CuGaS2 (Copper gallium sulfide)

Semiconductors and photonic platforms anisotropic

4 datasets, together covering 0.55–11.5 µm. Default: Boyd et al. 1971: n(o) 0.55–11.5 µm; 20 °C.

Use it in Lightsmith

Load this data in Python, simulate in one more line

pip install lightsmith
import lightsmith as ls

# CuGaS2 (Copper gallium sulfide): Boyd et al. 1971: n(o) 0.55–11.5 µm; 20 °C
cugas2 = ls.fetch_refractiveindex("main", "CuGaS2", "Boyd-20-o", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(cugas2.range_nm)  # (550, 11500) nm
eps = cugas2.eps([633])  # complex permittivity

Downloads the original record once (pinned to the imported snapshot) and caches it.

Lightsmith is open source (MIT): Mie, T-matrix, BEM, DDA, FDTD, RCWA, TMM, mode solvers and inverse design behind one spec, on CPU or GPU. GitHub.

About CuGaS2 (Copper gallium sulfide)

Copper gallium sulfide (CuGaS2) is a ternary compound semiconductor that exhibits a chalcopyrite crystal structure. This material is notable for its non-linear optical properties and is frequently employed in non-linear frequency conversion applications such as second-harmonic generation and parametric down-conversion. Its large non-linear coefficients and extensive phase-matching capabilities make it an ideal choice for infrared and mid-infrared applications. The material also boasts high thermal conductivity and damage threshold, which lends itself well to high-power optical systems. While not as commonly used as some other non-linear optical materials, copper gallium sulfide remains a specialized choice for applications requiring efficient non-linear frequency conversion, particularly in the infrared spectrum.

Other names: Copper gallium sulfide, Copper gallium disulfide

API: /v1/materials/mat_6ccc75602a61 · slug cugas2