The
effects of RbF postdeposition treatment (RbF-PDT) on Cu(In,Ga)Se2, CuInSe2, and CuGaSe2 thin films and
solar cell devices are comparatively studied. Similar to the effect
of the KF postdeposition treatment (KF-PDT), Cu(In,Ga)Se2 and CuInSe2 film surfaces show significant pore formation
resulting in a rough surface morphology with RbF-PDT, whereas this
is not the case for In-free CuGaSe2. The device properties
of the In-containing and In-free Cu(In,Ga)Se2 solar cells
also show contrasting results, namely, Cu(In,Ga)Se2 or
CuInSe2 devices show an increase in the open circuit voltage
(V
oc) and fill factor (FF) values and
almost constant or a slight decrease in the short-circuit current
density (J
sc) values with RbF-PDT, whereas
CuGaSe2 devices show no significant improvements in the V
oc and FF values but a substantial increase
in the J
sc values. These results suggest
that the alkali effects on the Cu(In,Ga)Se2 film and device
properties strongly depend on the group III elemental composition
in the Cu(In,Ga)Se2 films as well as alkali-metal species.
Scanning transmission electron microscopy-energy dispersive X-ray spectroscopy measurements performed on Cu(In,Ga)Se2 (CIGS) thin-film devices grown with RbF postdeposition treatment (RbF-PDT) revealed the formation of a RbInSe2 compound at the p-CIGS/n-CdS heterointerface. However, this type of Rb-compound formation was not observed with elemental In-free ternary CuGaSe2 (CGS) devices. The film surface of CIGS grown with RbF-PDT was found to be Ga-depleted; thus, the practical interface structure turned out to be CIGS/(CuInSe2, RbInSe2)/CdS. In contrast to the significant improvements observed in In-containing CIGS photovoltaic device performance with RbF-PDT, no significant improvements have been observed in In-free CGS devices thus far. These results suggest that the presence of elemental In plays a key role in obtaining beneficial alkali Rb effects for enhancing device performance as well as surface modification with RbF-PDT.
We report a scandium oxyhydride BaScOH prepared by solid state reaction under high pressure. Rietveld refinements against powder synchrotron X-ray and neutron diffraction data revealed that BaScOH adopts the ideal cubic perovskite structure (Pm3̅m), where oxide (O) and hydride (H) anions are disordered. H nuclear magnetic resonance (NMR) spectroscopy provides a positive chemical shift of about +4.4 ppm, which can be understood by the distance to the nearest (and possibly the next nearest) cation from the H nucleus. A further analysis of the NMR data and calculations based on ab initio random structure searches suggest a partial cis preference in ScOH octahedra. The present oxyhydride, if compositionally or structurally tuned, may become a candidate for H conductors.
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