QED Corrections and Hyperfine Structure/Nuclear Size, Moments, and Isotope Shifts

Lesson 4.31,015 words

Nuclear Size, Moments, and Isotope Shifts

A real nucleus has a finite size, a mass that changes between isotopes, and, when its spin is at least one, an electric quadrupole moment. Each leaves a fingerprint in the atomic spectrum: the volume shift from s-electrons sampling the charge distribution, the mass and field isotope shifts that separate on a King plot, the quadrupole interaction that breaks the Landé interval rule, and the hyperfine anomaly from the magnetization distribution.

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The hyperfine structure treated the nucleus as a point magnetic dipole. Three further departures from a structureless point charge shift atomic levels measurably: the nucleus has a finite spatial extent, its mass differs from one isotope to the next, and if its spin is it carries an electric quadrupole moment. Each effect is small, but each maps a distinct nuclear property onto the spectrum, and laser spectroscopy has become a standard tool for measuring nuclear charge radii and moments — including for short-lived isotopes produced one atom at a time.

The finite nuclear size

A point charge produces the Coulomb potential all the way to . A real nucleus of radius spreads its charge over a small ball, so an electron that penetrates inside sees less charge enclosed. Modelling the nucleus as a uniformly charged sphere, the potential inside is a parabola that stays finite at the origin,

matching the point potential at . The difference is positive (the real potential is less deep) and confined to . Only -electrons have appreciable density there. Treating as constant across the tiny nuclear volume, first-order perturbation theory gives a level shift1

where is the mean-square nuclear charge radius ( for the uniform sphere). The shift is positive: finite size reduces the binding of -states, because the electron spends part of its time where the attraction is weaker than a point charge would supply.

A point nucleus (dashed) gives the full 1/r Coulomb well; a finite nucleus of radius R (solid) flattens the potential inside, so a penetrating s-electron is bound slightly less tightly. The gap acts only for r < R.

For hydrogen the volume shift is about in the level — a minute effect that nevertheless enters the precision determination of the Rydberg constant. It grows steeply with nuclear charge, roughly as through the electron density and the growing radius, so in heavy atoms it dominates the isotope shift.

The isotope shift

Comparing the same spectral line in two isotopes of one element reveals a small frequency difference, the isotope shift, with two additive origins.

  • Mass shift. The atomic energies depend on the nucleus only through the reduced mass ; a heavier isotope has a slightly larger and therefore deeper levels. The normal mass shift follows directly from , giving a fractional shift between isotopes of masses and , In many-electron atoms a specific mass shift (mass polarization) adds a cross term of the same scale but of either sign and much harder to compute. Both fall off as , so the mass shift dominates the isotope shift in light elements.
  • Field (volume) shift. The difference in nuclear charge radius between the isotopes changes the volume shift derived above, which grows as (or faster) through the electron density and so dominates the isotope shift in heavy elements.
The same line measured in two isotopes appears at slightly different frequencies. The heavier isotope (larger reduced mass, larger charge radius) is displaced from the lighter one; the split is the isotope shift.

Because the mass and field shifts scale differently with mass and with the electronic transition, they can be separated. Plotting the modified isotope shift of one transition against that of another for a chain of isotopes produces a straight line — a King plot — whose slope and intercept isolate the field and mass contributions, and thus across the chain. This is how the charge radii of exotic isotopes far from stability are measured.

A King plot. For an isotope chain the mass-scaled shift of one line plotted against that of a second line falls on a straight line; the slope fixes the ratio of field-shift factors and the intercept the mass contribution.

The electric quadrupole interaction

A nucleus with spin can be non-spherical, carrying an electric quadrupole moment . A quadrupole has no interaction with a uniform field, but it couples to the gradient of the electric field the electrons produce at the nucleus. This adds a term to the hyperfine Hamiltonian beyond the magnetic dipole,

with the quadrupole coupling constant set by the nuclear moment and the electronic field gradient.2 Unlike the magnetic-dipole energy, which is linear in , the quadrupole energy is quadratic in . Its presence breaks the Landé interval rule: successive hyperfine intervals are no longer proportional to . Fitting the departures from the interval rule extracts , and thence once the electronic field gradient is known.

A prolate nucleus (quadrupole moment Q) in the electric field gradient of the electrons. The energy depends on the orientation of the nuclear spin relative to the gradient axis, adding a term quadratic in I·J.

The hyperfine anomaly

The magnetic hyperfine constant is proportional to the nuclear -factor, so the ratio of -values for two isotopes should equal the ratio of their -factors. It does not, quite. The nuclear magnetization is distributed over the nuclear volume rather than sitting at a point, and -electrons sample that distribution. The resulting fractional discrepancy is the hyperfine anomaly (the Bohr–Weisskopf effect),

where is typically .3 Small as it is, the anomaly is a rare window on how magnetization is arranged inside the nucleus, complementing the charge-radius information from the field shift.

Reading nuclear structure from atomic spectra

Collecting the effects of this module, each nuclear property leaves a specific, separable signature in the atomic spectrum.

Nuclear propertyAtomic signatureExtracted from
Spin number of hyperfine componentscounting multiplet lines
Magnetic moment magnetic constant Landé interval spacings
Quadrupole moment quadrupole constant interval-rule departures
Mean-square radius field (volume) shiftKing plot of isotope shifts
Magnetization distributionhyperfine anomaly-ratio vs -ratio

The precision of these measurements makes atomic spectroscopy a nuclear probe. The muonic-hydrogen Lamb shift — where the muon's small orbit magnifies the volume shift by — measured the proton charge radius to , and the initial disagreement with the value from ordinary hydrogen (the proton radius puzzle) drove a decade of re-measurement before converging.4 Optical spectroscopy of trapped radioactive isotopes now maps along entire isotope chains, turning the atom into an instrument for nuclear physics. The hierarchy established across this module — gross structure, fine structure, the Lamb shift, hyperfine structure, and now the nuclear corrections — is the full ledger of what sets an atomic energy level, ordered from the electronvolt down to the fraction of a megahertz.

Footnotes

  1. Bransden & Joachain, §5.6 — the finite-nuclear-size (volume) correction from a uniformly charged sphere, ; see also Foot, §6.4.
  2. Foot, §6.5 — the electric-quadrupole hyperfine energy and the breaking of the Landé interval rule; the quadrupole coupling constant . Also Demtröder, Ch. 5.
  3. Foot, §6.5 — the hyperfine anomaly (Bohr–Weisskopf effect) from the finite distribution of nuclear magnetization. Bohr, A. & Weisskopf, V. F. (1950), Phys. Rev. 77, 94.
  4. Antognini, A. et al. (2013), Proton Structure from the Measurement of 2S–2P Transition Frequencies of Muonic Hydrogen, Science 339, 417: . CODATA 2018 proton rms charge radius , physics.nist.gov/cgi-bin/cuu/Value?rp.

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