Comparison of the Migdal transition probabilities in electron-atom inelastic cross sections
Wakutaka Nakano
TL;DR
This work assesses the reliability of Migdal transition probabilities for dark matter–nucleus scattering by directly comparing them to total single-electron inelastic cross sections in isolated Ar and Xe. Using a center-of-mass formalism and a Born-level Coulomb interaction, the cross section is connected to Migdal transition factors derived from FAC calculations, revealing sizable discrepancies: ~30% for Argon and ~80% for Xenon around 1 keV. The dominance of outer-shell excitations (Ar: 3p; Xe: 5p, with 4d contributing at higher fractions) explains much of the difference and highlights sensitivities to shell structure and correlation effects. The study also contrasts these results with Bethe-type and Salvat cross sections, noting underestimation in the keV regime and emphasizing avenues for improvement, including multi-channel and liquid-atom effects for realistic detector contexts.
Abstract
The Migdal transition probabilities for dark matter scattering are compared to the total single-electron inelastic cross sections of electron-atom scattering for isolated Ar and Xe. The comparison is done by expressing the electron-atom scattering cross section by connecting the Migdal probability. The resultant differences are around $30 \ \%$ for Ar and $80 \ \%$ for Xe in $\sim$ 1 keV of incoming electron energy. The transition is dominated from the $3p$ shell electrons for Ar. For Xe, $5p$ states dominate the contribution, but, $4d$ states give $\sim 40\ \%$ contribution at 1 keV.
