Abstract
Photoionisation cross sections for the 4s, 3d and 3p subshells and the 3d angular distribution have been calculated for atomic Mn by many-body perturbation theory. Spin-orbit effects in the 3p to 3d resonance and resonances due to 3p to ns,nd (n>3) excitations have been computed. Comparison is made with recent experiments.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
