Photoinduced charge separation is
the key step determining the
efficiency of photon-to-electron conversion in solar cells, while
charge carrier lifetimes govern the overall solar cell performance.
Experiments report that copper(I) thiocyanate (CuSCN) is a very promising
hole extraction layer for perovskite solar cells. Using nonadiabatic
molecular dynamics combined with ab initio time-domain
density functional theory, we show that termination of CH3NH3PbI3 (MAPbI3) at MAPbI3/CuSCN heterojunctions has a strong influence on both charge separation
and recombination. Both processes are favored by MAI termination,
compared to PbI2 termination. Because the MAPbI3 valence band originates from iodine orbitals while the conduction
band arises from Pb orbitals, MAI termination places holes close to
CuSCN, favoring extraction, and creates an MAI barrier for recombination
of electrons in MAPbI3 and holes in CuSCN. The opposite
is true for PbI2 termination. The origin of these effects
is attributed solely to the properties of the MAPbI3 surfaces,
and therefore, the conclusions should apply to other hole-transporting
materials and can be generalized to other perovskites. Importantly,
the simulations show that the injected hole remains hot for several
hundreds of femtoseconds, allowing it to escape the interfacial region
and prevent formation of bound excitons. This study suggests that
metal halide perovskites should be treated with an organic precursor,
such as MAI, prior to the formation of their interfaces with hole-transporting
materials. The reported results advance the fundamental understanding
of the highly unusual properties of metal halide perovskites and provide
specific guidelines for optimizing the performance of perovskite solar
cells and other devices.