Dec 2, 2024
3:00pm - 3:30pm
Hynes, Level 3, Room 308
Mario Borunda1,Rosty Martinez1,Ahmad Kirmani2,Ian Sellers3
Oklahoma State University1,Rochester Institute of Technology2,University at Buffalo, The State University of New York3
Mario Borunda1,Rosty Martinez1,Ahmad Kirmani2,Ian Sellers3
Oklahoma State University1,Rochester Institute of Technology2,University at Buffalo, The State University of New York3
Predicting radiation damage to materials requires estimating the threshold displacement energy (E<sub>d</sub>). We calculated E<sub>d</sub> using <i>ab initio</i> molecular dynamics for halide perovskites. The E<sub>d</sub> values we have obtained, which are considerably lower than those commonly assumed in the literature for several species, hold significant implications for predicting radiation damage to materials. We performed Monte Carlo simulations with the AIMD-obtained E<sub>d</sub> and compared them to those obtained using the default E<sub>d</sub>. Our results show an increase in specific vacancies in halide perovskites that were not captured in simulations using the default E<sub>d </sub>values. This suggests that the default E<sub>d </sub>values may not accurately predict the radiation damage in these materials.