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Magnetic translations move the guiding center of a charged particle in a uniform magnetic field without changing its cyclotron energy. They combine a spatial shift with a phase. We first consider a spinless particle of nonzero charge on the entire plane, with no electric potential or confining boundary; either can break the translation symmetry.

The surprise is that magnetic translations generally do not commute. Moving by a\mathbf a and then by b\mathbf b differs from moving by b\mathbf b and then by a\mathbf a by a phase proportional to the magnetic flux through the parallelogram spanned by a\mathbf a and b\mathbf b.

That noncommuting translation algebra is a compact symmetry explanation of Landau-level degeneracy, magnetic flux quantization on a torus, and the magnetic-unit-cell structure behind lattice quantum Hall models.

For a free particle, ordinary translations are generated by canonical momentum:

T(a)=exp⁡(−iℏa⋅p).T(\mathbf a) = \exp\left( -\frac{i}{\hbar}\mathbf a\cdot\mathbf p \right).

They act on a wavefunction as

(T(a)ψ)(r)=ψ(r−a).(T(\mathbf a)\psi)(\mathbf r) = \psi(\mathbf r-\mathbf a).

In a vector potential, the Hamiltonian is

H=12m(p−qA(r))2.H = \frac{1}{2m} \left( \mathbf p-q\mathbf A(\mathbf r) \right)^2.

If A\mathbf A changes under a spatial shift, the ordinary translation operator need not commute with this particular gauge-fixed Hamiltonian even when the magnetic field itself is uniform. The physical field may be translation invariant while the chosen vector potential is not.

Magnetic translations repair this mismatch. They translate the wavefunction and include the phase needed to compare the vector potential at neighboring points.

Now take a two-dimensional particle in a uniform field

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

with Hamiltonian

H=π22m,π=p−qA.H = \frac{\boldsymbol\pi^2}{2m}, \qquad \boldsymbol\pi = \mathbf p-q\mathbf A.

The kinetic momenta obey

[πx,πy]=iℏqB.[\pi_x,\pi_y] = i\hbar qB.

Kinetic momentum is not conserved: the Lorentz force rotates it during cyclotron motion. Instead, use the guiding-center coordinates

X=x+πyqB,Y=y−πxqB.X = x+\frac{\pi_y}{qB}, \qquad Y = y-\frac{\pi_x}{qB}.

They commute with the Hamiltonian:

[X,H]=[Y,H]=0,[X,H]=[Y,H]=0,

but not with each other:

[X,Y]=−iℏqB.[X,Y] = -\frac{i\hbar}{qB}.

The noncommutativity of magnetic translations is the finite version of this guiding-center commutator.

With the conventions above, define the magnetic translation by

TB(a)=exp⁡[iℏqB(axY−ayX)].\mathsf T_B(\mathbf a) = \exp\left[ \frac{i}{\hbar} qB(a_xY-a_yX) \right].

It shifts the guiding center:

TB(a)†XTB(a)=X+ax,\mathsf T_B(\mathbf a)^\dagger X \mathsf T_B(\mathbf a) = X+a_x,

and

TB(a)†YTB(a)=Y+ay.\mathsf T_B(\mathbf a)^\dagger Y \mathsf T_B(\mathbf a) = Y+a_y.

Because XX and YY commute with HH, the magnetic translation also commutes with the uniform-field Hamiltonian:

[TB(a),H]=0.[\mathsf T_B(\mathbf a),H]=0.

This is the symmetry statement behind the fact that shifting a cyclotron orbit’s guiding center costs no energy in the ideal Landau problem.

Define the conserved momentum-like generator

K=(−qBY,qBX)=π+qB×r,TB(a)=e−ia⋅K/ℏ.\mathbf K=(-qBY,qBX) =\boldsymbol\pi+q\mathbf B\times\mathbf r, \qquad \mathsf T_B(\mathbf a)=e^{-i\mathbf a\cdot\mathbf K/\hbar}.

Its commutators are [Ki,πj]=0[K_i,\pi_j]=0 and [Kx,Ky]=−iℏqB[K_x,K_y]=-i\hbar qB. In symmetric gauge, A=12B×r\mathbf A=\tfrac12\mathbf B\times\mathbf r, we have K=p+qA\mathbf K=\mathbf p+q\mathbf A. The translation acts as

(TB(a)ψ)(r)=exp⁡ ⁣[iqB2ℏ(axy−ayx)]ψ(r−a).(\mathsf T_B(\mathbf a)\psi)(\mathbf r) =\exp\!\left[\frac{iqB}{2\hbar}(a_xy-a_yx)\right] \psi(\mathbf r-\mathbf a).

The phase gradient compensates the change in A\mathbf A under the shift, so πTB=TBπ\boldsymbol\pi\mathsf T_B=\mathsf T_B\boldsymbol\pi and consequently [H,TB]=0[H,\mathsf T_B]=0.

In another gauge, A′=A+∇χ\mathbf A'=\mathbf A+\nabla\chi, use

TB′(a)=UχTB(a)Uχ†,Uχ=eiqχ/ℏ.\mathsf T'_B(\mathbf a)=U_\chi\mathsf T_B(\mathbf a)U_\chi^\dagger, \qquad U_\chi=e^{iq\chi/\hbar}.

The coordinate-space phase gains q[χ(r)−χ(r−a)]/ℏq[\chi(\mathbf r)-\chi(\mathbf r-\mathbf a)]/\hbar. Thus the symmetry has a gauge-covariant description.

Parallel transport is a different operation

Section titled “Parallel transport is a different operation”

A straight Wilson-line transport is

(W(a)ψ)(r)=exp⁡ ⁣[iqℏ∫r−arA⋅dℓ]ψ(r−a).(W(\mathbf a)\psi)(\mathbf r) =\exp\!\left[\frac{iq}{\hbar} \int_{\mathbf r-\mathbf a}^{\mathbf r}\mathbf A\cdot d\boldsymbol\ell\right] \psi(\mathbf r-\mathbf a).

This also transforms covariantly, but covariance alone does not imply a symmetry. In symmetric gauge its phase is −qB(axy−ayx)/(2ℏ)-qB(a_xy-a_yx)/(2\hbar), the opposite of the magnetic-translation phase above. Its infinitesimal generator is π\boldsymbol\pi, which does not commute with HH. Use WW to compare phases along a path and TB\mathsf T_B to translate a Landau orbit without changing its energy.

Let

A(a,b)=axby−aybxA(\mathbf a,\mathbf b) = a_xb_y-a_yb_x

be the signed area of the parallelogram spanned by a\mathbf a and b\mathbf b. Since [X,Y][X,Y] is central, the Baker-Campbell-Hausdorff formula gives

TB(a)TB(b)=exp⁡[iqB2ℏA(a,b)]TB(a+b).\mathsf T_B(\mathbf a) \mathsf T_B(\mathbf b) = \exp\left[ \frac{iqB}{2\hbar} A(\mathbf a,\mathbf b) \right] \mathsf T_B(\mathbf a+\mathbf b).

Swapping the two translations gives the opposite half-phase, so

TB(a)TB(b)=exp⁡[iqBℏA(a,b)]TB(b)TB(a).\mathsf T_B(\mathbf a) \mathsf T_B(\mathbf b) = \exp\left[ \frac{iqB}{\hbar} A(\mathbf a,\mathbf b) \right] \mathsf T_B(\mathbf b) \mathsf T_B(\mathbf a).

Thus magnetic translations commute only when

exp⁡[iqBℏA(a,b)]=1.\exp\left[ \frac{iqB}{\hbar} A(\mathbf a,\mathbf b) \right] = 1.

The exponent is the Aharonov–Bohm phase for the magnetic flux through the parallelogram:

qℏΦa,b,Φa,b=B A(a,b).\frac{q}{\hbar} \Phi_{\mathbf a,\mathbf b}, \qquad \Phi_{\mathbf a,\mathbf b} = B\,A(\mathbf a,\mathbf b).

The algebra is a projective representation of the ordinary translation group. The projective phase is not an arbitrary convention; it is magnetic flux.

The algebraic group commutator follows directly from the multiplication law:

TB(a)TB(b)TB(−a)TB(−b)=eiqBA(a,b)/ℏI.\mathsf T_B(\mathbf a)\mathsf T_B(\mathbf b) \mathsf T_B(-\mathbf a)\mathsf T_B(-\mathbf b) =e^{iqB A(\mathbf a,\mathbf b)/\hbar}I.

Operators act from right to left. Chronologically moving by a\mathbf a, then b\mathbf b, then −a-\mathbf a, then −b-\mathbf b instead gives

TB(−b)TB(−a)TB(b)TB(a)=e−iqBA(a,b)/ℏI.\mathsf T_B(-\mathbf b)\mathsf T_B(-\mathbf a) \mathsf T_B(\mathbf b)\mathsf T_B(\mathbf a) =e^{-iqB A(\mathbf a,\mathbf b)/\hbar}I.

Both formulas express the same noncommuting symmetry algebra. A Wilson transport around the geometrical loop has phase e+iqΦ/ℏe^{+iq\Phi/\hbar} with its chosen path orientation; it is a different operation. Keeping the operator order and the transport definition explicit avoids assigning the wrong sign by an appeal to flux alone.

The Landau Hamiltonian depends only on the kinetic momenta:

H=12m(πx2+πy2).H = \frac{1}{2m} \left( \pi_x^2+\pi_y^2 \right).

The kinetic momenta create the cyclotron oscillator and determine the Landau-level energy. The guiding-center coordinates commute with that energy and label the degeneracy inside each Landau level.

Because

[X,Y]=−i sgn⁡(qB)ℓB2,ℓB=ℏ∣q∣B,[X,Y] = -i\,\operatorname{sgn}(qB)\ell_B^2, \qquad \ell_B = \sqrt{ \frac{\hbar}{\lvert q\rvert B} },

the guiding-center plane is itself a noncommutative phase plane. A region of area AA supports roughly one independent guiding-center state per area 2πℓB22\pi\ell_B^2:

NΦ≈A2πℓB2=∣q∣BAh.N_\Phi \approx \frac{A}{2\pi\ell_B^2} = \frac{\lvert q\rvert BA}{h}.

This is the degeneracy count derived in wave-mechanics language in Degeneracy of Landau Levels. Magnetic translations explain why the degeneracy is a symmetry structure, not an accidental feature of Landau gauge.

On a torus, translations around two fundamental cycles must be globally consistent. If the torus has side vectors L1\mathbf L_1 and L2\mathbf L_2, the two large magnetic translations obey

TB(L1)TB(L2)=exp⁡[iqΦtotℏ]TB(L2)TB(L1),\mathsf T_B(\mathbf L_1) \mathsf T_B(\mathbf L_2) = \exp\left[ \frac{iq\Phi_{\mathrm{tot}}}{\hbar} \right] \mathsf T_B(\mathbf L_2) \mathsf T_B(\mathbf L_1),

where

Φtot=B A(L1,L2).\Phi_{\mathrm{tot}} = B\,A(\mathbf L_1,\mathbf L_2).

Nonzero flux requires gauge-compatible boundary conditions, rather than one globally periodic vector potential and scalar wavefunction. Write the two boundary identifications as TB(Li)ψ=eiθiψ\mathsf T_B(\mathbf L_i)\psi=e^{i\theta_i}\psi. Applying them in either order must agree, so the phase must be unity:

qΦtotℏ=2πN,N∈Z.\frac{q\Phi_{\mathrm{tot}}}{\hbar} = 2\pi N, \qquad N\in\mathbb Z.

Equivalently,

Φtot=Nhq\Phi_{\mathrm{tot}} = N\frac{h}{q}

with orientation included in the sign of qΦtotq\Phi_{\mathrm{tot}}. In magnitude, the condition is an integer number of single-particle flux quanta:

∣qΦtot∣h∈Z.\frac{\lvert q\Phi_{\mathrm{tot}}\rvert}{h} \in \mathbb Z.

For nonzero flux, each ideal Landau level on the torus then has exactly ∣N∣|N| orbital states. A finite sample with edges instead has only an approximate bulk count; edge energies can disperse.

On a lattice with primitive vectors a1,a2\mathbf a_1,\mathbf a_2, magnetic translations along the two lattice directions commute only if the flux through the primitive cell is an integer multiple of the flux quantum:

exp⁡[iqΦcellℏ]=1.\exp\left[ \frac{iq\Phi_{\mathrm{cell}}}{\hbar} \right] = 1.

If the flux per cell is rational in flux-quantum units,

ΦcellΦ0=pQ,Φ0=h∣q∣,\frac{\Phi_{\mathrm{cell}}}{\Phi_0} = \frac{p}{Q}, \qquad \Phi_0=\frac{h}{\lvert q\rvert},

with pp and QQ coprime, then an enlarged magnetic unit cell with QQ ordinary cells can restore commuting magnetic translations. This assumes the scalar lattice potential also respects the corresponding Bravais translations. This is the symmetry reason behind magnetic Bloch bands and the Hofstadter spectrum. The Peierls phase realizes this algebra in a lattice hopping model.

  • Saying a uniform magnetic field destroys translation symmetry. It destroys ordinary gauge-fixed translation symmetry, but magnetic translations remain.
  • Using canonical momentum translations in a magnetic field and expecting them to commute with the Hamiltonian in every gauge.
  • Forgetting that magnetic translations commute only up to a flux phase.
  • Treating kyk_y in Landau gauge as a universal physical momentum rather than one gauge-dependent way to label guiding centers.
  • Ignoring flux quantization when imposing periodic boundary conditions in both directions.
  • Losing the charge sign in the algebra. Many formulas change phase orientation when qq or BB is reversed.
  1. Derive the magnetic-translation commutator.

Using

[X,Y]=−iℏqB,[X,Y]=-\frac{i\hbar}{qB},

and

TB(a)=exp⁡[iℏqB(axY−ayX)],\mathsf T_B(\mathbf a) = \exp\left[ \frac{i}{\hbar} qB(a_xY-a_yX) \right],

show that

TB(a)TB(b)=exp⁡[iqBℏA(a,b)]TB(b)TB(a).\mathsf T_B(\mathbf a) \mathsf T_B(\mathbf b) = \exp\left[ \frac{iqB}{\hbar} A(\mathbf a,\mathbf b) \right] \mathsf T_B(\mathbf b) \mathsf T_B(\mathbf a).
Solution

Let

G(a)=qB(axY−ayX).G(\mathbf a) = qB(a_xY-a_yX).

Then

[G(a),G(b)]=−iℏqB(axby−aybx).[G(\mathbf a),G(\mathbf b)] = -i\hbar qB \left( a_xb_y-a_yb_x \right).

Because this commutator is a scalar, Baker-Campbell-Hausdorff gives

TB(a)TB(b)=exp⁡[iqB2ℏA(a,b)]TB(a+b).\mathsf T_B(\mathbf a)\mathsf T_B(\mathbf b) = \exp\left[ \frac{iqB}{2\hbar}A(\mathbf a,\mathbf b) \right] \mathsf T_B(\mathbf a+\mathbf b).

Swapping a\mathbf a and b\mathbf b flips the sign of AA. Taking the ratio gives

TB(a)TB(b)=exp⁡[iqBℏA(a,b)]TB(b)TB(a).\mathsf T_B(\mathbf a) \mathsf T_B(\mathbf b) = \exp\left[ \frac{iqB}{\hbar} A(\mathbf a,\mathbf b) \right] \mathsf T_B(\mathbf b) \mathsf T_B(\mathbf a).
  1. Find when two magnetic lattice translations commute.

Let the flux through a lattice unit cell be Φcell\Phi_{\mathrm{cell}}. What condition makes magnetic translations along the two primitive lattice vectors commute?

Solution

They commute when the flux phase is unity:

exp⁡(iqΦcellℏ)=1.\exp\left( \frac{iq\Phi_{\mathrm{cell}}}{\hbar} \right) = 1.

Therefore

qΦcellℏ=2πn,n∈Z.\frac{q\Phi_{\mathrm{cell}}}{\hbar} = 2\pi n, \qquad n\in\mathbb Z.

Equivalently,

∣qΦcell∣h∈Z.\frac{\lvert q\Phi_{\mathrm{cell}}\rvert}{h} \in \mathbb Z.
  1. Connect the algebra to Landau degeneracy.

Use the guiding-center commutator to explain why an area AA supports roughly A/(2πℓB2)A/(2\pi\ell_B^2) states in one Landau level.

Solution

The guiding-center coordinates obey

[X,Y]=−i sgn⁡(qB)ℓB2.[X,Y] = -i\,\operatorname{sgn}(qB)\ell_B^2.

This is analogous to a canonical phase plane with effective Planck area 2πℓB22\pi\ell_B^2. Therefore a region of ordinary area AA contains roughly

NΦ=A2πℓB2N_\Phi = \frac{A}{2\pi\ell_B^2}

independent guiding-center states. Since the Landau Hamiltonian depends on the cyclotron variables rather than on X,YX,Y, these states have the same Landau-level energy in the ideal problem.

  1. Show why gauge covariance does not by itself guarantee a translation symmetry. Compute [πx,H][\pi_x,H] and [πy,H][\pi_y,H], then compare them with the conserved generators Kx=πx−qByK_x=\pi_x-qBy and Ky=πy+qBxK_y=\pi_y+qBx.
Solution

Using [πx,πy]=iℏqB[\pi_x,\pi_y]=i\hbar qB,

[πx,H]=iℏqBmπy,[πy,H]=−iℏqBmπx.[\pi_x,H]=\frac{i\hbar qB}{m}\pi_y, \qquad [\pi_y,H]=-\frac{i\hbar qB}{m}\pi_x.

Also [y,H]=iℏπy/m[y,H]=i\hbar\pi_y/m and [x,H]=iℏπx/m[x,H]=i\hbar\pi_x/m. Hence the two terms in [Kx,H][K_x,H] cancel, as do those in [Ky,H][K_y,H].

The straight Wilson-line shift has infinitesimal generator π\boldsymbol\pi and therefore is not a symmetry of this Hamiltonian. The magnetic translation generated by K\mathbf K is. Both operations have a consistent transformation law under a change of gauge.

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  • D. R. Hofstadter, “Energy levels and wave functions of Bloch electrons in rational and irrational magnetic fields,” Physical Review B 14, 2239–2249, 1976.
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