posted on 2016-09-21, 00:00authored byZhuan Zhu, Viktor G. Hadjiev, Yaoguang Rong, Rui Guo, Bo Cao, Zhongjia Tang, Fan Qin, Yang Li, Yanan Wang, Fang Hao, Swaminathan Venkatesan, Wenzhi Li, Steven Baldelli, Arnold M. Guloy, Hui Fang, Yandi Hu, Yan Yao, Zhiming Wang, Jiming Bao
Microscopic
understanding of interaction between H2O
and MAPbI3 (CH3NH3PbI3) is essential to further improve efficiency and stability of perovskite
solar cells. A complete picture of perovskite from initial physical
uptake of water molecules to final chemical transition to its monohydrate
MAPbI3·H2O is obtained with in situ infrared
spectroscopy, mass monitoring, and X-ray diffraction. Despite strong
affinity of MA to water, MAPbI3 absorbs almost no water
from ambient air. Water molecules penetrate the perovskite lattice
and share the space with MA up to one H2O per MA at high-humidity
levels. However, the interaction between MA and H2O through
hydrogen bonding is not established until the phase transition to
monohydrate where H2O and MA are locked to each other.
This lack of interaction in water-infiltrated perovskite is a result
of dynamic orientational disorder imposed by tetragonal lattice symmetry.
The apparent inertness of H2O along with high stability
of perovskite in an ambient environment provides a solid foundation
for its long-term application in solar cells and optoelectronic devices.