In this study, a novel structure using a sandwiched CuGa/CuInGa/In precursor layer is employed for improving the Voc and Jsc of a CIGS solar cell. The addition of a CuGa layer on the surface of CuInGa precursor enhanced the Ga concentration in the space charge region and thus enhanced the Voc by about 18.2%. The addition of an In layer to the bottom of CuGa/CuInGa/In precursors increased the absorber solar spectrum edge and thus improved the Jsc by about 14%. The device conversion efficiency using this novel precursor structure was found to increase by about 50% from 6.2% to 9.5%.
REFERENCES
1.
S.
Niki
, M.
Contreras
, I.
Repins
, M.
Powalla
, K.
Kushiya
, S.
Ishizuka1
, and K.
Matsubara
, Prog. Photovolt: Res. Appl.
18
, 453
–466
(2010
).2.
W.
Li
, Y.
Sun
, W.
Liu
, and L.
Zhou
, Solar Energy
80
, 191
–195
(2006
).3.
Y.
Goushi
, H.
Hakuma
, K.
Tabuchi
, S.
Kijima
, and K.
Kushiya
, Solar Energy Mater. Solar Cells
93
, 1318
–1320
(2009
).4.
C.-Y.
Su
, W.-H.
Ho
, H.-C.
Lin
, C.-Y.
Nieh
, and S.-C.
Liang
, Solar Energy Mater. Solar Cells
95
, 261
–263
(2011
).5.
V.
Alberts
, J.
Titus
, and R. W.
Birkmire
, Thin Solid Films
451–452
, 207
–211
(2004
).6.
V.
Alberts
, Thin Solid Films
517
, 2115
–2120
(2009
).7.
H.
Park
, S. C.
Kim
, S.-H.
Lee
, J.
Koo
, S. H.
Lee
, C.-W.
Jeon
, S.
Yoon
, and W. K.
Kim
, Thin Solid Films
519
, 7245
–7249
(2011
).8.
T.
Nakada
and A.
Kunioka
, Appl. Phys. Lett.
74
, 17
(1999
).9.
C.-S.
Jiang
, F. S.
Hasoon
, H. R.
Moutinho
, H. A.
Al-Thani
, M. J.
Romero
, and M. M.
Al-Jassim
, Appl. Phys. Lett.
82
, 1
(2003
).10.
W. K.
Metzger
, I. L.
Repins
, and M. A.
Contreras
, Appl. Phys. Lett.
93
, 022110
(2008
).11.
J.
Song
, S. S.
Li
, C. H.
Huang
, O. D.
Crisalle
, and T. J.
Anderson
, Solid State Electron.
48
, 73
–79
(2004
).12.
C.-S.
Jiang
, R.
Noufi
, K.
Ramanathan
, J. A.
AbuShama
, H. R.
Moutinho
, and M. M.
Al-Jassim
, Appl. Phys. Lett.
85
, 13
(2004
).13.
S.-H.
Wei
, S. B.
Zhang
, and A.
Zunger
, Appl. Phys. Lett.
72
, 3199
–3201
(1998
).© 2012 American Institute of Physics.
2012
American Institute of Physics
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