Radiative corrections to the spin asymmetry in elastic polarized electron-nucleus collisions at high energy
D. H. Jakubassa-Amundsen
TL;DR
The paper addresses radiative corrections to the beam-normal spin asymmetry $S$ in elastic $e$–nucleus scattering by combining dispersive two-photon exchange with nonperturbative QED corrections implemented as $V_{ m vac}$ and $V_{ m vs}$ in the Dirac equation. It extends dispersion calculations to GeV energies and evaluates the total effect $S_{ m tot}$ for $^{208}$Pb and $^{12}$C, finding that QED corrections can dominate in many cases, while dispersion remains significant at lower energies and larger angles for Pb. Across the studied kinematics, the theory largely fails to explain high-energy experimental measurements beyond 500 MeV, particularly for Pb, indicating unresolved physics (the Pb puzzle) at GeV energies. The work highlights the relative importance of dipole, quadrupole, and octupole nuclear excitations in shaping $S$ and demonstrates the necessity of combining dispersion with nonperturbative QED effects for accurate predictions in elastic polarized electron–nucleus collisions.
Abstract
Modifying the numerical codes, dispersion corrections to the beam-normal spin asymmetry which arise from low-lying transient nuclear excitations up to 30 MeV, are estimated for collision energies between 50 MeV and 1 GeV. A nonperturbative calculation of vacuum polarization and the vertex plus self-energy correction, using optimized potentials, indicates that for small scattering angles both these quantum electrodynamical (QED) effects on the spin asymmetry decrease with energy above 200 MeV and can be neglected at high energies. Examples are given for the 12C and 208Pb nuclei. The available measurements of the spin asymmetry at collision energies beyond 500 MeV cannot be explained by the present theory.
