2011
DOI: 10.1016/j.jallcom.2010.12.032
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Transparent yttrium hydride thin films prepared by reactive sputtering

Abstract: Metal hydrides have earlier been suggested for utilization in solar cells. With this as a motivation we have prepared thin films of yttrium hydride by reactive magnetron sputter deposition. The resulting films are metallic for low partial pressure of hydrogen during the deposition, and black or yellow-transparent for higher partial pressure of hydrogen. Both metallic and semiconducting transparent YH x films have been prepared directly in-situ without the need of capping layers and post-deposition hydrogenatio… Show more

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Cited by 48 publications
(45 citation statements)
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“…In contrast to what was previously reported by Mongstad et al, 6,7 we do not always obtain transparent and photochromic films after reactive sputtering of Y in Ar/H 2 mixtures followed by exposure to air. Uncapped films prepared below a certain critical deposition pressure remain dark metallic upon exposure to air.…”
contrasting
confidence: 99%
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“…In contrast to what was previously reported by Mongstad et al, 6,7 we do not always obtain transparent and photochromic films after reactive sputtering of Y in Ar/H 2 mixtures followed by exposure to air. Uncapped films prepared below a certain critical deposition pressure remain dark metallic upon exposure to air.…”
contrasting
confidence: 99%
“…To investigate the effect of different cations and postdeposition oxidation on the thin film crystal structure, the lattice constants are summarized in 7 In comparison, we observe significantly smaller lattice constants in Pd capped YH 2 , DyH 2 , and ErH 2 thin films prepared by sputtering of metal layers in pure Ar followed by a separate hydrogenation step at p H2 ¼ 1 bar at RT (full red diamonds). These results are closer to the reference values which represent highly ordered structures obtained by hydrogenation of (bulk) metals at elevated temperatures.…”
Section: A)mentioning
confidence: 99%
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“…The main recorded reflection peaks (111), (200), (220), (311), and (331) were indexed with the space group Fm 3m similar to that known for YH 2 . 12 The intensity of the (200) and the (311) peaks was seen to decrease when increasing the deposition pressure from 1 to 3 Pa. This result might be related to a difference in film texture (orientation) or to a change in the oxygen lattice.…”
mentioning
confidence: 92%
“…Table I displays the direct band gaps, E dir g , estimated from the transmittance and reflectance spectra according to the procedure described in Ref. 12. Analysis shows that E dir g increases with increasing deposition pressure.…”
mentioning
confidence: 99%