We present the new
homologous series (C(NH2)3)(CH3NH3)
n
Pb
n
I3n+1 (n = 1, 2, 3)
of layered 2D perovskites. Structural characterization
by single-crystal X-ray diffraction reveals that these compounds adopt
an unprecedented structure type, which is stabilized by the alternating
ordering of the guanidinium and methylammonium cations in the interlayer
space (ACI). Compared to the more common Ruddlesden–Popper
(RP) 2D perovskites, the ACI perovskites have a different stacking
motif and adopt a higher crystal symmetry. The higher symmetry of
the ACI perovskites is expressed in their physical properties, which
show a characteristic decrease of the bandgap with respect to their
RP perovskite counterparts with the same perovskite layer thickness
(n). The compounds show a monotonic decrease in the
optical gap as n increases: E
g = 2.27 eV for n = 1 to E
g = 1.99 eV for n = 2 and E
g = 1.73 eV for n = 3, which show slightly
narrower gaps compared to the corresponding RP perovskites. First-principles
theoretical electronic structure calculations confirm the experimental
optical gap trends suggesting that the ACI perovskites are direct
bandgap semiconductors with wide valence and conduction bandwidths.
To assess the potential of the ACI perovskites toward solar cell applications,
we studied the (C(NH2)3)(CH3NH3)3Pb3I10 (n = 3) compound. Compact thin films from the (C(NH2)3)(CH3NH3)3Pb3I10 compound with excellent surface coverage can be obtained
from the antisolvent dripping method. Planar photovoltaic devices
from optimized ACI perovskite films yield a power-conversion-efficiency
of 7.26% with a high open-circuit voltage of ∼1 V and a striking
fill factor of ∼80%.