Despite
the intense research on photovoltaic lead halide perovskites, reported
optical properties as basic as the absorption onset and the optical
band gap vary significantly. To unambiguously answer the question
whether the discrepancies are a result of differences between bulk
and “near-surface” material, we perform two nonlinear
spectroscopies with drastically different information depths on single
crystals of the prototypical (CH3NH3)PbI3 methylammonium lead iodide. Two-photon absorption, detected
via the resulting generation of carriers and photocurrents (2PI–PC),
probes the interband transitions with an information depth in the
millimeter range relevant for bulk (single-crystal) material. In contrast,
the transient magneto-optical Kerr effect (trMOKE) measured in a reflection
geometry determines the excitonic transition energies in the region
near (hundreds of nm) the surface which also determine the optical
properties in typical thin films. To identify differences between
structural phases, we sweep the sample temperature across the orthorhombic–tetragonal
phase transition temperature. In the application-relevant room-temperature
tetragonal phase (at 170 K), we find a bulk band gap of 1.55 ±
0.01 eV, whereas in the near-surface region excitonic transitions
occur at 1.59 ± 0.01 eV. The latter value is consistent with
previous reflectance measurements by other groups and considerably
higher than the bulk band gap. The small band gap of the bulk material
explains the extended infrared absorption of crystalline perovskite
solar cells, the low-energy bands which carry optically driven spin-polarized
currents, and the narrow bandwidth of crystalline perovskite photodetectors
making use of the spectral filtering at the surface.