Copper indium gallium selenide

Copper indium gallium selenide

CIGS unit cell. Red = Cu, yellow = Se, blue = In/Ga
Identifiers
CAS Number
  • 12018-95-0(CuInSe2)
ChemSpider
Properties
Chemical formula
CuIn1−xGaxSe2
Density ~5.7 g/cm3
Melting point 1,070 to 990 °C (1,960 to 1,810 °F; 1,340 to 1,260 K) (x = 0–1)[1]
Band gap 1.0–1.7 eV (x = 0–1)[1]
Structure
Crystal structure
tetragonal, Pearson symbol tI16 [1]
Space group
I42d
Lattice constant
a = 0.56–0.58 nm (x = 0–1), c = 1.10–1.15 nm (x = 0–1)
Except where otherwise noted, data are given for materials in their standard state (at 25 °C [77 °F], 100 kPa).
Infobox references
Chemical compound

Copper indium gallium (di)selenide (CIGS) is a I-III-VI2 semiconductor material composed of copper, indium, gallium, and selenium. The material is a solid solution of copper indium selenide (often abbreviated "CIS") and copper gallium selenide. It has a chemical formula of CuIn1−xGaxSe2, where the value of x can vary from 0 (pure copper indium selenide) to 1 (pure copper gallium selenide). CIGS is a tetrahedrally bonded semiconductor, with the chalcopyrite crystal structure, and a bandgap varying continuously with x from about 1.0 eV (for copper indium selenide) to about 1.7 eV (for copper gallium selenide).

Structure

CIGS is a tetrahedrally bonded semiconductor, with the chalcopyrite crystal structure. Upon heating it transforms to the zincblende form and the transition temperature decreases from 1045 °C for x = 0 to 805 °C for x = 1.[1]

Applications

It is best known as the material for CIGS solar cells a thin-film technology used in the photovoltaic industry.[2] In this role, CIGS has the advantage of being able to be deposited on flexible substrate materials, producing highly flexible, lightweight solar panels. Improvements in efficiency have made CIGS an established technology among alternative cell materials.

See also

References

  1. ^ a b c d Tinoco, T.; Rincón, C.; Quintero, M.; Pérez, G. Sánchez (1991). "Phase Diagram and Optical Energy Gaps for CuInyGa1−ySe2 Alloys". Physica Status Solidi A. 124 (2): 427. Bibcode:1991PSSAR.124..427T. doi:10.1002/pssa.2211240206.
  2. ^ "DOE Solar Energy Technologies Program Peer Review" (PDF). U.S. department of energy 2009. Retrieved 10 February 2011.
  • v
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Salts and covalent derivatives of the selenide ion
H2Se
H2Se2
+H
-H
He
Li2Se Be SexByOz CSe2
OCSe
(CH3)2Se
(NH4)2Se O F Ne
Na2Se MgSe Al2Se3 Si PxSey
-P
+S Cl Ar
K2Se CaSe Sc2Se3 TiSe2 V CrSe
Cr2Se3
MnSe
MnSe2
FeSe CoSe NiSe CuSe ZnSe GaSe
Ga2Se3
-Ga
GeSe
GeSe2
-Ge
As2Se3
As4Se3
Se2−
n
Br Kr
Rb2Se SrSe Y2Se3 Zr NbSe2
NbSe3
MoSe2 Tc Ru Rh Pd Ag2Se CdSe In2Se3 SnSe
SnSe2
-Sn
Sb2Se3 Te +I Xe
Cs2Se BaSe * LuSe
Lu2Se3
Hf TaSe2 WSe2
WSe3
ReSe2 Os Ir PtSe2 Au HgSe Tl2Se PbSe Bi2Se3 Po At Rn
Fr Ra ** Lr Rf Db Sg Bh Hs Mt Ds Rg CnSe Nh Fl Mc Lv Ts Og
 
* LaSe
La2Se3
CeSe
Ce2Se3
PrSe
Pr2Se3
NdSe
Nd2Se3
Pm SmSe
Sm2Se3
EuSe
Eu2Se3
GdSe
Gd2Se3
TbSe
Tb2Se3
DySe
Dy2Se3
HoSe
Ho2Se3
ErSe
Er2Se3
TmSe
Tm2Se3
YbSe
Yb2Se3
** Ac ThSe2 Pa USe2 Np PuSe Am Cm Bk Cf Es Fm Md No