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Rotor in External Fields: First Encounter

An isolated rigid rotor has full rotational symmetry. Its energy depends on JJ but not on MM, so every level with J>0J\gt0 contains a (2J+1)(2J+1)-fold multiplet. An external field changes the question: the field selects a direction in space, breaks the full rotational symmetry, and can split or mix states that were previously degenerate.

This page is a first encounter. It explains the symmetry logic and the simplest electric-field coupling for a polar linear rotor. Detailed Stark and Zeeman spectroscopy, line strengths in fields, hyperfine structure, and molecular-structure fits belong to later molecular and approximation-method pages.

The ideal linear rotor Hamiltonian is

H^0=BEJ^2/ℏ2,BE=ℏ22I.\hat H_0 = B_E\hat J^2/\hbar^2, \qquad B_E = \frac{\hbar^2}{2I}.

The eigenstates are

∣J,M⟩,J=0,1,2,…,M=−J,…,J,\lvert J,M\rangle, \qquad J=0,1,2,\ldots, \qquad M=-J,\ldots,J,

with energies

EJ(0)=BEJ(J+1).E_J^{(0)} = B_EJ(J+1).

The energy does not depend on MM. The degeneracy is a symmetry statement: without a selected axis, the different orientations of a fixed angular-momentum multiplet are physically equivalent.

A static uniform field supplies a laboratory vector. If the field is chosen along the lab zz axis, the full rotation symmetry is reduced to rotations about that axis:

SO(3)⟶SO(2).SO(3) \longrightarrow SO(2).

The usual consequence is:

  • MM often remains a good quantum number, because rotations about the field axis remain a symmetry.
  • JJ need not remain a good quantum number, because the field can mix different total-angular-momentum multiplets.
  • The old MM degeneracy can be partly or fully lifted.
  • Parity can be broken by a static electric field acting on a permanent dipole.

The exact outcome depends on the coupling. A scalar perturbation preserves more symmetry than a vector perturbation; a magnetic field can also break time-reversal symmetry.

Rigid rotor in a static external field and schematic multiplet splitting

A static electric field selects the lab zz axis. For a polar rotor, the interaction V=−dEcos⁡θV=-d\mathcal E\cos\theta depends on the angle between the molecular axis and the field. Axial symmetry can preserve MM while splitting the field-free MM multiplet.

For a polar linear molecule with body-fixed dipole magnitude dd, a static electric field

E=Ez^\boldsymbol{\mathcal E} = \mathcal E\hat{\mathbf z}

gives the orienting interaction

V^E=−d⋅E=−dEcos⁡θ,\hat V_E = - \mathbf d\cdot\boldsymbol{\mathcal E} = - d\mathcal E\cos\theta,

where θ\theta is the angle between the molecular axis and the field axis.

The Hamiltonian is

H^=BEJ^2/ℏ2−dEcos⁡θ.\hat H = B_E\hat J^2/\hbar^2 - d\mathcal E\cos\theta.

The dimensionless field strength is roughly

η=dEBE.\eta = \frac{d\mathcal E}{B_E}.

When η≪1\eta\ll1, perturbation theory is appropriate. When η\eta is large, the rotor becomes partially oriented and the eigenstates are often called pendular states. That strong-field regime is beyond this first encounter.

The operator cos⁡θ\cos\theta is not diagonal in JJ. Its action on spherical harmonics has the form

cos⁡θ YJM=aJ+1,MYJ+1M+aJ,MYJ−1M,\cos\theta\,Y_J^M = a_{J+1,M}Y_{J+1}^M + a_{J,M}Y_{J-1}^M,

where

aJ+1,M=(J+1)2−M2(2J+1)(2J+3),a_{J+1,M} = \sqrt{ \frac{(J+1)^2-M^2} {(2J+1)(2J+3)} },

and

aJ,M=J2−M2(2J−1)(2J+1).a_{J,M} = \sqrt{ \frac{J^2-M^2} {(2J-1)(2J+1)} }.

Thus the static electric field couples states with

ΔJ=±1,ΔM=0\Delta J=\pm1, \qquad \Delta M=0

when the field defines the lab zz axis. The MM selection rule is the axial-symmetry statement. The ΔJ\Delta J rule is the angular structure of a vector operator.

For the simple linear rigid rotor, the diagonal matrix element

⟨J,M∣cos⁡θ∣J,M⟩\langle J,M\vert\cos\theta\vert J,M\rangle

vanishes. One way to see this is parity: ∣J,M⟩\lvert J,M\rangle has parity (−1)J(-1)^J, while cos⁡θ\cos\theta is parity odd. Therefore the first-order Stark shift is zero for an isolated field-free rotor level.

The first nonzero shift is typically second order in the electric field. For the ground state, only ∣1,0⟩\lvert1,0\rangle contributes at lowest order because

cos⁡θ Y00=13Y10.\cos\theta\,Y_0^0 = \frac{1}{\sqrt3}Y_1^0.

Using

E1(0)−E0(0)=2BE,E_1^{(0)}-E_0^{(0)} = 2B_E,

the second-order shift is

ΔE0,0(2)=∣⟨1,0∣(−dEcos⁡θ)∣0,0⟩∣2E0(0)−E1(0)=−d2E26BE.\begin{aligned} \Delta E_{0,0}^{(2)} &= \frac{ \left\lvert \langle1,0\vert (-d\mathcal E\cos\theta) \vert0,0\rangle \right\rvert^2 } {E_0^{(0)}-E_1^{(0)}} \\ &= - \frac{d^2\mathcal E^2}{6B_E}. \end{aligned}

This negative shift is the simplest quantum version of induced alignment: the field lowers the energy by admixing a small amount of the J=1J=1 state into the J=0J=0 ground state.

The field-free rotor has energy EJ(0)E_J^{(0)} independent of MM. A static electric field along zz preserves rotations about zz, so MM remains a useful label, but the energy shifts can depend on MM.

For an electric field alone and no additional time-reversal breaking, states with MM and −M-M often remain degenerate. Thus the J=1J=1 triplet can split into an M=0M=0 level and a twofold ∣M∣=1\lvert M\rvert=1 level rather than three unrelated levels.

A magnetic field can split the signs of MM if the rotor has a magnetic moment that couples to the field. In a simple effective model with

μ=γJ^,\boldsymbol\mu = \gamma\hat{\mathbf J},

the Zeeman-like perturbation is

V^B=−μ⋅B=−γBzJ^z.\hat V_B = - \boldsymbol\mu\cdot\mathbf B = - \gamma B_z\hat J_z.

Then

ΔEJ,M(1)=−γBzℏM.\Delta E_{J,M}^{(1)} = - \gamma B_z\hbar M.

This formula is a model for a rotor with the stated magnetic moment. It should not be applied automatically to every neutral rigid rotor.

The safest way to decide labels is to ask what commutes with the Hamiltonian.

For the field-free rotor,

[H^0,J^2]=0,[H^0,J^z]=0.[\hat H_0,\hat J^2]=0, \qquad [\hat H_0,\hat J_z]=0.

For the electric-field rotor,

H^=BEJ^2/ℏ2−dEcos⁡θ,\hat H = B_E\hat J^2/\hbar^2 - d\mathcal E\cos\theta,

the Hamiltonian still commutes with J^z\hat J_z:

[H^,J^z]=0,[\hat H,\hat J_z]=0,

because the field is axially symmetric about zz. But it does not commute with J^2\hat J^2:

[H^,J^2]≠0.[\hat H,\hat J^2]\ne0.

Therefore MM can label exact eigenstates in the static field, while JJ becomes an approximate or field-free label when the electric coupling is nonzero.

External fields change rotational spectra in two ways. First, they shift the energy levels. Second, they change the eigenstates, and therefore change transition matrix elements and selection-rule details.

In weak fields, one often speaks of Stark or Zeeman shifts of the field-free rotational lines. In stronger fields, the states are better described as field-dressed rotor states, and the field-free JJ label becomes only a guide.

The canonical lesson here is modest but important: a degeneracy is not just a repeated number in a formula. It encodes a symmetry. Once an external field removes part of the symmetry, the degeneracy can split.

  • Treating an external field as adding the same constant energy to every rotor state.
  • Assuming JJ remains an exact quantum number for a polar rotor in a static electric field.
  • Expecting a first-order Stark shift for the J=0J=0 state of a simple linear rotor.
  • Forgetting that an electric field can preserve MM while mixing different JJ values.
  • Applying a permanent-dipole coupling to a homonuclear diatomic molecule with no body-fixed electric dipole.
  • Using a Zeeman formula without specifying the magnetic moment that couples to the field.
  • Confusing the lab field axis with the molecule’s body-fixed axis.
  1. Which field-free quantum numbers remain exact for a polar linear rotor in a static electric field along zz?
Solution

The field leaves rotations about the zz axis as a symmetry, so MM remains exact. The perturbation is proportional to cos⁡θ\cos\theta, which mixes JJ with J±1J\pm1, so JJ is not exact once the field is nonzero.

  1. Show directly that the first-order Stark shift of the J=0J=0 state vanishes.
Solution

For J=0J=0,

Y00=14π.Y_0^0 = \frac{1}{\sqrt{4\pi}}.

The first-order shift is proportional to

∫S2(Y00)∗cos⁡θY00 dΩ.\int_{S^2} \left(Y_0^0\right)^* \cos\theta Y_0^0\,d\Omega.

This is

14π∫02π∫0πcos⁡θsin⁡θ dθ dϕ=0,\frac{1}{4\pi} \int_0^{2\pi} \int_0^\pi \cos\theta\sin\theta\,d\theta\,d\phi = 0,

because the integrand is odd under reflection across the equator.

  1. Use cos⁡θ Y00=Y10/3\cos\theta\,Y_0^0=Y_1^0/\sqrt3 to compute the second-order ground-state Stark shift.
Solution

The only coupled state at this order is ∣1,0⟩\lvert1,0\rangle. The matrix element is

⟨1,0∣(−dEcos⁡θ)∣0,0⟩=−dE3.\langle1,0\vert (-d\mathcal E\cos\theta) \vert0,0\rangle = - \frac{d\mathcal E}{\sqrt3}.

Since E1(0)−E0(0)=2BEE_1^{(0)}-E_0^{(0)}=2B_E,

ΔE0,0(2)=d2E2/3−2BE=−d2E26BE.\Delta E_{0,0}^{(2)} = \frac{d^2\mathcal E^2/3}{-2B_E} = - \frac{d^2\mathcal E^2}{6B_E}.
  1. In the effective magnetic model V^B=−γBzJ^z\hat V_B=-\gamma B_z\hat J_z, what are the first-order shifts of the J=1J=1 states?
Solution

For J=1J=1, the possible values are

M=−1,0,1.M=-1,0,1.

Since J^z∣J,M⟩=ℏM∣J,M⟩\hat J_z\lvert J,M\rangle=\hbar M\lvert J,M\rangle,

ΔE1,M(1)=−γBzℏM.\Delta E_{1,M}^{(1)} = - \gamma B_z\hbar M.

Thus

ΔE1,−1(1)=γBzℏ,ΔE1,0(1)=0,ΔE1,1(1)=−γBzℏ.\Delta E_{1,-1}^{(1)} = \gamma B_z\hbar, \qquad \Delta E_{1,0}^{(1)} = 0, \qquad \Delta E_{1,1}^{(1)} = - \gamma B_z\hbar.
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