Abstract
Angular dependence of photoemission time delay for the valence np3/2 and np1/2 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.
Original language | English |
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Article number | 013423 |
Journal | Physical Review A |
Volume | 94 |
Issue number | 1 |
DOIs | |
Publication status | Published - 25 Jul 2016 |