In reviewing the literature that concerns the CsCl-type intermetallic compo
und Ti2AlMo (B2), the question arises if this compound is preferably formed
with respect to the high-temperature bcc completely disordered structure (
A2). Our present work takes an ab initio approach to this subject. The firs
t-principles linear-muffin-tin-orbital method was used to calculate the tot
al energy of a series of bcc structures in the ternary system Ti-Al-Mo. Sec
ond, a cluster expansion in the tetrahedron approximation was calculated fo
r each formation energy. Finally, a Connolly-Williams-like inversion scheme
was used to obtain the formation energy of both the A2 phase and the parti
ally ordered structure B2. From the calculations, the B2 formation energy c
ame out to be aprox 10 mRy/atom lower than the A2 energy, suggesting a rela
tive greater stability. The relative stability of other possible structures
with the same global composition Ti50Al25Mo25 is discussed.