohm effect is a related effect involving scalar potentials and time-dependent phases. This page focuses on the magnetic case because it most directly displays holonomy around an excluded region.

  • Saying A\mathbf A itself is directly observable. The gauge-invariant object is the closed-loop phase factor.
  • Treating B=0\mathbf B=0 along the paths as implying zero phase. The loop can enclose flux outside the accessible region.
  • Applying Stokes theorem on a spanning surface that crosses an excluded region without accounting for the flux there.
  • Forgetting the charge sign and loop orientation when comparing formulas.
  • Calling the phase purely topological. The winding class is topological, but the phase also depends continuously on ΦB\Phi_B modulo Φ0\Phi_0.
  • Confusing Aharonov–Bohm holonomy in real space with Berry holonomy in parameter space.
  • Y. Aharonov and D. Bohm, “Significance of electromagnetic potentials in the quantum theory,” Physical Review 115, 485-491, 1959.
  • R. G. Chambers, “Shift of an electron interference pattern by enclosed magnetic flux,” Physical Review Letters 5, 3-5, 1960.
  • A. Tonomura et al., “Evidence for Aharonov–Bohm effect with magnetic field completely shielded from electron wave,” Physical Review Letters 56, 792-795, 1986.
  • M. Peshkin and A. Tonomura, The Aharonov–Bohm Effect, Springer, 1989.
  • M. V. Berry, “Quantal phase factors accompanying adiabatic changes,” Proceedings of the Royal Society A 392, 45-57, 1984.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  1. Compute the loop integral for the thin-flux-tube potential.

Let

A=ΦB2πrθ^\mathbf A = \frac{\Phi_B}{2\pi r} \hat{\boldsymbol\theta}

for r>0r>0. Show that a counterclockwise circle centered on the flux tube has Aharonov–Bohm phase qΦB/ℏq\Phi_B/\hbar.

Solution

On a circle of radius rr, the displacement is

dr=r dθ θ^.d\mathbf r = r\,d\theta\,\hat{\boldsymbol\theta}.

Therefore

∮A⋅dr=∫02πΦB2πrr dθ=ΦB.\begin{aligned} \oint \mathbf A\cdot d\mathbf r &= \int_0^{2\pi} \frac{\Phi_B}{2\pi r} r\,d\theta\\ &= \Phi_B. \end{aligned}

The phase is

ΔφAB=qℏ∮A⋅dr=qΦBℏ.\Delta\varphi_{\mathrm{AB}} = \frac{q}{\hbar} \oint \mathbf A\cdot d\mathbf r = \frac{q\Phi_B}{\hbar}.
  1. Show gauge invariance of the closed-loop phase.

Suppose A↦A+∇χ\mathbf A\mapsto\mathbf A+\nabla\chi with a single-valued χ\chi on the loop. Show that W(C)W(C) is unchanged.

Solution

The exponent changes by

iqℏ∮C∇χ⋅dr.\frac{iq}{\hbar} \oint_C \nabla\chi\cdot d\mathbf r.

Along the closed loop, this integral is

χ(endpoint)−χ(startpoint)=0\chi(\text{endpoint})-\chi(\text{startpoint}) = 0

for a single-valued χ\chi. Hence

W(C)=exp⁡(iqℏ∮CA⋅dr)W(C) = \exp \left( \frac{iq}{\hbar} \oint_C \mathbf A\cdot d\mathbf r \right)

is unchanged.

  1. Include winding number.

A loop winds ww times around the excluded flux region. What is the phase, and what flux change leaves the interference pattern invariant?

Solution

The loop integral is multiplied by the winding number:

∮CA⋅dr=wΦB.\oint_C \mathbf A\cdot d\mathbf r = w\Phi_B.

Thus

ΔφAB=qwΦBℏ.\Delta\varphi_{\mathrm{AB}} = \frac{qw\Phi_B}{\hbar}.

The interference pattern is unchanged when the phase changes by 2πk2\pi k with k∈Zk\in\mathbb Z. For one winding, the smallest positive flux period in magnitude is

Φ0=h∣q∣.\Phi_0 = \frac{h}{\lvert q\rvert}.

For fixed winding w≠0w\ne0, changing the flux by Φ0/∣w∣\Phi_0/\lvert w\rvert changes this loop phase by 2π2\pi in magnitude, although the fundamental flux periodicity of a system containing all allowed winding sectors remains Φ0\Phi_0.

  1. Compare Aharonov–Bohm and Berry phases.

Give one similarity and one difference between the two phases.

Solution

A similarity is that both are holonomies: they are phases associated with closed-loop transport and are physically meaningful modulo 2π2\pi.

A difference is the base space and connection. The Aharonov–Bohm phase comes from the electromagnetic vector potential over real configuration space. Berry phase comes from a connection built from parameter-dependent eigenvectors over parameter space, usually under an adiabatic assumption.