20141128 lunch meeting
TRANSCRIPT
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Reporters : Meng-Chia Hsieh
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Introduction
1. Kesterite Structure (similar to CIGS Chalcopyrite)
2. Direct band gap energy (1.01.! e") by tuning S#Se ratio
$. %o& cost (abundant ' economical elements) replace In and Ga
SLG : Substrate
CdS / ZnS : Buffer layer (50nm)
ITO : Wind! layer (0"#$%"um)
&': *nti refle+tin' layer
(%%0nm)
CZTS : *bsrber layer (%"5$ um)
,i/*l : rnt +nta+t
& : Ba+- +nta+t (0"#$% um)
i.ZnO : Buffer layer (50nm)
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I*+
depo.
Sputter
C,-eaporation
C*/S precursor
i-*n, (0nm) depo.
I/, (200nm) depo.
-Sputter
ExperimentalExperimental
3a deposition
Sul4uri5ation
I*+ yttria-stabili5ed 5irconia
Sul4uri5ation
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Starting3a
thic6ness
+ercent o4total sodium4ound at the
sur4ace
Concentration o43a in C*/S 4i lm
region (appro7.)
1 nm 8.9: $.; < 1018cm=$
>.! nm 8.9: 1.0 < 101;cm=$
2$ nm $$.2: 2.0 < 101;cm=$
SIMSSIMS
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XPSXPS
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SEMSEM
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Sample?ain region 2
(;!@190 K)Ame"B
?ain region $
(18!@2!0 K)Ame"B
3o sodium 2> 10
1 nm 3a 2! 9
>.! nm 3a 28 2;
2$ nm 3a 2$ 2>
Extracted activation energies
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Conclusion