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Copper indium gallium selenide

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Copper indium gallium selenide
CIGS unit cell. Red = Cu, yellow = Se, blue = In/Ga
Identifiers
3D model (JSmol)
  • Ga:In = 1:1: InChI=1S/2Cu.Ga.In.4Se/q2*+1;2*+3;4*-2
    Key: HEKINFXMJXBFGJ-UHFFFAOYSA-N
  • Ga:In = 1:1: [Cu+1].[Cu+1].[Ga+3].[In+3].[Se-2].[Se-2].[Se-2].[Se-2]
Properties
CuIn1−xGaxSe2
Density~5.7 g/cm3
Melting point1,070 to 990 °C (1,960 to 1,810 °F; 1,340 to 1,260 K) (x = 0–1)[1]
Band gap1.0–1.7 eV (x = 0–1)[1]
Structure
tetragonal,Pearson symbol tI16[1]
I42d
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 theirstandard state (at 25 °C [77 °F], 100 kPa).
Chemical compound

Copper indium gallium (di)selenide (CIGS) is aI-III-VI2semiconductor material composed ofcopper,indium,gallium, andselenium. The material is asolid solution ofcopper indium selenide (often abbreviated "CIS") andcopper gallium selenide. It has a chemical formula of CuIn1−xGaxSe2, where the value ofx can vary from 0 (pure copper indium selenide) to 1 (pure copper gallium selenide). CIGS is atetrahedrallybonded semiconductor, with thechalcopyrite crystal structure, and abandgap varying continuously withx from about 1.0 eV (for copper indium selenide) to about 1.7 eV (for copper gallium selenide).

Structure

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CIGS is atetrahedrallybonded semiconductor, with thechalcopyrite crystal structure. Upon heating it transforms to thezincblende form and the transition temperature decreases from 1045 °C forx = 0 to 805 °C forx = 1.[1]

Applications

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

See also

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References

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  1. ^abcdTinoco, 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. Retrieved10 February 2011.
Salts and covalent derivatives of theselenide ion
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