Mercury selenide (HgSe) is a narrow-bandgap II-VI semiconductor compound formed from mercury and selenium. It is primarily used in infrared (IR) detection and thermal imaging applications, where its ability to respond to mid- and long-wavelength infrared radiation makes it valuable for military, aerospace, and scientific instrumentation. HgSe is chosen for photodetectors and focal plane arrays in scenarios requiring sensitivity in the IR spectrum; it competes with alternatives like HgCdTe and InSb but offers distinct band alignment properties for specific wavelength windows.
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| Property | Value | Unit | Conditions | Source | |
|---|---|---|---|---|---|
Bulk Modulus(K)2 entries | 41.17 | GPa | — | ||
| ↳ | 45.90 | GPa | — | ||
Poisson's Ratio(ν) | 0.3800 | - | — | ||
Shear Modulus(G)2 entries | 13.25 | GPa | — | ||
| ↳ | 13.44 | GPa | — |
| Property | Value | Unit | Conditions | Source | |
|---|---|---|---|---|---|
Density(ρ) | 7.661 | kg/m³ | — |
| Property | Value | Unit | Conditions | Source | |
|---|---|---|---|---|---|
Band Gap(Eg)2 entries | 0.07000 | eV | — | ||
| ↳ | 0.000 | eV | — | ||
Dielectric Constant (Relative Permittivity)(εr) | 25.33 | - | — | ||
Magnetic Moment(μB) | 0.000 | µB | — | ||
Piezoelectric Modulus(eij) | 0.9658 | C/m² | — | ||
Seebeck Coefficient(S) | -66.64 | µV/K | — |
| Property | Value | Unit | Conditions | Source | |
|---|---|---|---|---|---|
Energy Above Hull(ΔEhull) | 0.01740 | eV/atom | — | ||
Formation Energy(ΔHf)2 entries | -0.2254 | eV/atom | — | ||
| ↳ | 0.00402 | eV/atom | — |