Optical constants
Refractive index of Pb (Lead)
Ordal et al. 1987: n,k 0.667–667 µm
- Data
- tabulated nk
- Range
- 0.667–667 µm
- Points
- 52
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 39.8
- Extinction coefficient k
- 53.85
- Permittivity ε1
- -1315.78
- Permittivity ε2
- 4286.46
- Absorption coefficient α
- 320710 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 62.3615 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 1.27273 µm⁻¹
- Group index ng
- 12.9455
- Group velocity dispersion
- — fs²/mm
- Dispersion parameter D
- — ps/(nm·km)
- Photon energy
- 0.0587603 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
# Pb (Lead): Ordal et al. 1987: n,k 0.667–667 µm
pb = ls.fetch_refractiveindex("main", "Pb", "Ordal", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(pb.range_nm) # (667, 667000) nm
eps = pb.eps([21100]) # 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_24753cdd7089/lightsmith"
pb = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(pb.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (pb/ordal-1987).
# ... load pb as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=pb)],
medium_index=1.0,
wavelengths=ls.WavelengthRange(start_nm=667, 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
- doi:10.1364/ao.26.000744 Optical properties of Au, Ni, and Pb at submillimeter wavelengths, Applied Optics (1987)
Cite
Mark A. Ordal, Robert J. Bell, Ralph W. Alexander, Larry L. Long and Marvin R. Querry. Optical properties of Au, Ni, and Pb at submillimeter wavelengths. Applied Optics, 26, 744 (1987), doi:10.1364/ao.26.000744; Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)
Data
52 rows as published| λ (µm) | n | k |
|---|---|---|
| 0.667 | 1.88 | 3.49 |
| 0.714 | 1.74 | 3.58 |
| 0.769 | 1.55 | 3.85 |
| 0.833 | 1.46 | 4.25 |
| 0.909 | 1.39 | 4.7 |
| 1.0 | 1.36 | 5.26 |
| 1.05 | 1.35 | 5.58 |
| 1.11 | 1.36 | 5.94 |
| 1.18 | 1.38 | 6.35 |
| 1.25 | 1.42 | 6.8 |
| 1.33 | 1.48 | 7.31 |
| 1.43 | 1.57 | 7.88 |
| 1.54 | 1.69 | 8.53 |
| 1.67 | 1.85 | 9.27 |
| 1.82 | 2.04 | 10.1 |
| 2.0 | 2.31 | 11.2 |
| 2.11 | 2.49 | 11.7 |
| 2.22 | 2.7 | 12.4 |
| 2.35 | 2.98 | 13.1 |
| 2.5 | 3.18 | 13.8 |
| 2.67 | 3.58 | 14.7 |
| 2.86 | 3.94 | 15.6 |
| 3.08 | 4.39 | 16.7 |
| 3.33 | 5.01 | 17.9 |
| 3.64 | 5.72 | 19.2 |
| 4.0 | 6.54 | 20.7 |
| 4.44 | 7.58 | 22.6 |
| 5.0 | 9.02 | 24.8 |
| 5.71 | 11.0 | 27.2 |
| 6.67 | 13.5 | 30.1 |
| 8.0 | 16.6 | 33.7 |
| 10.0 | 21.4 | 38.1 |
| 11.1 | 23.8 | 40.1 |
| 12.5 | 26.5 | 42.6 |
| 14.3 | 30.0 | 45.3 |
| 16.7 | 33.9 | 48.3 |
| 20.0 | 38.4 | 52.5 |
| 22.2 | 41.2 | 55.2 |
| 25.0 | 44.7 | 58.5 |
| 28.6 | 49.0 | 62.5 |
| 33.3 | 54.5 | 67.1 |
| 40.0 | 61.4 | 72.7 |
| 44.4 | 65.5 | 76.1 |
| 50.0 | 70.2 | 80.0 |
| 57.1 | 75.5 | 84.6 |
| 66.7 | 81.8 | 90.6 |
| 80.0 | 89.5 | 98.7 |
| 100.0 | 99.5 | 111.0 |
| 133.0 | 114.0 | 129.0 |
| 200.0 | 141.0 | 164.0 |
| 400.0 | 211.0 | 244.0 |
| 667.0 | 289.0 | 319.0 |
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
- —