Thermodynamical factors that affect growth of the thallium-bearing zin
c-blende alloys InTlP and InTlAs are examined within the local density
approximation (LDA), using the linear muffin-tin orbital method. The
LDA predicts TlP and TlAs to be unstable with respect to decomposition
into the elemental constituent solids, or marginally stable if conser
vative estimates of the LDA errors are made. Several thallium-rich and
anion-rich compounds have also been examined; some are found to have
excess energies per atom comparable to the zinc-blende phase. The equi
librium partial pressures over InTlP and InTlAs have also been calcula
ted as a function of composition. Even with conservative error estimat
es, we predict that only low concentrations of thallium can be achieve
d in InTlP (<5% at 350 degrees C) using gas source molecular beam epit
axy (GSMBE), far less than the 67% needed for long-wave infrared (LWIR
)applications. Although much less than 1% thallium is predicted to be
soluble in InTlAs for GSMBE growth at 350 degrees C, the addition of e
rror estimates into the calculation indicates that obtaining the 15% t
hallium needed for LWIR applications may be possible. Native defect po
pulations have been calculated for alloy compositions corresponding to
band gaps in the LWIR, and the anion antisite densities are predicted
to be quite high, especially in InTlP, reflecting the comparable stab
ility of the TIP and TlP3 phases.