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Holonomy

Holonomy is the transformation left after a state, vector, or internal degree of freedom is transported around a closed loop. In quantum mechanics, the most common holonomy is a phase:

∣ψ⟩⟼eiγ∣ψ⟩.\lvert\psi\rangle \longmapsto e^{i\gamma}\lvert\psi\rangle.

The central example in this chapter is Berry phase. When a nondegenerate eigenstate is transported adiabatically around a closed loop CC in parameter space, the geometric part of the phase is the holonomy of the Berry connection:

eiγn[C]=exp⁡(i∮CAn),An=i⟨n(R)∣dn(R)⟩.e^{i\gamma_n[C]} = \exp \left( i\oint_C A_n \right), \qquad A_n=i\langle n(R)|d n(R)\rangle.

The abstract mathematical notion is covered in Holonomy. This page explains how the same idea appears in quantum phases, spin examples, electromagnetic loop phases, and degenerate eigenspaces.

Along an open path, transport compares different fibers: the state line or eigenspace at the initial parameter value with the one at the final parameter value. Along a closed loop, the starting and ending base point are the same, so the result can be compared directly with the identity.

For a nondegenerate adiabatic eigenstate, the transported line returns to itself:

R(T)=R(0),C∣n(T)⟩=C∣n(0)⟩.R(T)=R(0), \qquad \mathbb C\lvert n(T)\rangle = \mathbb C\lvert n(0)\rangle.

The vector representative can still return with a phase. After removing the dynamical phase,

∣n(0)⟩⟼eiγn[C]∣n(0)⟩.\lvert n(0)\rangle \longmapsto e^{i\gamma_n[C]} \lvert n(0)\rangle.

That phase factor is the Berry holonomy.

The Berry connection is the local one-form

An=i⟨n(R)∣dn(R)⟩.A_n = i\langle n(R)|d n(R)\rangle.

Pull it back to a time-parametrized loop R(t)R(t):

At(t)=i⟨n(R(t))|ddtn(R(t))⟩.A_t(t) = i\left\langle n(R(t)) \middle| \frac{d}{dt}n(R(t)) \right\rangle.

Then the Berry phase is

γn[C]=∫0TAt(t) dt=∮CAn.\gamma_n[C] = \int_0^T A_t(t)\,dt = \oint_C A_n.

The total adiabatic phase is

αn=−1ℏ∫0TEn(t) dt+γn[C].\alpha_n = -\frac{1}{\hbar} \int_0^T E_n(t)\,dt + \gamma_n[C].

Holonomy names the second term’s geometric origin. The first term records energy over time; the second records closed-loop transport of the eigenline.

The local eigenvector may be rephased:

∣n(R)⟩↦eiχ(R)∣n(R)⟩.\lvert n(R)\rangle \mapsto e^{i\chi(R)} \lvert n(R)\rangle.

With the convention used here,

An↦An−dχ.A_n \mapsto A_n-d\chi.

Thus

γn[C]↦γn[C]−∮Cdχ.\gamma_n[C] \mapsto \gamma_n[C] - \oint_C d\chi.

For a smooth single-valued phase choice around the loop, ∮Cdχ=0\oint_Cd\chi=0. More generally the phase itself is defined modulo 2π2\pi, while the phase factor eiγn[C]e^{i\gamma_n[C]} is the invariant object. This is why a Berry connection can be gauge dependent while its closed-loop holonomy is physically meaningful.

Berry curvature is the local field

Fn=dAn.F_n=dA_n.

If the loop CC bounds an oriented surface Σ\Sigma and a smooth gauge is available on that surface, Stokes’ theorem gives

γn[C]=∫ΣFnmod⁡2π.\gamma_n[C] = \int_\Sigma F_n \quad \operatorname{mod}2\pi.

This is the curvature-flux formula for Berry phase. It is useful, but it has assumptions. If the surface passes through a degeneracy, if no single smooth gauge covers it, or if the accessible parameter space has holes, the holonomy may be well-defined even though the naive one-patch flux calculation fails.

The practical rule is:

  • small contractible loops measure local curvature;
  • large or noncontractible loops can also measure global topology and gauge patching;
  • a flat local connection can still have nontrivial holonomy on a space with noncontractible loops.

Along an open path, one can choose a Parallel Transport phase convention in which

At(t)=i⟨n(t)∣n˙(t)⟩=0.A_t(t) = i\langle n(t)|\dot n(t)\rangle = 0.

This is a parallel-transport gauge: the eigenvector representative is chosen so that it has no local phase rotation along the path. For a closed loop, this gauge may not return to the original vector phase. Instead,

∣n(T)⟩pt=eiγn[C]∣n(0)⟩pt.\lvert n(T)\rangle_{\mathrm{pt}} = e^{i\gamma_n[C]} \lvert n(0)\rangle_{\mathrm{pt}}.

The holonomy is precisely the obstruction to choosing a single phase convention that is locally parallel and globally returns unchanged.

Parallel transport of tangent vectors on a sphere is the classical picture to keep nearby. A vector carried around a closed curve on a curved surface can return rotated even though it was kept locally parallel at every point.

Berry holonomy is analogous, but the transported object is not usually a tangent vector in physical space. It is a phase line or eigenspace over parameter space. The loop might be a loop of magnetic-field directions, molecular coordinates, crystal momenta, or other control parameters.

The analogy is structural:

closed-loop transport⟶final mismatch.\text{closed-loop transport} \quad\longrightarrow\quad \text{final mismatch}.

The type of mismatch depends on the connection: a rotation for tangent vectors, a phase for a U(1)U(1) quantum eigenline, and a matrix for a degenerate eigenspace.

For a spin-1/21/2 adiabatically following a magnetic-field direction, the parameter space at fixed field magnitude is a sphere. In the convention used in Berry Phase for Spin-1/2, the aligned state has

γ+[C]=−Ω[C]2,\gamma_+[C] = -\frac{\Omega[C]}{2},

where Ω[C]\Omega[C] is the oriented solid angle enclosed by the loop of field directions.

The corresponding holonomy is

eiγ+[C]=exp⁡(−iΩ[C]2).e^{i\gamma_+[C]} = \exp \left( -\frac{i\Omega[C]}{2} \right).

This is not a statement that the spin is literally being carried along the surface like a tangent arrow. It is a statement that the eigenline over the field-direction sphere has a Berry connection whose closed-loop holonomy is controlled by solid angle.

The Aharonov–Bohm phase is a close cousin of Berry holonomy, but the base space and connection are different. A charged particle encircling magnetic flux Φ\Phi acquires

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

in the common minimal-coupling convention. Here A\mathbf A is the electromagnetic vector potential over physical configuration space, not the Berry connection over Hamiltonian parameter space.

The family resemblance is important: both are loop phases of a connection. The distinction is equally important: Berry phase comes from adiabatic transport of eigenstates, while the Aharonov–Bohm phase comes from electromagnetic gauge holonomy around inaccessible flux. See Aharonov–Bohm Effect for the physical setup.

If an isolated eigenspace has dimension r>1r>1, adiabatic transport can rotate states within that subspace. Choose an orthonormal local basis ∣n,a(R)⟩\lvert n,a(R)\rangle, a=1,…,ra=1,\ldots,r, and define the matrix-valued Berry connection

Aab=i⟨n,a(R)∣dn,b(R)⟩.\mathcal A_{ab} = i\langle n,a(R)|d n,b(R)\rangle.

The holonomy around a loop is a unitary matrix

UC=Pexp⁡(i∮CA),\mathcal U_C = \mathcal P \exp \left( i\oint_C \mathcal A \right),

with path ordering P\mathcal P because matrices at different points need not commute. Under a change of basis inside the degenerate subspace, UC\mathcal U_C changes by conjugation at the base point. Its eigenvalues and trace-type data are the gauge-invariant content.

This is the Wilczek–Zee or nonabelian Berry phase setting; see Non-Abelian Berry Phase Preview.

Holonomy is not just “phase caused by going in a circle.” The loop must be accompanied by a connection that tells what it means to transport the state. A cyclic time-dependent Hamiltonian can produce ordinary dynamical phase, nonadiabatic transitions, or resonant rotations without being well described by Berry holonomy.

Holonomy is also not automatically topological. A Berry phase can change continuously when the loop is deformed. It becomes topologically constrained only when extra conditions apply, such as quantized curvature flux over a closed surface, a noncontractible loop with protected flux, or a symmetry/gap condition that prevents smooth deformation to a trivial value.

  • Calling any cyclic phase a holonomy without specifying the connection and transported object.
  • Confusing the Berry connection with the electromagnetic vector potential.
  • Assuming a Berry phase is always topological.
  • Applying the curvature-flux formula across a degeneracy or gauge singularity.
  • Treating the phase γ\gamma rather than the phase factor eiγe^{i\gamma} as absolutely defined.
  • Forgetting that nonabelian holonomy matrices are basis covariant, not individually gauge invariant.
  • Dropping the dynamical phase when predicting a measured total phase.
  • B. Simon, “Holonomy, the quantum adiabatic theorem, and Berry’s phase,” Physical Review Letters 51, 2167-2170, 1983.
  • M. V. Berry, “Quantal phase factors accompanying adiabatic changes,” Proceedings of the Royal Society A 392, 45-57, 1984.
  • Y. Aharonov and D. Bohm, “Significance of electromagnetic potentials in the quantum theory,” Physical Review 115, 485-491, 1959.
  • F. Wilczek and A. Zee, “Appearance of gauge structure in simple dynamical systems,” Physical Review Letters 52, 2111-2114, 1984.
  • A. Shapere and F. Wilczek, eds., Geometric Phases in Physics, World Scientific, 1989.
  • M. Nakahara, Geometry, Topology and Physics, 2nd ed., CRC Press, 2003.
  1. Show that eiγ[C]e^{i\gamma[C]} is unchanged under A↦A−dχA\mapsto A-d\chi for a smooth single-valued χ\chi around a closed loop.
Solution

The transformed phase is

γ′[C]=∮C(A−dχ)=γ[C]−∮Cdχ.\gamma'[C] = \oint_C(A-d\chi) = \gamma[C]-\oint_Cd\chi.

For a closed loop and single-valued χ\chi,

∮Cdχ=χ(end)−χ(start)=0.\oint_Cd\chi = \chi(\text{end})-\chi(\text{start}) = 0.

Therefore γ′[C]=γ[C]\gamma'[C]=\gamma[C], and the phase factor is unchanged. If the phase changes by 2πk2\pi k under a large convention change, eiγe^{i\gamma} is still unchanged.

  1. A spin-1/21/2 aligned eigenstate follows a loop enclosing oriented solid angle Ω=π\Omega=\pi. In the convention γ=−Ω/2\gamma=-\Omega/2, what is the holonomy phase factor?
Solution

The Berry phase is

γ=−π2.\gamma = -\frac{\pi}{2}.

The phase factor is

eiγ=e−iπ/2=−i.e^{i\gamma} = e^{-i\pi/2} = -i.
  1. A charged particle of charge qq encircles flux Φ=h/q\Phi=h/q once. What is the Aharonov–Bohm phase factor in the convention above?
Solution

The phase is

Δφ=qΦℏ=q(h/q)ℏ=hℏ=2π.\Delta\varphi = \frac{q\Phi}{\hbar} = \frac{q(h/q)}{\hbar} = \frac{h}{\hbar} = 2\pi.

Therefore the phase factor is

eiΔφ=ei2π=1.e^{i\Delta\varphi} = e^{i2\pi} = 1.
  1. Why does F=0F=0 not always imply trivial holonomy?
Solution

Curvature is local. On a space with noncontractible loops, a flat connection can still have a nonzero integral around a loop. For example, on a circle,

A=α dθA=\alpha\,d\theta

has

F=dA=0,F=dA=0,

but

∮A=∫02πα dθ=2πα.\oint A = \int_0^{2\pi}\alpha\,d\theta = 2\pi\alpha.

The holonomy is ei2παe^{i2\pi\alpha}, which need not be 11.

  1. In the nonabelian case, why is path ordering needed?
Solution

The connection is matrix-valued. Matrices evaluated at different points along the loop need not commute:

[A(t1),A(t2)]≠0.[\mathcal A(t_1),\mathcal A(t_2)] \ne 0.

The ordered exponential records the sequence in which infinitesimal transports are applied. Without path ordering, the exponential would treat noncommuting factors as though their order did not matter.