Optical constants
Refractive index of Au (Gold)
Hagemann et al. 1974: n,k 0.000008266–248 µm
- Data
- tabulated nk
- Range
- 8.266e-06–248 µm
- Points
- 149
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 0.559288
- Extinction coefficient k
- 2.92561
- Permittivity ε1
- -8.24641
- Permittivity ε2
- 3.27252
- Absorption coefficient α
- 625669 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 31.9658 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- -2.23801 µm⁻¹
- Group index ng
- 1.87434
- 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
# Au (Gold): Hagemann et al. 1974: n,k 0.000008266–248 µm
au = ls.fetch_refractiveindex("main", "Au", "Hagemann", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(au.range_nm) # (0.008266, 248000) nm
eps = au.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_5b94071a5b82/lightsmith"
au = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(au.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (au/hagemann-1974).
# ... load au as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=au)],
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 |
|---|---|---|
| 8.266e-06 | 1.0 | 2.56e-09 |
| 1.494e-05 | 1.002 | 1.95e-08 |
| 1.55e-05 | 1.0 | 5.22e-09 |
| 2.48e-05 | 1.0 | 3.05e-08 |
| 4.133e-05 | 1.0 | 1.85e-07 |
| 6.199e-05 | 1.0 | 8.83e-07 |
| 8.266e-05 | 1.0 | 2.28e-06 |
| 8.856e-05 | 1.001 | 1.94e-06 |
| 9.537e-05 | 1.001 | 2.56e-06 |
| 0.000124 | 1.0 | 2.53e-06 |
| 0.000248 | 1.001 | 2.87e-05 |
| 0.0004275 | 0.999 | 0.000164 |
| 0.000435 | 0.999 | 0.000145 |
| 0.0004959 | 1.0 | 0.000211 |
| 0.0006199 | 1.0 | 0.00012 |
| 0.00124 | 0.998 | 0.00096 |
| 0.00155 | 0.997 | 0.00163 |
| 0.002066 | 0.996 | 0.0034 |
| 0.00248 | 0.995 | 0.00471 |
| 0.003542 | 0.992 | 0.00731 |
| 0.004133 | 0.991 | 0.00895 |
| 0.004428 | 0.989 | 0.00976 |
| 0.004769 | 0.988 | 0.0106 |
| 0.005166 | 0.987 | 0.0113 |
| 0.005636 | 0.986 | 0.0118 |
| 0.006199 | 0.983 | 0.0115 |
| 0.006525 | 0.981 | 0.0111 |
| 0.006888 | 0.979 | 0.0107 |
| 0.007293 | 0.975 | 0.0103 |
| 0.007749 | 0.97 | 0.0101 |
| 0.008266 | 0.963 | 0.0101 |
| 0.008856 | 0.955 | 0.0109 |
| 0.009184 | 0.949 | 0.0118 |
| 0.009537 | 0.944 | 0.0133 |
| 0.009919 | 0.937 | 0.0152 |
| 0.01033 | 0.929 | 0.0178 |
| 0.01078 | 0.92 | 0.0224 |
| 0.01127 | 0.911 | 0.0283 |
| 0.01181 | 0.9 | 0.0353 |
| 0.0124 | 0.889 | 0.0454 |
| 0.01305 | 0.877 | 0.057 |
| 0.01333 | 0.872 | 0.0636 |
| 0.01362 | 0.868 | 0.0718 |
| 0.01393 | 0.865 | 0.0807 |
| 0.01409 | 0.866 | 0.0838 |
| 0.01417 | 0.865 | 0.0844 |
| 0.01425 | 0.863 | 0.087 |
| 0.01442 | 0.862 | 0.0918 |
| 0.01459 | 0.864 | 0.0956 |
| 0.01467 | 0.865 | 0.0962 |
| 0.01476 | 0.865 | 0.0938 |
| 0.01485 | 0.861 | 0.0943 |
| 0.01494 | 0.86 | 0.0963 |
| 0.01512 | 0.857 | 0.101 |
| 0.0155 | 0.853 | 0.109 |
| 0.0159 | 0.85 | 0.117 |
| 0.01631 | 0.847 | 0.124 |
| 0.01675 | 0.842 | 0.131 |
| 0.01722 | 0.835 | 0.14 |
| 0.01771 | 0.828 | 0.155 |
| 0.01823 | 0.827 | 0.171 |
| 0.01879 | 0.828 | 0.186 |
| 0.01937 | 0.83 | 0.199 |
| 0.02 | 0.833 | 0.211 |
| 0.02066 | 0.838 | 0.219 |
| 0.02138 | 0.836 | 0.223 |
| 0.02214 | 0.83 | 0.23 |
| 0.02296 | 0.82 | 0.241 |
| 0.02384 | 0.808 | 0.255 |
| 0.0248 | 0.795 | 0.272 |
| 0.0253 | 0.787 | 0.284 |
| 0.02583 | 0.778 | 0.298 |
| 0.02638 | 0.771 | 0.315 |
| 0.02695 | 0.767 | 0.335 |
| 0.02755 | 0.767 | 0.355 |
| 0.02818 | 0.77 | 0.371 |
| 0.02883 | 0.77 | 0.384 |
| 0.02952 | 0.766 | 0.398 |
| 0.03024 | 0.76 | 0.415 |
| 0.031 | 0.754 | 0.438 |
| 0.03179 | 0.751 | 0.461 |
| 0.03263 | 0.749 | 0.484 |
| 0.03351 | 0.745 | 0.511 |
| 0.03444 | 0.741 | 0.54 |
| 0.03542 | 0.737 | 0.573 |
| 0.03647 | 0.73 | 0.617 |
| 0.03757 | 0.73 | 0.672 |
| 0.03875 | 0.757 | 0.747 |
| 0.03999 | 0.818 | 0.788 |
| 0.04065 | 0.844 | 0.799 |
| 0.04133 | 0.868 | 0.804 |
| 0.04203 | 0.887 | 0.803 |
| 0.04275 | 0.896 | 0.802 |
| 0.04428 | 0.892 | 0.814 |
| 0.04592 | 0.885 | 0.855 |
| 0.04769 | 0.886 | 0.917 |
| 0.04959 | 0.905 | 1.0 |
| 0.05166 | 0.953 | 1.12 |
| 0.05276 | 1.005 | 1.18 |
| 0.05391 | 1.08 | 1.24 |
| 0.0551 | 1.183 | 1.28 |
| 0.05636 | 1.292 | 1.29 |
| 0.05767 | 1.406 | 1.27 |
| 0.05904 | 1.499 | 1.21 |
| 0.06199 | 1.584 | 1.07 |
| 0.06525 | 1.612 | 0.95 |
| 0.06888 | 1.565 | 0.865 |
| 0.07293 | 1.513 | 0.865 |
| 0.07749 | 1.505 | 0.898 |
| 0.08266 | 1.54 | 0.934 |
| 0.08856 | 1.591 | 0.922 |
| 0.09537 | 1.592 | 0.899 |
| 0.1033 | 1.583 | 0.908 |
| 0.1078 | 1.569 | 0.92 |
| 0.1127 | 1.556 | 0.945 |
| 0.1181 | 1.548 | 0.99 |
| 0.124 | 1.572 | 1.05 |
| 0.1305 | 1.585 | 1.07 |
| 0.1378 | 1.614 | 1.14 |
| 0.1459 | 1.666 | 1.17 |
| 0.155 | 1.727 | 1.22 |
| 0.1653 | 1.786 | 1.15 |
| 0.1771 | 1.728 | 1.13 |
| 0.1907 | 1.665 | 1.19 |
| 0.2066 | 1.618 | 1.3 |
| 0.2254 | 1.603 | 1.45 |
| 0.248 | 1.638 | 1.65 |
| 0.261 | 1.702 | 1.77 |
| 0.2818 | 1.848 | 1.87 |
| 0.2952 | 1.927 | 1.89 |
| 0.31 | 1.995 | 1.88 |
| 0.3263 | 2.039 | 1.86 |
| 0.3444 | 2.024 | 1.81 |
| 0.3594 | 1.967 | 1.84 |
| 0.3757 | 1.96 | 1.88 |
| 0.3936 | 1.96 | 1.89 |
| 0.4133 | 1.95 | 1.86 |
| 0.4428 | 1.862 | 1.81 |
| 0.4769 | 1.541 | 1.71 |
| 0.5166 | 0.878 | 2.01 |
| 0.5636 | 0.613 | 2.64 |
| 0.6199 | 0.487 | 3.31 |
| 0.8266 | 0.418 | 5.13 |
| 1.24 | 0.375 | 8.36 |
| 2.48 | 1.273 | 18.1 |
| 12.4 | 26.9 | 80.7 |
| 24.8 | 65.5 | 124.0 |
| 124.0 | 222.0 | 256.0 |
| 248.0 | 345.0 | 379.0 |
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
- —