Wenchao Yang,Catherine S. P. De Castro,Safakath Karuthedath,Yuliar Firdaus,Nisreen Alshehri,Si Chen,Diego Rosas Villalva,Christopher E. Petoukhoff,A.S. Dahman,Derya Baran,Thomas D. Anthopoulos,Frédéric Laquai,Julien Gorenflot
Abstract Long exciton diffusion length ( L D ) is key to maximizing excitation harvesting in organic solar cells, but contradicting values are reported for non‐fullerene acceptors (NFA). To understand the factors enabling large L D , experimental observation of exciton decay by transient absorption spectroscopy (TAS) is combined with microscopic Kinetic Monte Carlo (KMC) simulations on 4 ITIC derivatives. Exciton decays are fitted considering singlet exciton‐singlet exciton annihilation (SSA) and the intrinsic exciton's lifetime τ , resulting in L D from 20 to 70 nm. The critical importance of an independent estimate of τ is discussed and its measurements from pristine NFA films is found to be more relevant than from NFA molecules embedded in an inert polystyrene matrix. From experimental parameters, the microscopic Förster Resonant Energy Transfer hopping rate and the annihilation rate in a cubic lattice are determined, considering a Gaussian energetic disorder. KMC simulation of those rates are able to reproduce the experimental transients and L D , provided a lattice constant a close to the molecular π‐π stacking distance is used. It is found that this tight packing and a low disorder are critical to reach large L D , and empirically relate linearly such that 40 meV more disorder can be compensated by 1 Angstrom tighter packing (shorter a ).