Rotational Raman spectroscopy observes a frequency change of scattered light associated with molecular rotation. The coupling uses the induced electric dipole moment, , where is the electric polarizability tensor. For a linear molecule, the useful anisotropy is : the response differs for an electric field parallel or perpendicular to the molecular axis. A permanent electric dipole moment is not required.[ref]
For the spin-free linear rigid rotor in one internal quantum state, the anisotropic tensor depends quadratically on the molecular direction. Its angular part has even parity and degree two in spherical harmonics. The triangle inequality for coupled angular momenta permits , and even parity removes odd , leaving . The contribution is unshifted light; shifted rotational lines have . Consequently the rigid-model Stokes shifts, in ordinary frequency units, are
Successive allowed shifts are separated by , rather than the absorption spacing of pure rotational electric-dipole selection rules. In spectroscopic wavenumber units replace by and by , using the speed of light in for .
A homonuclear diatomic molecule such as molecular hydrogen has no permanent electric dipole moment in its symmetric internal state, so it lacks the ordinary electric-dipole microwave ladder. Its anisotropic electric polarizability can nevertheless give rotational Raman spectroscopy lines. Nuclear-spin symmetry can change the populations of even and odd levels, so the spin-free population example above must not be reused unchanged for molecular hydrogen. The method of coupling, as well as the energy eigenvalues, determines what the experiment can see.
For the spin-free linear rigid rotor in thermal equilibrium at temperature , assume all integer are allowed and ignore nuclear-spin restrictions. Each level has quantum states sharing one energy eigenvalue, an instance of degenerate energy levels, so the Boltzmann distribution gives
Here is a rotational partition function, the Planck constant, the Boltzmann constant, and a frequency in . Thus is dimensionless. The factor counts magnetic quantum numbers; it does not mean that a whole level is one quantum state. For the stipulated , the most populated levels are at and at .
Population alone is insufficient to predict intensity. In weak, unsaturated absorption, the integrated absorption coefficient includes the transition frequency, the squared electric dipole moment matrix element, and the difference of lower and upper substate populations because stimulated emission returns energy to the field. A pulsed FTMW spectroscopy signal additionally depends on excitation, quantum coherence, cavity tuning, and receiver response.[ref]
For an isotropic sample with polarization of an electromagnetic wave along , write . Normalized spherical harmonics give
The last equality follows from . Combining this sum with the per-substate Boltzmann distribution and subtracting stimulated emission gives relative integrated absorption areas
The common factor includes and cancels upon normalization. This formula describes integrated weak absorption in a thermal, spin-free linear rigid rotor, not arbitrary peak heights. The example's strongest integrated lines originate at and for and , respectively: they differ from the most populated levels. A missing line can reflect population, coupling, coverage, or sensitivity; it does not prove that the corresponding quantum state is absent.