The poor stability of perovskite materials can be comprehensively
understood at the atomic level through molecular simulations based
on classical force fields. The accuracy of these force fields significantly
impacts the reliability and precision of information obtained from
molecular simulations. This study presents a detailed evaluation of
five CsPbI3 force fields developed after 2020, namely,
LJ-Coul, B-Coul, EABC, AMOEBA, and ReaxFF, with a specific focus on
their ability to accurately describe the stability and phase transitions
of CsPbI3 polymorphs. Among the five force fields evaluated,
only LJ-Coul demonstrates reasonably accurate descriptions of the
thermodynamic stability and phase transitions of the CsPbI3 system, while the other four force fields encounter various issues.
Specifically, the B-Coul force field fails to stabilize δ-CsPbI3 at 300 K and other structures at high temperatures. The EABC
force field inaccurately predicts the CsPbI3 perovskite
phases. The AMOEBA and ReaxFF force fields underestimate the stabilities
of δ- and α-CsPbI3, respectively. A thorough
analysis of these issues is provided along with proposed improvement
methods. The insights gained from this study are invaluable for selecting
an appropriate force field for CsPbI3 and offer significant
guidance for future force field development pertaining to related
materials.