The
efficiency of Cu(In,Ga)Se2 (CIGS)-based solar cells
can be markedly improved by controlled introduction of alkali metal
(AM) atoms using post-deposition treatment (PDT) after CIGS growth.
Previous studies have indicated that AM atoms may act as impurities
or agglomerate into secondary phases. To enable further progress,
understanding of atomic level processes responsible for these improvements
is required. To this end, we have investigated theoretically the effects
of the AM elements Li, Na, K, Rb, and Cs on the properties of the
parent material CuInSe2. First, the effects of the AM impurities
in CuInSe2 have been investigated in terms of formation
energies, charge transition levels, and migration energy barriers.
We found that AM atoms preferentially substitute for Cu atoms at the
neutral charge state. Under In-poor conditions, AM atoms at the In
site also show low formation energies and are acceptors. The migration
energy barriers show that the interstitial diffusion mechanism may
be relevant only for Li, Na, and K, whereas all the AM atoms can diffuse
with the help of Cu vacancies. The competition between these two mechanisms
strongly depends on the concentration of Cu vacancies. We also discuss
how AM atoms can contribute to increasing Cu-depleted regions. Second,
AM atoms can form secondary phases with Se and In atoms. We suggest
a mechanism for the secondary phase formation following the PDT process.
On the basis of the calculated reaction enthalpies and migration considerations,
we find that mixed phases are more likely in the case of LiInSe2 and NaInSe2, whereas formation of secondary phases
is expected for KInSe2, RbInSe2, and CsInSe2. We discuss our findings in the light of experimental results
obtained for AM treatments. The secondary phases have large energy
band gaps and improve the morphology of the buffer surface by enabling
a favorable band alignment, which can improve the electrical properties
of the device. Moreover, they can also passivate the surface by forming
a diffusion barrier. Overall, our work points to different roles played
by the light and heavy AM atoms and suggests that both types may be
needed to maximize their benefits on the solar cell performance.