Abstract
A four-body classical trajectory Monte Carlo method and a simple binary encounter model was applied in the study of K-shell vacancy production in N7+ and Ti collisions in the impact velocity range 12–30 a.u. The total cross sections of the single and double K-shell vacancy productions are calculated and the ratios between them are compared with experimental data. Independent electron approximations fail to reproduce the measured double/single vacancy production ratios.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.