Alloying a Cu(In,Ga)Se2 (CIGS) solar cell
absorber with
silver to form (Ag,Cu)(In,Ga)Se2 (ACIGS) is an effective
route for improving the performance of CIGS-based thin-film solar
cells by increasing the optical band gap and open-circuit voltage.
While the role of Ag on the solar cell’s performance and crystal
structure has been analyzed, important gaps in our understanding remain,
especially regarding the atomistic (short-range) structure. Previous
X-ray absorption spectroscopy (XAS) results have shown that local
atomic arrangements in Ag-free CIGS deviate from the long-range crystallographic
structure deduced from X-ray diffraction (XRD). However, it is unclear
how these structural deviations evolve with Ag alloying, particularly
in the presence of Ga depth gradient. In this work, we employ angle-resolved
XAS to probe the local environment of Se atoms within different depths
of ACIGS absorbers with varying Ag content and Ga depth gradient.
By complementing XAS results with X-ray diffraction measurements for
long-range structures, glow discharge optical emission spectroscopy
for elemental profiles, and scanning transmission electron microscopy
for morphologies, changes in element-specific bond lengths, cell parameters,
and anion displacement depending on compositions of Group [I] (Cu,
Ag) and Group [III] (In, Ga) elements were mapped. The results suggest
that the local atomic arrangement of the investigated ACIGS thin-film
solar cell samples is depth-dependent and deviates from the long-range
crystallographic structure. Possible reasons include tetragonal distortion
or the presence of other phases or off-stoichiometry compounds. For
the sample with the highest Ag content, increased bond lengths of
Se–Group [I] atoms and Se–Ga are observed from the absorber
bulk toward the near-absorber/buffer interface, whereas, in Ag-free
CIGS, no significant changes are found. Results further indicate nonlinear
anion displacement with Ag addition in the absorber bulk or with depth
composition variation, which is likely to affect the electronic properties
of solar cells. These findings offer a better understanding of the
atomic-scale properties of ACIGS absorbers in actual thin-film solar
cells containing in-depth composition variations.