Tin-halide
perovskite solar cells (Sn-PSCs) are promising candidates
as an alternative to toxic lead-halide PSCs. However, Sn2+ is easily oxidized to Sn4+, so Sn-PSCs are unstable in
air. Here, we use first-principles density functional theory calculations
to elucidate the oxidation process of Sn2+ at the surface
of ASnBr3 [A = Cs or CH3NH3 (MA)].
Regardless of the A-site cation, adsorption of O2 leads
to the formation of SnO2, which creates a Sn vacancy at
the surface. The A-site cation determines whether the created vacancies
are stabilized in the bulk or at the surface. For CsSnBr3, the Sn vacancy is stabilized at the surface, so further oxidation
is limited. For MASnBr3, the Sn vacancy moves into bulk
region, so additional Sn is supplied to the surface; as a result,
a continuous oxidation process can occur. The stabilization of Sn
vacancy is closely related to the polarization that the A-site cation
causes in the system.