Optical constants
Refractive index of MgAl2O4 (Magnesium aluminate, spinel)
Chernova et al. 2017: n,k 0.14–1.67 µm
- Data
- tabulated nk
- Range
- 0.1409–1.675 µm
- Points
- 100
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 1.71338
- Extinction coefficient k
- 9.39116e-13
- Permittivity ε1
- 2.93568
- Permittivity ε2
- 3.21813e-12
- Absorption coefficient α
- 2.00839e-07 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 9.95824e+13 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- -0.0558899 µm⁻¹
- Group index ng
- 1.74622
- Group velocity dispersion
- — fs²/mm
- Dispersion parameter D
- — ps/(nm·km)
- Photon energy
- 2.11001 eV
ε = (n + ik)², α = 4πk/λ, ng = n − λ dn/dλ, GVD = λ³/(2πc²) d²n/dλ², D = −(λ/c) d²n/dλ². Group-velocity dispersion is given for formula data only.
Use it in Lightsmith
Load this data in Python, simulate in one more line
pip install lightsmith
import lightsmith as ls
# MgAl2O4 (Magnesium aluminate, spinel): Chernova et al. 2017: n,k 0.14–1.67 µm
mgal2o4 = ls.fetch_refractiveindex("main", "MgAl2O4", "Chernova", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(mgal2o4.range_nm) # (140.89, 1675.5) nm
eps = mgal2o4.eps([633]) # complex permittivity
Downloads the original record once (pinned to the imported snapshot) and caches it.
import json, urllib.request
import lightsmith as ls
url = "https://materials.lightsmith.dev/v1/datasets/ds_16125bb87170/lightsmith"
mgal2o4 = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(mgal2o4.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (mgal2o4/chernova-2017).
# ... load mgal2o4 as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=mgal2o4)],
medium_index=1.0,
wavelengths=ls.WavelengthRange(start_nm=400, stop_nm=1000, num=81),
)
res = ls.solve(sim) # exact Mie for a sphere
print(res.q_ext) # extinction efficiency at each wavelength
Same spec runs with DDA, FDTD, BEM or T-matrix: ls.compare(sim, ["mie", "dda"]).
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.
Comments and conditions
References
[Calculation script (Python)]
- doi:10.1364/ome.7.003844 Optical NIR-VIS-VUV constants of advanced substrates for thin-film devices, Optical Materials Express (2017)
Cite
E. Chernova et al.. Optical NIR-VIS-VUV constants of advanced substrates for thin-film devices. Optical Materials Express, 7, 3844 (2017), doi:10.1364/ome.7.003844; [Calculation script (Python)]; Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)
Data
100 rows as published| λ (µm) | n | k |
|---|---|---|
| 0.14089 | 2.22 | 0.51961 |
| 0.14221 | 2.2003 | 0.48161 |
| 0.14355 | 2.1714 | 0.46322 |
| 0.14491 | 2.1465 | 0.47182 |
| 0.14631 | 2.1462 | 0.50377 |
| 0.14772 | 2.1862 | 0.53757 |
| 0.14917 | 2.2613 | 0.54317 |
| 0.15065 | 2.3458 | 0.50233 |
| 0.15215 | 2.4095 | 0.41915 |
| 0.15369 | 2.4339 | 0.31448 |
| 0.15525 | 2.4177 | 0.21304 |
| 0.15685 | 2.3731 | 0.13226 |
| 0.15849 | 2.3165 | 0.07771 |
| 0.16015 | 2.2608 | 0.04545 |
| 0.16185 | 2.2124 | 0.027789 |
| 0.16359 | 2.172 | 0.01804 |
| 0.16537 | 2.1382 | 0.012211 |
| 0.16719 | 2.1093 | 0.008384 |
| 0.16904 | 2.0841 | 0.0057324 |
| 0.17094 | 2.0618 | 0.0038702 |
| 0.17288 | 2.0418 | 0.0025726 |
| 0.17486 | 2.0236 | 0.0016825 |
| 0.1769 | 2.0071 | 0.0010825 |
| 0.17897 | 1.992 | 0.00068534 |
| 0.1811 | 1.978 | 0.00042726 |
| 0.18328 | 1.9651 | 0.00026218 |
| 0.18552 | 1.9531 | 0.00015838 |
| 0.1878 | 1.9418 | 9.4211e-05 |
| 0.19015 | 1.9313 | 5.5207e-05 |
| 0.19255 | 1.9214 | 3.1888e-05 |
| 0.19502 | 1.912 | 1.817e-05 |
| 0.19755 | 1.9032 | 1.0228e-05 |
| 0.20014 | 1.8948 | 5.6987e-06 |
| 0.20281 | 1.8868 | 3.1531e-06 |
| 0.20555 | 1.8792 | 1.7427e-06 |
| 0.20836 | 1.8719 | 9.6734e-07 |
| 0.21125 | 1.865 | 5.4426e-07 |
| 0.21422 | 1.8583 | 3.1397e-07 |
| 0.21728 | 1.8519 | 1.88e-07 |
| 0.22042 | 1.8458 | 1.1804e-07 |
| 0.22366 | 1.84 | 7.809e-08 |
| 0.22699 | 1.8343 | 5.4302e-08 |
| 0.23043 | 1.8289 | 3.9374e-08 |
| 0.23397 | 1.8237 | 2.9459e-08 |
| 0.23762 | 1.8187 | 2.2523e-08 |
| 0.24139 | 1.8138 | 1.7451e-08 |
| 0.24527 | 1.8091 | 1.3624e-08 |
| 0.24929 | 1.8046 | 1.0679e-08 |
| 0.25344 | 1.8003 | 8.3835e-09 |
| 0.25773 | 1.796 | 6.5831e-09 |
| 0.26216 | 1.792 | 5.1662e-09 |
| 0.26675 | 1.788 | 4.0499e-09 |
| 0.27151 | 1.7842 | 3.1706e-09 |
| 0.27644 | 1.7806 | 2.4785e-09 |
| 0.28155 | 1.777 | 1.9348e-09 |
| 0.28685 | 1.7736 | 1.5081e-09 |
| 0.29236 | 1.7702 | 1.1735e-09 |
| 0.29808 | 1.767 | 9.1171e-10 |
| 0.30403 | 1.7639 | 7.0715e-10 |
| 0.31023 | 1.7609 | 5.4759e-10 |
| 0.31668 | 1.758 | 4.2334e-10 |
| 0.3234 | 1.7551 | 3.2674e-10 |
| 0.33042 | 1.7524 | 2.5177e-10 |
| 0.33775 | 1.7498 | 1.9369e-10 |
| 0.34541 | 1.7472 | 1.4879e-10 |
| 0.35342 | 1.7447 | 1.1412e-10 |
| 0.36182 | 1.7423 | 8.7388e-11 |
| 0.37063 | 1.74 | 6.6808e-11 |
| 0.37987 | 1.7378 | 5.0991e-11 |
| 0.38959 | 1.7356 | 3.8855e-11 |
| 0.39982 | 1.7335 | 2.956e-11 |
| 0.4106 | 1.7315 | 2.2451e-11 |
| 0.42198 | 1.7295 | 1.7024e-11 |
| 0.434 | 1.7277 | 1.2888e-11 |
| 0.44673 | 1.7259 | 9.7427e-12 |
| 0.46023 | 1.7241 | 7.354e-12 |
| 0.47458 | 1.7224 | 5.5419e-12 |
| 0.48984 | 1.7208 | 4.1695e-12 |
| 0.50612 | 1.7192 | 3.1318e-12 |
| 0.52352 | 1.7177 | 2.3486e-12 |
| 0.54216 | 1.7163 | 1.7584e-12 |
| 0.56217 | 1.7149 | 1.3143e-12 |
| 0.58372 | 1.7136 | 9.8083e-13 |
| 0.60698 | 1.7123 | 7.3076e-13 |
| 0.63218 | 1.7111 | 5.4364e-13 |
| 0.65956 | 1.7099 | 4.0386e-13 |
| 0.68942 | 1.7088 | 2.9953e-13 |
| 0.72211 | 1.7078 | 2.2179e-13 |
| 0.75806 | 1.7068 | 1.6396e-13 |
| 0.79777 | 1.7058 | 1.2101e-13 |
| 0.84187 | 1.7049 | 8.9167e-14 |
| 0.89113 | 1.7041 | 6.5595e-14 |
| 0.94652 | 1.7033 | 4.8176e-14 |
| 1.0092 | 1.7026 | 3.5325e-14 |
| 1.0809 | 1.7019 | 2.5862e-14 |
| 1.1635 | 1.7012 | 1.8908e-14 |
| 1.2597 | 1.7006 | 1.38e-14 |
| 1.3733 | 1.7001 | 1.0054e-14 |
| 1.5094 | 1.6996 | 7.3113e-15 |
| 1.6755 | 1.6991 | 5.305e-15 |
Optical transmission calculator
Free-standing sample in vacuum, normal incidence- Transmittance T
- —
- Reflectance R
- —
Fresnel reflection calculator
- Rp
- —
- Rs
- —
- R = (Rp+Rs)/2
- —
- Phase φp
- —
- Phase φs
- —
- Brewster angle θB
- —
- Critical angle θC
- —
MgAl2O4, magnesium aluminate spinel (MAS)