Berry Phase Problems
These solved problems practice geometric phase calculations: line integrals of Berry connections, gauge changes, spin- solid angles, Aharonov–Bohm holonomy, Berry-curvature flux, and Chern-number normalization.
Use Berry Phase for the physical setup, Berry Connection for gauge conventions, Berry Curvature for flux language, and Berry Phase for Spin-1/2 for the spin convention used below. The Aharonov–Bohm examples use Aharonov–Bohm Effect.
Conventions
Section titled “Conventions”For a nondegenerate instantaneous eigenstate,
the Berry connection is
For a closed loop ,
Under a phase convention change
the connection transforms as
The curvature is
For the spin- Hamiltonian
the lower state has
where is the oriented solid angle enclosed by the loop of on the unit sphere.
For an electromagnetic Aharonov–Bohm loop,
For a closed oriented two-dimensional parameter space,
Skill Map
Section titled “Skill Map”| Problem group | Skills | Preparation |
|---|---|---|
| Gauge changes | connection transformation, closed-loop phase | Berry Connection |
| Spin- loops | solid angle, dynamical versus geometric phase | Berry Phase for Spin-1/2 |
| Curvature flux | exterior derivative, Stokes’ theorem, monopole analogy | Berry Curvature |
| Aharonov–Bohm holonomy | winding number, flux phase, gauge invariance | Aharonov–Bohm Effect |
| Chern numbers | normalized curvature flux, gap protection | Chern Numbers |
Problems
Section titled “Problems”1. Gauge Shift Around a Circle
Section titled “1. Gauge Shift Around a Circle”On a parameter circle with coordinate , suppose a Berry connection is
where is constant. Compute the Berry phase around the circle. Then apply the gauge change with integer and check what happens to the phase factor.
Solution
The Berry phase is
Under
and
the connection becomes
The transformed loop integral is
The phase factor is unchanged:
The integer condition matters because is single-valued on the circle only when is an integer.
2. Constant-Polar-Angle Spin Loop
Section titled “2. Constant-Polar-Angle Spin Loop”For the spin convention in this volume, the lower state has Berry connection
Compute the Berry phase for a loop at fixed with . Evaluate the result for the north pole, the equator, and reversed orientation.
Solution
At fixed ,
Therefore
The solid angle of the cap is
so
At the north pole, , so
At the equator, , so
If the loop orientation is reversed, the line integral changes sign:
Only the phase factor is physically invariant modulo .
3. Dynamical Phase Versus Berry Phase
Section titled “3. Dynamical Phase Versus Berry Phase”For
the system remains in the lower instantaneous eigenstate while traces a closed loop of solid angle in time . Assume is constant. Find the total phase in the adiabatic approximation.
Solution
The lower-state energy is
The dynamical phase is
The Berry phase for the chosen convention is
Thus the total phase is
Changing the traversal time changes the first term. Keeping the same oriented loop in the adiabatic limit keeps the second term fixed.
4. Curvature from the Spin Connection
Section titled “4. Curvature from the Spin Connection”Starting from
compute . Then integrate it over a spherical cap , .
Solution
Differentiate the connection:
Since
the curvature is
Integrating over the cap gives
This equals the line-integral result for the boundary circle. The cap solid angle is , so the flux is .
5. Aharonov–Bohm Phase and Flux Period
Section titled “5. Aharonov–Bohm Phase and Flux Period”A charged particle with charge winds once counterclockwise around an inaccessible magnetic flux . Find the Aharonov–Bohm phase. Then specialize to an electron with and identify the flux period.
Solution
For one winding with the chosen orientation,
Thus
For an electron, , so
Using
this becomes
The phase factor is periodic under
The sign depends on charge and loop orientation. The periodicity does not.
6. Flat Locally, Nontrivial Globally
Section titled “6. Flat Locally, Nontrivial Globally”Outside an ideal thin flux tube, take
on the punctured plane . Show that the field is zero locally outside the tube but that a circle around the origin has nonzero holonomy.
Solution
For , this vector potential has zero curl:
The magnetic field is confined to the excluded flux tube. The accessible region is not simply connected, so zero local curl does not force every loop integral to vanish.
For a counterclockwise circle of radius ,
Therefore
For winding number ,
The Aharonov–Bohm phase is therefore sensitive to winding around the excluded region even though the local magnetic field vanishes along the path.
7. Chern Number of the Spin Sphere
Section titled “7. Chern Number of the Spin Sphere”For the lower spin state in the convention above,
Compute the Chern number over the full parameter sphere with the standard orientation.
Solution
Integrate over the full sphere:
The Chern number is
The opposite eigenstate has the opposite Chern number in the matching convention. Reversing the orientation of the sphere also reverses the sign.
8. Toy Monopole Charge
Section titled “8. Toy Monopole Charge”Suppose a line bundle over a parameter sphere has curvature
where is an integer. Compute its Chern number. Why should an arbitrary real coefficient not be accepted as a globally valid quantum line bundle without further checks?
Solution
The curvature flux is
Therefore
The integrality is not a decorative convention. For a globally well-defined quantum line bundle over a closed surface, transition functions between patches must be single-valued, and their winding numbers are integers. A random real coefficient would give a noninteger normalized flux, signaling that the assumed curvature cannot be the curvature of an ordinary globally defined eigenstate line bundle over the closed sphere without changing the setup.
9. Can the Chern Number Change Smoothly?
Section titled “9. Can the Chern Number Change Smoothly?”A Hamiltonian family over a closed two-dimensional parameter space has an isolated nondegenerate band with Chern number . The Hamiltonian is smoothly deformed. Under what condition must the Chern number remain fixed, and what must happen for it to change?
Solution
The Chern number is integer-valued and stable under smooth deformations as long as the relevant eigenstate or band remains isolated over the entire parameter space. In band language, the spectral gap separating the band or occupied subspace from the rest of the spectrum must stay open everywhere.
If the gap never closes, cannot drift continuously from to another integer. A change requires a singular event for the bundle being tracked, typically a degeneracy or gap closing:
at some parameter value. At that point the isolated-band Berry curvature for that band is not defined, and after the gap reopens curvature flux can be redistributed between bands.
Common Mistakes
Section titled “Common Mistakes”- Calling the dynamical phase part of the Berry phase.
- Treating the Berry connection as gauge invariant instead of its closed-loop holonomy or curvature.
- Forgetting that spin- solid-angle signs depend on the Hamiltonian and eigenstate convention.
- Applying Stokes’ theorem across a surface where no smooth gauge exists without patching.
- Confusing Aharonov–Bohm holonomy in real configuration space with Berry phase in Hamiltonian parameter space.
- Calling any curvature integral a Chern number without checking that the parameter space is closed and the eigenstate remains isolated.
- Assuming a Chern number can change without a gap closing or other singular loss of the isolated bundle.
References
Section titled “References”- M. V. Berry, “Quantal phase factors accompanying adiabatic changes,” Proceedings of the Royal Society A 392, 45–57, 1984.
- B. Simon, “Holonomy, the quantum adiabatic theorem, and Berry’s phase,” Physical Review Letters 51, 2167–2170, 1983.
- Y. Aharonov and D. Bohm, “Significance of electromagnetic potentials in quantum theory,” Physical Review 115, 485–491, 1959.
- A. Shapere and F. Wilczek, eds., Geometric Phases in Physics, World Scientific, 1989.
- D. Xiao, M.-C. Chang, and Q. Niu, “Berry phase effects on electronic properties,” Reviews of Modern Physics 82, 1959–2007, 2010.
- J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.