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.
Cite
CITATION STYLE
APA
Kheifets, A., Mandal, A., Deshmukh, P. C., Dolmatov, V. K., Keating, D. A., & Manson, S. T. (2016). Relativistic calculations of angle-dependent photoemission time delay. Physical Review A, 94(1). https://doi.org/10.1103/PhysRevA.94.013423
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free