Optical constants
Refractive index of Cu (Copper)
Hagemann et al. 1974: n,k 0.0000248–248 µm
- Data
- tabulated nk
- Range
- 2.48e-05–248 µm
- Points
- 149
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 0.505403
- Extinction coefficient k
- 2.78806
- Permittivity ε1
- -7.51784
- Permittivity ε2
- 2.81819
- Absorption coefficient α
- 596252 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 33.5428 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- -13.3582 µm⁻¹
- Group index ng
- 8.35469
- 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
# Cu (Copper): Hagemann et al. 1974: n,k 0.0000248–248 µm
cu = ls.fetch_refractiveindex("main", "Cu", "Hagemann", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(cu.range_nm) # (0.0248, 248000) nm
eps = cu.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_b2c5a3c0ff79/lightsmith"
cu = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(cu.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (cu/hagemann-1974).
# ... load cu as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=cu)],
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.
References
2) H.-J. Hagemann, W. Gudat, C. Kunz. DESY report SR-74/7 (1974)
- doi:10.1364/josa.65.000742 Optical constants from the far infrared to the x-ray region: Mg, Al, Cu, Ag, Au, Bi, C, and Al_2O_3, Journal of the Optical Society of America (1975)
Cite
H.-J. Hagemann, W. Gudat and C. Kunz. Optical constants from the far infrared to the x-ray region: Mg, Al, Cu, Ag, Au, Bi, C, and Al_2O_3. Journal of the Optical Society of America, 65, 742 (1975), doi:10.1364/josa.65.000742; H.-J. Hagemann, W. Gudat, C. Kunz. DESY report SR-74/7 (1974); Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)
Data
149 rows as published| λ (µm) | n | k |
|---|---|---|
| 2.48e-05 | 1.0 | 4.45e-09 |
| 4.133e-05 | 1.0 | 3.09e-08 |
| 8.266e-05 | 1.0 | 4.06e-07 |
| 0.0001378 | 1.001 | 3.65e-07 |
| 0.0001393 | 1.001 | 3.56e-07 |
| 0.000155 | 1.001 | 5.38e-07 |
| 0.00031 | 1.0 | 6.62e-06 |
| 0.0006199 | 1.0 | 9.49e-05 |
| 0.0008266 | 1.0 | 0.000273 |
| 0.001033 | 0.999 | 0.000624 |
| 0.001127 | 0.999 | 0.000823 |
| 0.00124 | 0.999 | 0.000851 |
| 0.001378 | 1.0 | 0.000174 |
| 0.00155 | 0.999 | 0.000263 |
| 0.001771 | 0.998 | 0.000395 |
| 0.002066 | 0.997 | 0.000651 |
| 0.00248 | 0.997 | 0.00111 |
| 0.0031 | 0.993 | 0.00245 |
| 0.004133 | 0.988 | 0.00513 |
| 0.006199 | 0.978 | 0.0159 |
| 0.008266 | 0.969 | 0.031 |
| 0.01033 | 0.965 | 0.054 |
| 0.01127 | 0.968 | 0.0599 |
| 0.01181 | 0.968 | 0.0625 |
| 0.0124 | 0.967 | 0.0653 |
| 0.01305 | 0.965 | 0.0693 |
| 0.01348 | 0.963 | 0.0744 |
| 0.01378 | 0.963 | 0.0788 |
| 0.01409 | 0.963 | 0.0834 |
| 0.01442 | 0.966 | 0.0877 |
| 0.01476 | 0.969 | 0.0911 |
| 0.01494 | 0.971 | 0.0923 |
| 0.01512 | 0.973 | 0.0934 |
| 0.01531 | 0.974 | 0.0943 |
| 0.0155 | 0.977 | 0.0946 |
| 0.01569 | 0.979 | 0.0941 |
| 0.0159 | 0.98 | 0.0936 |
| 0.0161 | 0.982 | 0.0921 |
| 0.01631 | 0.984 | 0.091 |
| 0.01653 | 0.983 | 0.0872 |
| 0.01675 | 0.979 | 0.085 |
| 0.01698 | 0.977 | 0.0857 |
| 0.01722 | 0.975 | 0.0868 |
| 0.01746 | 0.974 | 0.0881 |
| 0.01771 | 0.972 | 0.0893 |
| 0.01797 | 0.97 | 0.0908 |
| 0.01823 | 0.968 | 0.0927 |
| 0.01851 | 0.968 | 0.0945 |
| 0.01879 | 0.967 | 0.0963 |
| 0.01907 | 0.966 | 0.099 |
| 0.01937 | 0.965 | 0.102 |
| 0.01968 | 0.965 | 0.104 |
| 0.02 | 0.965 | 0.107 |
| 0.02033 | 0.966 | 0.108 |
| 0.02066 | 0.966 | 0.109 |
| 0.02101 | 0.966 | 0.109 |
| 0.02138 | 0.964 | 0.11 |
| 0.02175 | 0.962 | 0.112 |
| 0.02214 | 0.96 | 0.114 |
| 0.02254 | 0.958 | 0.117 |
| 0.02296 | 0.957 | 0.12 |
| 0.02339 | 0.956 | 0.123 |
| 0.02384 | 0.954 | 0.126 |
| 0.02431 | 0.953 | 0.13 |
| 0.0248 | 0.953 | 0.134 |
| 0.0253 | 0.952 | 0.137 |
| 0.02583 | 0.952 | 0.14 |
| 0.02638 | 0.951 | 0.143 |
| 0.02695 | 0.951 | 0.146 |
| 0.02755 | 0.949 | 0.148 |
| 0.02818 | 0.948 | 0.151 |
| 0.02883 | 0.945 | 0.154 |
| 0.02952 | 0.942 | 0.157 |
| 0.03024 | 0.938 | 0.161 |
| 0.031 | 0.934 | 0.167 |
| 0.03179 | 0.93 | 0.174 |
| 0.03263 | 0.927 | 0.18 |
| 0.03351 | 0.925 | 0.187 |
| 0.03444 | 0.922 | 0.193 |
| 0.03542 | 0.917 | 0.198 |
| 0.03647 | 0.91 | 0.205 |
| 0.03757 | 0.901 | 0.214 |
| 0.03875 | 0.891 | 0.223 |
| 0.03999 | 0.876 | 0.239 |
| 0.04133 | 0.856 | 0.262 |
| 0.04275 | 0.849 | 0.302 |
| 0.04428 | 0.862 | 0.346 |
| 0.04592 | 0.884 | 0.382 |
| 0.04769 | 0.921 | 0.403 |
| 0.04959 | 0.96 | 0.396 |
| 0.05166 | 0.961 | 0.373 |
| 0.05391 | 0.943 | 0.366 |
| 0.05636 | 0.917 | 0.381 |
| 0.05904 | 0.897 | 0.411 |
| 0.06199 | 0.882 | 0.455 |
| 0.06525 | 0.883 | 0.507 |
| 0.06888 | 0.89 | 0.561 |
| 0.07293 | 0.913 | 0.62 |
| 0.07749 | 0.954 | 0.673 |
| 0.07999 | 0.981 | 0.695 |
| 0.08266 | 1.009 | 0.707 |
| 0.08551 | 1.034 | 0.717 |
| 0.08856 | 1.055 | 0.724 |
| 0.09537 | 1.084 | 0.724 |
| 0.1033 | 1.091 | 0.713 |
| 0.1127 | 1.074 | 0.754 |
| 0.124 | 1.038 | 0.818 |
| 0.1305 | 1.029 | 0.867 |
| 0.1378 | 1.027 | 0.921 |
| 0.1459 | 1.029 | 0.979 |
| 0.155 | 1.029 | 1.03 |
| 0.1653 | 1.005 | 1.09 |
| 0.1771 | 0.972 | 1.2 |
| 0.1907 | 0.958 | 1.37 |
| 0.2066 | 1.036 | 1.59 |
| 0.2138 | 1.102 | 1.67 |
| 0.2214 | 1.183 | 1.74 |
| 0.2296 | 1.276 | 1.78 |
| 0.2384 | 1.378 | 1.8 |
| 0.248 | 1.47 | 1.78 |
| 0.2583 | 1.533 | 1.71 |
| 0.2695 | 1.52 | 1.67 |
| 0.2818 | 1.487 | 1.64 |
| 0.2952 | 1.419 | 1.64 |
| 0.31 | 1.344 | 1.72 |
| 0.3263 | 1.336 | 1.81 |
| 0.3444 | 1.31 | 1.87 |
| 0.3647 | 1.27 | 1.95 |
| 0.3875 | 1.232 | 2.07 |
| 0.4133 | 1.184 | 2.21 |
| 0.4428 | 1.169 | 2.36 |
| 0.4769 | 1.152 | 2.5 |
| 0.5166 | 1.121 | 2.6 |
| 0.5391 | 1.037 | 2.59 |
| 0.5636 | 0.826 | 2.6 |
| 0.5904 | 0.468 | 2.81 |
| 0.6199 | 0.272 | 3.24 |
| 0.6525 | 0.214 | 3.67 |
| 0.6702 | 0.215 | 3.86 |
| 0.6888 | 0.213 | 4.05 |
| 0.7085 | 0.214 | 4.24 |
| 0.7293 | 0.223 | 4.43 |
| 0.8266 | 0.26 | 5.26 |
| 1.24 | 0.433 | 8.46 |
| 2.48 | 1.692 | 17.6 |
| 12.4 | 29.1 | 71.1 |
| 24.8 | 62.8 | 103.0 |
| 124.0 | 186.0 | 213.0 |
| 248.0 | 270.0 | 294.0 |
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
- —