Abstract
Angular dependence of photoemission time delay for the valence and subshells of Ar, Kr, and Xe is studied in the dipole relativistic random phase approximation. Strong angular anisotropy of the time delay is reproduced near respective Cooper minima while the spin-orbit splitting affects the time delay near threshold.
- Received 20 May 2016
DOI:https://doi.org/10.1103/PhysRevA.94.013423
©2016 American Physical Society