20141128 lunch meeting

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  • 7/23/2019 20141128 Lunch Meeting

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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