Lead
toxicity and poor stability under operating conditions are
major drawbacks that impede the widespread commercialization of metal–halide
perovskite solar cells. Ti(IV) has been considered as an alternative
species to replace Pb(II) because it is relatively nontoxic and abundant
and its perovskite-like compounds have demonstrated promising performance
when applied in solar cells (η > 3%), photocatalysts, and
nonlinear
optical applications. Yet, Ti(IV) perovskites show instability in
air, hindering their use. On the other hand, Sn(IV) has a similar
cationic radius to Ti(IV), adopting the same vacancy-ordered double
perovskite (VODP) structure and showing good stability in ambient
conditions. We report here a combined experimental and computational
study on mixed titanium–tin bromide and iodide VODPs, motivated
by the hypothesis that these mixtures may show a stability higher
than that of the pure titanium compositions. Thermodynamic analysis
shows that the cations are highly miscible in these vacancy-ordered
structures. Experimentally, we synthesized mixed titanium–tin
VODPs as nanocrystals across the entire mixing range x (Cs2Ti1–x
Sn
x
X6; X = I or Br), using a colloidal synthetic
approach. Analysis of the experimental and computed absorption spectra
reveals weak hybridization and interactions between Sn and Ti octahedra
with the alloy absorption being essentially a linear combination of
the pure Sn and Ti compositions. These compounds are stabilized at
high percentages of Sn (x of ∼60%), as expected,
with bromide compositions demonstrating greater stability compared
to the iodides. Overall, we find that these materials behave akin
to molecular aggregates, with the thermodynamic and optoelectronic
properties governed by the intraoctahedral interactions.