TY - JOUR
T1 - Finite-temperature structure of the MAPbI3 perovskite
T2 - Comparing density functional approximations and force fields to experiment
AU - Lahnsteiner, Jonathan
AU - Kresse, Georg
AU - Heinen, Jurn
AU - Bokdam, Menno
N1 - Funding Information:
We would like to thank D. Dubbeldam for valuable input for the classical simulations with RASPA. Funding by the Austrian Science Fund (FWF): P 30316-N27 is gratefully acknowledged. Computations were performed on the Vienna Scientific Cluster VSC3.
Publisher Copyright:
© 2018 American Physical Society.
PY - 2018/7/16
Y1 - 2018/7/16
N2 - Determining the finite-temperature structure of the hybrid perovskite MAPbI3 is a challenge for both experimental and theoretical methods. A very powerful computational method that can resolve the atomic structure is molecular dynamics (MD). The resulting structure depends on the density functional approximation (DFA) in the case of ab initio MD and the force field in classical MD. We compare the structure between 250 and 400 K obtained with different DFAs and force fields in one consistent manner. The symmetry of the PbI3 framework is analyzed as well as the relative ordering of the neighboring organic molecules inside the framework. The distribution function of the molecules is used to map out an effective energy surface for the rotation of a single molecule. This surface is accurately modeled by a pair of cubic harmonics. Available experimental data in literature are discussed and compared to the structure obtained with the different methods. The spread in these data is still too large to uniquely determine the method that "best" describes the perovskite, however, promising candidates and outliers have been identified.
AB - Determining the finite-temperature structure of the hybrid perovskite MAPbI3 is a challenge for both experimental and theoretical methods. A very powerful computational method that can resolve the atomic structure is molecular dynamics (MD). The resulting structure depends on the density functional approximation (DFA) in the case of ab initio MD and the force field in classical MD. We compare the structure between 250 and 400 K obtained with different DFAs and force fields in one consistent manner. The symmetry of the PbI3 framework is analyzed as well as the relative ordering of the neighboring organic molecules inside the framework. The distribution function of the molecules is used to map out an effective energy surface for the rotation of a single molecule. This surface is accurately modeled by a pair of cubic harmonics. Available experimental data in literature are discussed and compared to the structure obtained with the different methods. The spread in these data is still too large to uniquely determine the method that "best" describes the perovskite, however, promising candidates and outliers have been identified.
UR - http://www.scopus.com/inward/record.url?scp=85059585588&partnerID=8YFLogxK
U2 - 10.1103/PhysRevMaterials.2.073604
DO - 10.1103/PhysRevMaterials.2.073604
M3 - Article
AN - SCOPUS:85059585588
SN - 2475-9953
VL - 2
JO - Physical Review Materials
JF - Physical Review Materials
IS - 7
M1 - 073604
ER -