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Germanium monoselenide

From Wikipedia, the free encyclopedia
(Redirected fromGermanium(II) selenide)
"GeSe" redirects here. For other uses, seeGese (disambiguation).
Germanium monoselenide
Names
IUPAC name
Germanium selenide
Other names
germanium(II) selenide
Identifiers
3D model (JSmol)
ChemSpider
ECHA InfoCard100.031.862Edit this at Wikidata
  • InChI=1S/GeSe/c1-2
    Key: RXQPCQXEUZLFTE-UHFFFAOYSA-N
  • [Ge]=[Se]
Properties
GeSe
Molar mass151.57 g/mol
Appearanceblack
Density5.56 g/cm3
Melting point667 °C (1,233 °F; 940 K) (decomposes)
Band gap1.33 eV (direct)[1]
2.5
Structure
Orthorhombic
Pnma
Related compounds[2]
Otheranions
Germanium monoxide
Germanium monosulfide
Germanium telluride
Othercations
Tin selenide
Lead selenide
Except where otherwise noted, data are given for materials in theirstandard state (at 25 °C [77 °F], 100 kPa).
☒N verify (what is checkY☒N ?)
Chemical compound

Germanium monoselenide is achemical compound with theformula GeSe. It exists as black crystalline powder havingorthorhombic (distortedNaCl-type) crystal symmetry; at temperatures ~650 °C, it transforms into the cubic NaCl structure.[3] GeSe has been shown to have stereochemically active Ge 4s lone pairs that are responsible for the distorted structure and the relatively high position of the valence band maximum with respect to the vacuum level.[4]

To grow GeSe crystals, GeSe powder is vaporized at the hot end of a sealed ampule and allowed to condense at the cold end. Usual crystals are small and show signs of irregular growth, caused mainly by convective motion in the gaseous medium. However, GeSe grown under condition of zero-gravity and reduced convection aboard theSkylab are ~10 times larger than Earth-grown crystals, and are free from visual defects.[5][6]

References

[edit]
  1. ^Philip A. E. Murgatroyd, Matthew J. Smiles, Christopher N. Savory, Thomas P. Shalvey, Jack E. N. Swallow, Nicole Fleck, Craig M. Robertson, Frank Jäckel, Jonathan Alaria, Jonathan D. Major, David O. Scanlon, and Tim D. Veal; et al. (2020)."GeSe: Optical Spectroscopy and Theoretical Study of a van der Waals Solar Absorber".Chemistry of Materials.32 (7):3245–3253.doi:10.1021/acs.chemmater.0c00453.PMC 7161679.PMID 32308255.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  2. ^GeSe at webelements
  3. ^Wiedemeier H., Siemers P.A. (1975). "The Thermal Expansion and High Temperature Transformation of GeSe".Zeitschrift für anorganische und allgemeine Chemie.411:90–96.doi:10.1002/zaac.19754110110.
  4. ^M. J. Smiles, J. M. Skelton, H. Shiel, L. A. H. Jones, J. E. N. Swallow, H. J. Edwards, T. J. Featherstone, P. A. E. Murgatroyd, P. K. Thakur, Tien-Lin Lee, V. R. Dhanak, and T. D. Veal; et al. (2021)."Ge 4s2 Lone Pairs and Band Alignments in GeS and GeSe for photovoltaics".J. Mater. Chem. A.9 (39):22440–22452.doi:10.1039/D1TA05955F.hdl:10023/24142.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  5. ^"SP-400 Skylab, Our First Space Station". NASA. Retrieved2009-06-06.
  6. ^H. Wiedemeier; et al. (1975). "Crystal growth and transport rates of GeSe and GeTe in micro-gravity environment".Journal of Crystal Growth.31: 36.Bibcode:1975JCrGr..31...36W.doi:10.1016/0022-0248(75)90107-4.
Ge(II)
Ge(IV)
Salts and covalent derivatives of theselenide ion
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