Skip to content

Particle in a Uniform Magnetic Field

A uniform magnetic field is the simplest setting where the difference between canonical momentum and kinetic momentum becomes visible. A charged particle is free along the field direction, but its transverse motion is curved by the Lorentz force. Quantum mechanically, that transverse motion becomes oscillator-like.

This page sets up the Landau-level problem physically. The canonical derivation of the energy spectrum, wavefunctions, guiding-center degeneracy, and flux counting belongs to Landau Levels. The goal here is to understand why that later problem is secretly an oscillator problem and why gauge-dependent labels must be handled carefully.

We consider a spinless nonrelativistic particle of mass mm and charge qq in the prescribed field

B=Bz^,B>0,\mathbf B = B\hat{\mathbf z}, \qquad B\gt0,

with scalar potential set to zero. Spin magnetic moments, Zeeman splitting, radiation, disorder, interactions, and boundaries are not part of this ideal setup.

Classically, the Lorentz force is

mv˙=qv×B.m\dot{\mathbf v} = q\mathbf v\times\mathbf B .

The velocity component parallel to B\mathbf B is unchanged, while the transverse velocity rotates. The positive cyclotron frequency is

ωc=∣q∣Bm.\omega_c = \frac{\lvert q\rvert B}{m}.

The sign of qBqB determines the direction of rotation in the transverse plane. The magnitude ωc\omega_c determines the time scale. For transverse speed v⊥v_\perp, the classical cyclotron radius is

rc=v⊥ωc=mv⊥∣q∣B.r_c = \frac{v_\perp}{\omega_c} = \frac{m v_\perp}{\lvert q\rvert B}.

This is the classical seed of the quantum problem: magnetic fields do not create a scalar potential well, but they do bind the transverse kinetic motion into circular orbits.

Uniform magnetic field giving cyclotron motion and a Landau-gauge oscillator center

A uniform field separates the physics into cyclotron motion and a guiding-center label. In Landau gauge, fixing kyk_y turns the transverse Hamiltonian into an oscillator centered at x0=ℏky/(qB)x_0=\hbar k_y/(qB).

Minimal coupling replaces canonical momentum by kinetic momentum:

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

With Φ=0\Phi=0, the Hamiltonian is

H^=π^ 22m=12m(p^−qA)2.\hat H = \frac{\hat{\boldsymbol\pi}^{\,2}}{2m} = \frac{1}{2m} \left( \hat{\mathbf p}-q\mathbf A \right)^2 .

The vector potential is not unique. Two standard choices for B=Bz^\mathbf B=B\hat{\mathbf z} are:

AL=Bx y^Landau gauge,\mathbf A_L = Bx\,\hat{\mathbf y} \qquad \text{Landau gauge},

and

AS=12B×r=B2(−y x^+x y^)symmetric gauge.\mathbf A_S = \frac12\mathbf B\times\mathbf r = \frac{B}{2} \left( -y\,\hat{\mathbf x} + x\,\hat{\mathbf y} \right) \qquad \text{symmetric gauge}.

Both satisfy

∇×A=Bz^.\nabla\times\mathbf A = B\hat{\mathbf z}.

The two gauges make different symmetries convenient. Landau gauge keeps translation invariance along one transverse direction. Symmetric gauge keeps rotation symmetry around the zz axis. Gauge transformations explain why these different-looking descriptions represent the same physical magnetic field.

The transverse kinetic momenta are

π^x=p^x−qAx,π^y=p^y−qAy.\hat\pi_x = \hat p_x-qA_x, \qquad \hat\pi_y = \hat p_y-qA_y.

For a uniform field,

[π^x,π^y]=iℏqB.[\hat\pi_x,\hat\pi_y] = i\hbar qB .

This is the algebraic reason a magnetic field changes the spectrum. Free-particle momenta commute; transverse kinetic momenta in a magnetic field do not. Their noncommutativity is proportional to the magnetic field itself.

The transverse Hamiltonian is

H^⊥=12m(π^x2+π^y2).\hat H_\perp = \frac{1}{2m} \left( \hat\pi_x^2+\hat\pi_y^2 \right).

Introduce the magnetic length

ℓB=ℏ∣q∣B\ell_B = \sqrt{ \frac{\hbar}{\lvert q\rvert B} }

and the sign

s=sgn⁡(qB).s = \operatorname{sgn}(qB).

Then the operator

a^=ℓB2 ℏ(π^x+isπ^y)\hat a = \frac{\ell_B}{\sqrt2\,\hbar} \left( \hat\pi_x+i s\hat\pi_y \right)

satisfies

[a^,a^†]=1.[\hat a,\hat a^\dagger]=1.

Moreover,

H^⊥=ℏωc(a^†a^+12).\hat H_\perp = \hbar\omega_c \left( \hat a^\dagger\hat a+\frac12 \right).

This is the central setup result: the transverse kinetic motion has the same algebra as a one-dimensional harmonic oscillator. The magnetic field creates the oscillator algebra without introducing an ordinary position-dependent potential.

In Landau gauge,

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

the two-dimensional transverse Hamiltonian becomes

H^⊥=12m[p^x2+(p^y−qBx)2].\hat H_\perp = \frac{1}{2m} \left[ \hat p_x^2 + \left( \hat p_y-qBx \right)^2 \right].

This Hamiltonian has no explicit yy dependence, so p^y\hat p_y commutes with H^⊥\hat H_\perp. If

ψ(x,y)=eikyyφ(x),\psi(x,y) = e^{ik_y y}\varphi(x),

then p^y\hat p_y acts as multiplication by ℏky\hbar k_y, and the xx equation contains

(ℏky−qBx)2=(qB)2(x−ℏkyqB)2.\left( \hbar k_y-qBx \right)^2 = (qB)^2 \left( x-\frac{\hbar k_y}{qB} \right)^2 .

Thus each value of kyk_y gives a harmonic oscillator in xx, centered at

x0=ℏkyqB.x_0 = \frac{\hbar k_y}{qB}.

The sign of x0x_0 depends on the charge convention, but the oscillator frequency is the positive quantity ωc=∣q∣B/m\omega_c=\lvert q\rvert B/m.

This derivation also hints at degeneracy: changing kyk_y shifts the oscillator center without changing the oscillator frequency. The full counting of allowed centers is part of Landau Levels.

In symmetric gauge,

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

the Hamiltonian does not single out the xx or yy direction. Instead, rotations about z^\hat{\mathbf z} are natural. This gauge is useful when angular momentum, circular orbits, or disk geometry matters.

The symmetric-gauge wavefunctions look different from the Landau-gauge wavefunctions. Their labels also look different. This is not a physical disagreement. Gauge-invariant quantities, such as the magnetic field, energy spectrum, local density after a complete degenerate subspace is handled consistently, and physical currents, agree.

For a particle in three dimensions, the uniform magnetic field affects the transverse motion but leaves the longitudinal kinetic energy free:

H^=H^⊥+p^z22m.\hat H = \hat H_\perp + \frac{\hat p_z^2}{2m}.

This separation is important. Landau quantization is not ordinary confinement in all directions. In the ideal infinite three-dimensional problem, the transverse energy is quantized while the zz direction remains continuous. Extra potentials, boundaries, lattice structure, or finite-size conditions can change that statement.

The magnetic length

ℓB=ℏ∣q∣B\ell_B = \sqrt{ \frac{\hbar}{\lvert q\rvert B} }

is the natural transverse quantum length scale. Stronger magnetic fields make ℓB\ell_B smaller and the cyclotron spacing larger:

ℏωc=ℏ∣q∣Bm.\hbar\omega_c = \frac{\hbar\lvert q\rvert B}{m}.

The area scale

2πℓB2=h∣q∣B2\pi\ell_B^2 = \frac{h}{\lvert q\rvert B}

is tied to one flux quantum through the plane. This is why the later degeneracy count can be expressed as flux through the sample divided by a flux quantum. This page only identifies the scale; the finite-area state counting is the responsibility of the Landau-level degeneracy discussion.

The useful mental split is:

  • kinetic cyclotron motion, which is oscillator-like and carries the energy;
  • guiding-center information, which labels where the orbit is centered and accounts for degeneracy in an extended system;
  • free longitudinal motion, if the particle is allowed to move along B\mathbf B.

In Landau gauge, the guiding-center information appears through kyk_y and x0x_0. In symmetric gauge, it appears through angular structure. Neither label should be mistaken for a universal gauge-invariant observable. The physical statements are the magnetic field, the kinetic energy scale, the magnetic length, and gauge-invariant currents or densities.

  • Treating p^\hat{\mathbf p} as the mechanical momentum after a vector potential is introduced.
  • Forgetting that ωc\omega_c is positive even when qq is negative.
  • Thinking the magnetic field creates an ordinary scalar potential well in the transverse plane.
  • Comparing Landau-gauge and symmetric-gauge wavefunctions without applying the appropriate gauge transformation.
  • Treating kyk_y in Landau gauge as a universal physical momentum rather than a convenient gauge-dependent label.
  • Forgetting that a three-dimensional uniform-field problem remains free along the field direction.
  • Including electron spin effects in the spinless Landau setup without saying so.
  1. Verify that the Landau and symmetric gauges both produce B=Bz^\mathbf B=B\hat{\mathbf z}.
Solution

For Landau gauge,

Ax=0,Ay=Bx,Az=0.A_x=0, \qquad A_y=Bx, \qquad A_z=0.

Thus

(∇×AL)z=∂Ay∂x−∂Ax∂y=B,(\nabla\times\mathbf A_L)_z = \frac{\partial A_y}{\partial x} - \frac{\partial A_x}{\partial y} = B,

and the other components vanish.

For symmetric gauge,

Ax=−B2y,Ay=B2x,Az=0.A_x=-\frac{B}{2}y, \qquad A_y=\frac{B}{2}x, \qquad A_z=0.

Then

(∇×AS)z=∂Ay∂x−∂Ax∂y=B2−(−B2)=B,(\nabla\times\mathbf A_S)_z = \frac{\partial A_y}{\partial x} - \frac{\partial A_x}{\partial y} = \frac{B}{2} - \left( -\frac{B}{2} \right) = B,

with zero xx and yy components.

  1. Derive the commutator [π^x,π^y]=iℏqB[\hat\pi_x,\hat\pi_y]=i\hbar qB in Landau gauge.
Solution

In Landau gauge,

π^x=p^x,π^y=p^y−qBx.\hat\pi_x=\hat p_x, \qquad \hat\pi_y=\hat p_y-qBx.

Therefore

[π^x,π^y]=[p^x,p^y]−qB[p^x,x].[\hat\pi_x,\hat\pi_y] = [\hat p_x,\hat p_y] - qB[\hat p_x,x].

The first commutator vanishes and

[p^x,x]=−iℏ.[\hat p_x,x] = -i\hbar.

Hence

[π^x,π^y]=iℏqB.[\hat\pi_x,\hat\pi_y] = i\hbar qB.
  1. Show that the transverse kinetic Hamiltonian has oscillator form.
Solution

Let

a^=ℓB2 ℏ(π^x+isπ^y),s=sgn⁡(qB).\hat a = \frac{\ell_B}{\sqrt2\,\hbar} \left( \hat\pi_x+i s\hat\pi_y \right), \qquad s=\operatorname{sgn}(qB).

Using

[π^x,π^y]=isℏ2ℓB2,[\hat\pi_x,\hat\pi_y] = i s\frac{\hbar^2}{\ell_B^2},

one finds

[a^,a^†]=1.[\hat a,\hat a^\dagger]=1.

Also,

a^†a^=ℓB22ℏ2(π^x2+π^y2−ℏ2ℓB2).\hat a^\dagger\hat a = \frac{\ell_B^2}{2\hbar^2} \left( \hat\pi_x^2+\hat\pi_y^2 - \frac{\hbar^2}{\ell_B^2} \right).

Solving for π^x2+π^y2\hat\pi_x^2+\hat\pi_y^2 gives

π^x2+π^y22m=ℏ2mℓB2(a^†a^+12).\frac{\hat\pi_x^2+\hat\pi_y^2}{2m} = \frac{\hbar^2}{m\ell_B^2} \left( \hat a^\dagger\hat a+\frac12 \right).

Since

ℏ2mℓB2=ℏωc,\frac{\hbar^2}{m\ell_B^2} = \hbar\omega_c,

the transverse Hamiltonian is

H^⊥=ℏωc(a^†a^+12).\hat H_\perp = \hbar\omega_c \left( \hat a^\dagger\hat a+\frac12 \right).
  1. In Landau gauge, explain why changing kyk_y shifts the oscillator center but not the oscillator frequency.
Solution

With ψ=eikyyφ(x)\psi=e^{ik_y y}\varphi(x),

(p^y−qBx)2→(ℏky−qBx)2.\left( \hat p_y-qBx \right)^2 \to \left( \hbar k_y-qBx \right)^2.

Completing the square gives

(ℏky−qBx)2=(qB)2(x−ℏkyqB)2.\left( \hbar k_y-qBx \right)^2 = (qB)^2 \left( x-\frac{\hbar k_y}{qB} \right)^2 .

The center is

x0=ℏkyqB,x_0 = \frac{\hbar k_y}{qB},

so changing kyk_y changes the center. The quadratic coefficient is (qB)2/(2m)(qB)^2/(2m), which corresponds to the same positive frequency ωc=∣q∣B/m\omega_c=\lvert q\rvert B/m for every kyk_y.

  • 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.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • R. E. Prange and S. M. Girvin, eds., The Quantum Hall Effect, 2nd ed., Springer, 1990.