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Central Potentials and Rotational Symmetry

A central potential is a scalar potential that depends only on distance from one fixed origin,

V(r)=V(r),r=∣r∣.V(\mathbf r)=V(r), \qquad r=\lvert\mathbf r\rvert.

For a spinless particle with Hamiltonian

H=P22m+V(r),H=\frac{\mathbf P^2}{2m}+V(r),

this is not merely a convenient coordinate choice. It is a symmetry statement: rotations leave the Hamiltonian invariant. The consequence is that energy eigenstates can be organized by orbital angular momentum,

L2ψ=ℏ2ℓ(ℓ+1)ψ,Lzψ=ℏmψ,L^2\psi=\hbar^2\ell(\ell+1)\psi, \qquad L_z\psi=\hbar m\psi,

with

ℓ=0,1,2,…,m=−ℓ,−ℓ+1,…,ℓ.\ell=0,1,2,\ldots, \qquad m=-\ell,-\ell+1,\ldots,\ell.

This page explains the symmetry engine behind central-potential problems. The explicit radial equation, boundary conditions, and model-specific spectra live in Central Potentials and the Radial Schrödinger Equation.

The symmetry content of a central potential is:

  • rotations are generated by orbital angular momentum L\mathbf L;
  • the Hamiltonian commutes with every component LiL_i;
  • HH, L2L^2, and one chosen component such as LzL_z may be diagonalized together;
  • the angular dependence is described by spherical harmonics;
  • the magnetic quantum number mm labels a rotational multiplet, not a different radial problem.

The dynamical content is separate. The functional form of V(r)V(r) determines whether the spectrum has bound states, continuum states, special accidental degeneracies, or no bound states at all.

Let

L=R×P\mathbf L=\mathbf R\times\mathbf P

be orbital angular momentum. Its components rotate position and momentum as vectors:

[Li,Rj]=iℏ∑kϵijkRk,[L_i,R_j] = i\hbar\sum_k\epsilon_{ijk}R_k,

and

[Li,Pj]=iℏ∑kϵijkPk.[L_i,P_j] = i\hbar\sum_k\epsilon_{ijk}P_k.

Therefore scalar combinations built from dot products are rotationally invariant. In particular,

[Li,R2]=0,[Li,P2]=0.[L_i,\mathbf R^2]=0, \qquad [L_i,\mathbf P^2]=0.

Since r=(R2)1/2r=(\mathbf R^2)^{1/2}, a sufficiently well-defined function of rr also commutes with L\mathbf L:

[Li,V(r)]=0.[L_i,V(r)]=0.

For the central-potential Hamiltonian,

H=P22m+V(r),H=\frac{\mathbf P^2}{2m}+V(r),

one obtains

[H,Li]=0,i=x,y,z.[H,L_i]=0, \qquad i=x,y,z.

Equivalently, if

U(R)=exp⁡(−iℏθ⋅L)U(\mathcal R) = \exp\left( -\frac{i}{\hbar}\boldsymbol\theta\cdot\mathbf L \right)

is the unitary implementing a spatial rotation R\mathcal R, then

U(R)HU(R)†=H.U(\mathcal R)HU(\mathcal R)^\dagger=H.

The infinitesimal commutator and the finite rotation statement are the same symmetry expressed in two languages.

Because every LiL_i commutes with HH, the Casimir L2L^2 also commutes with HH:

[H,L2]=0.[H,L^2]=0.

Since

[L2,Lz]=0,[L^2,L_z]=0,

we may choose stationary states that are simultaneous eigenstates of HH, L2L^2, and LzL_z:

H∣α,ℓ,m⟩=Eαℓ∣α,ℓ,m⟩,L2∣α,ℓ,m⟩=ℏ2ℓ(ℓ+1)∣α,ℓ,m⟩,Lz∣α,ℓ,m⟩=ℏm∣α,ℓ,m⟩.\begin{aligned} H|\alpha,\ell,m\rangle &= E_{\alpha\ell}|\alpha,\ell,m\rangle, \\ L^2|\alpha,\ell,m\rangle &= \hbar^2\ell(\ell+1)|\alpha,\ell,m\rangle, \\ L_z|\alpha,\ell,m\rangle &= \hbar m|\alpha,\ell,m\rangle. \end{aligned}

The label α\alpha denotes whatever additional information is needed to distinguish states with the same angular labels. For bound central potentials it is often a radial quantum number nrn_r; for hydrogen it is often traded for a principal quantum number nn; for scattering states it may be an energy, wavenumber, and boundary convention.

The set {H,L2,Lz}\{H,L^2,L_z\} is therefore a natural commuting set, but it need not be complete in the presence of degeneracies. Extra labels may be required when several independent states have the same EE, ℓ\ell, and mm.

Rotational symmetry gives

[H,Lx]=[H,Ly]=[H,Lz]=0.[H,L_x]=[H,L_y]=[H,L_z]=0.

It does not make the angular momentum components commute with one another:

[Lx,Ly]=iℏLz.[L_x,L_y]=i\hbar L_z.

Thus an energy eigenstate can be chosen to have definite L2L^2 and definite LzL_z, but not generally definite LxL_x, LyL_y, and LzL_z simultaneously. The zz axis is a convention for labeling a basis inside the multiplet. In a pure central potential there is no physical zz direction.

In position representation, the same symmetry appears as angular-radial separation:

ψαℓm(r,θ,ϕ)=Rαℓ(r)Yℓm(θ,ϕ).\psi_{\alpha\ell m}(r,\theta,\phi) = R_{\alpha\ell}(r)Y_\ell^m(\theta,\phi).

The spherical harmonic carries the representation-theoretic data:

L2Yℓm=ℏ2ℓ(ℓ+1)Yℓm,LzYℓm=ℏmYℓm.L^2Y_\ell^m = \hbar^2\ell(\ell+1)Y_\ell^m, \qquad L_zY_\ell^m = \hbar mY_\ell^m.

The radial factor carries the dynamics of the particular potential. For a generic bound central potential one expects energies of the form

E=Enrℓ,E=E_{n_r\ell},

not E=EnE=E_n independent of ℓ\ell. The derivation of the separated radial equation is given in Angular and Radial Separation, and the half-line boundary conventions are collected in the Radial Schrödinger Equation.

The commutator

[H,Li]=0[H,L_i]=0

implies

[H,L±]=0,L±=Lx±iLy.[H,L_\pm]=0, \qquad L_\pm=L_x\pm iL_y.

If ∣α,ℓ,m⟩|\alpha,\ell,m\rangle is an energy eigenstate, then

H(L±∣α,ℓ,m⟩)=Eαℓ(L±∣α,ℓ,m⟩).H(L_\pm|\alpha,\ell,m\rangle) = E_{\alpha\ell}(L_\pm|\alpha,\ell,m\rangle).

The ladder operators change mm while leaving ℓ\ell fixed:

L±∣α,ℓ,m⟩=ℏℓ(ℓ+1)−m(m±1)∣α,ℓ,m±1⟩.L_\pm|\alpha,\ell,m\rangle = \hbar \sqrt{\ell(\ell+1)-m(m\pm1)} |\alpha,\ell,m\pm1\rangle.

Therefore all nonzero states in the same fixed-ℓ\ell ladder have the same energy. For each ℓ\ell this gives

2ℓ+12\ell+1

states with different mm labels. This is the magnetic degeneracy of a central potential. The word “magnetic” refers to the magnetic quantum number mm, not to the presence of a magnetic field.

This degeneracy is best understood as a representation statement. A rotationally invariant Hamiltonian acts the same way on every orientation inside an irreducible angular-momentum multiplet. The radial dynamics may change from one ℓ\ell sector to another, but it cannot distinguish m=−ℓm=-\ell from m=ℓm=\ell without a preferred direction.

Rotational symmetry guarantees less than many first encounters with the hydrogen atom suggest.

StatementGuaranteed by central symmetry?Reason
mm degeneracy within a fixed ℓ\ell sectoryesrotations relate the 2ℓ+12\ell+1 orientations
integer orbital ℓ\ell for scalar wavefunctionsyessingle-valued functions on the sphere
degeneracy between different ℓ\ell valuesnodifferent ℓ\ell sectors have different radial equations
hydrogenic n2n^2 bound-state degeneracynoit uses the special Coulomb problem
conservation of total spinnot part of this scalar modelspin requires extra Hilbert-space factors

For a generic central potential,

E=EnrℓE=E_{n_r\ell}

is the natural expectation. The ideal Coulomb potential has a stronger degeneracy:

En=−μe42(4πϵ0)2ℏ21n2,E_n = -\frac{\mu e^4}{2(4\pi\epsilon_0)^2\hbar^2} \frac{1}{n^2},

which is independent of ℓ\ell as well as mm. That stronger pattern comes from hidden structure beyond ordinary rotational invariance and is the standard example in Accidental Symmetry and Degeneracy of the Hydrogen Atom.

A small noncentral perturbation can break part of the angular-momentum labeling. For example,

H=P22m+V(r)+ϵZH = \frac{\mathbf P^2}{2m} +V(r) +\epsilon Z

selects the zz axis. The perturbation ϵZ\epsilon Z is invariant under rotations around the zz axis but not under arbitrary rotations. Consequently,

[H,Lz]=0,[H,L_z]=0,

while generally

[H,L2]≠0.[H,L^2]\ne0.

The label mm may remain useful, but ℓ\ell is no longer protected. This is the symmetry reason external fields split and mix central-potential multiplets.

Similarly, a spin-orbit interaction of the form

f(r) L⋅Sf(r)\,\mathbf L\cdot\mathbf S

is rotationally invariant under simultaneous rotations of orbital and spin degrees of freedom, but it need not commute with L\mathbf L and S\mathbf S separately. In that problem the protected angular momentum is the total

J=L+S,\mathbf J=\mathbf L+\mathbf S,

not orbital angular momentum alone. The angular-momentum-addition analysis is developed in Spin–Orbit Coupling.

Worked Example: Degeneracy from Ladder Operators

Section titled “Worked Example: Degeneracy from Ladder Operators”

Suppose HH is central and has a normalized eigenstate ∣α,ℓ,m⟩|\alpha,\ell,m\rangle with

H∣α,ℓ,m⟩=E∣α,ℓ,m⟩.H|\alpha,\ell,m\rangle = E|\alpha,\ell,m\rangle.

Since [H,L+]=0[H,L_+]=0,

H(L+∣α,ℓ,m⟩)=L+H∣α,ℓ,m⟩=E(L+∣α,ℓ,m⟩).\begin{aligned} H(L_+|\alpha,\ell,m\rangle) &= L_+H|\alpha,\ell,m\rangle \\ &= E(L_+|\alpha,\ell,m\rangle). \end{aligned}

If m<ℓm<\ell, the raised state is nonzero and proportional to ∣α,ℓ,m+1⟩|\alpha,\ell,m+1\rangle. It has the same energy EE. Repeating the argument connects all states from m=−ℓm=-\ell to m=ℓm=\ell. At the endpoints the ladder coefficient vanishes, so the argument stops naturally.

This proof uses symmetry only. It says nothing about the actual numerical value of EE, which requires solving the radial problem.

A central potential has no preferred direction. Different values of mm are different orientations of the same angular pattern relative to an arbitrarily chosen axis. Rotating the entire state changes mm components inside the same multiplet but does not change the energy.

The label ℓ\ell is different. It changes the total amount of orbital angular momentum and hence the centrifugal contribution to radial motion. That is why ℓ\ell is a dynamical sector label rather than merely an orientation label.

The central-potential problem is therefore a clean example of the general rule:

symmetry⟹commuting generators, multiplets, and degeneracies.\text{symmetry} \quad\Longrightarrow\quad \text{commuting generators, multiplets, and degeneracies}.

It is also a warning: symmetries constrain spectra, but they do not usually solve the radial dynamics by themselves.

  • Treating “central” as synonymous with “Coulomb.” The Coulomb potential is one special central potential.
  • Assuming rotational symmetry makes the energy independent of ℓ\ell. It guarantees independence of mm, not generic independence of ℓ\ell.
  • Thinking that choosing LzL_z means the system has a physical zz axis. The axis is a labeling convention unless an external field or boundary condition selects it.
  • Forgetting that LxL_x, LyL_y, and LzL_z do not commute with each other even though each commutes with a central Hamiltonian.
  • Treating spherical harmonics as hydrogen-specific functions rather than universal angular momentum eigenfunctions.
  • Applying spin-orbit conclusions to a spinless central Hamiltonian without changing the conserved angular momentum from L\mathbf L to J\mathbf J.
  • J. J. Sakurai and J. Napolitano, Modern Quantum Mechanics, 3rd ed., Cambridge University Press, 2020.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
  • A. R. Edmonds, Angular Momentum in Quantum Mechanics, Princeton University Press, 1957.
  1. Use [Li,Rj]=iℏ∑kϵijkRk[L_i,R_j]=i\hbar\sum_k\epsilon_{ijk}R_k to show that [Li,R2]=0[L_i,\mathbf R^2]=0.
Solution

Write

R2=∑jRjRj.\mathbf R^2=\sum_j R_jR_j.

Then

[Li,R2]=∑j([Li,Rj]Rj+Rj[Li,Rj]).[L_i,\mathbf R^2] = \sum_j \left( [L_i,R_j]R_j +R_j[L_i,R_j] \right).

Substitute the vector commutator:

[Li,R2]=iℏ∑j,kϵijk(RkRj+RjRk).[L_i,\mathbf R^2] = i\hbar \sum_{j,k} \epsilon_{ijk} \left( R_kR_j+R_jR_k \right).

The position components commute, so the factor in parentheses is symmetric in jj and kk. Contracting a symmetric tensor with the antisymmetric ϵijk\epsilon_{ijk} gives zero. Therefore

[Li,R2]=0.[L_i,\mathbf R^2]=0.
  1. Prove that all mm states in a fixed ℓ\ell multiplet have the same energy for a central Hamiltonian.
Solution

For a central Hamiltonian, [H,Li]=0[H,L_i]=0, hence [H,L±]=0[H,L_\pm]=0. If

H∣α,ℓ,m⟩=E∣α,ℓ,m⟩,H|\alpha,\ell,m\rangle = E|\alpha,\ell,m\rangle,

then

H(L±∣α,ℓ,m⟩)=L±H∣α,ℓ,m⟩=E(L±∣α,ℓ,m⟩).H(L_\pm|\alpha,\ell,m\rangle) = L_\pm H|\alpha,\ell,m\rangle = E(L_\pm|\alpha,\ell,m\rangle).

Whenever the laddered state is nonzero, it is proportional to ∣α,ℓ,m±1⟩|\alpha,\ell,m\pm1\rangle. Repeated raising or lowering connects every allowed mm value in the fixed ℓ\ell multiplet, so all of them share the same energy.

  1. Consider H=P2/(2m)+V(r)+ϵZH=\mathbf P^2/(2m)+V(r)+\epsilon Z. Which angular-momentum labels remain protected?
Solution

The term ϵZ\epsilon Z is invariant under rotations about the zz axis, so LzL_z remains conserved:

[H,Lz]=0.[H,L_z]=0.

It is not invariant under general rotations. For example, using

[Lx,Z]=−iℏY,[L_x,Z]=-i\hbar Y,

one finds that [H,Lx]≠0[H,L_x]\ne0 when ϵ≠0\epsilon\ne0. Therefore L2L^2 is not generally conserved, and ℓ\ell is not protected. The magnetic label mm can remain a good label, but the full 2ℓ+12\ell+1 degeneracy is generally split.

  1. Why does rotational symmetry not by itself explain the full hydrogen degeneracy?
Solution

Rotational symmetry explains degeneracy among different mm values for fixed radial label and fixed ℓ\ell. A generic central potential has energies of the form

E=Enrℓ.E=E_{n_r\ell}.

The ideal Coulomb bound-state energy depends only on

n=nr+ℓ+1,n=n_r+\ell+1,

so states with different ℓ\ell but the same nn are also degenerate. That stronger degeneracy is not forced by ordinary rotations; it is special to the Coulomb problem and its additional hidden symmetry.