Relativistic calculations of angle-dependent photoemission time delay
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.
|Collections||ANU Research Publications|
|Source:||Physical Review A|
|Access Rights:||Open Access|
|01 Kheifets A Relativistic calculations of 2016.pdf||186.49 kB||Adobe PDF|
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