Optical constants

Refractive index of Mo (Molybdenum)

Werner et al. 2009: n,k 0.01759–2.480 µm

Data: tabulated nk
Range: 0.01759–2.48 µm
Points: 150
Licence: CC0-1.0

Axis Log x Log y

Click the plot to set the calculator wavelength.

At one wavelength

Refractive index n: 0.69688
Extinction coefficient k: 8.06633

Permittivity ε₁: -64.58
Permittivity ε₂: 11.2425

Absorption coefficient α: 1.72506e+06 cm⁻¹
Penetration depth δ = λ/(2πk): 11.5938 nm

Abbe number V_d: —
Chromatic dispersion dn/dλ: 2.56243 µm⁻¹

Group index n_g: -0.808803
Group velocity dispersion: — fs²/mm

Dispersion parameter D: — ps/(nm·km)
Photon energy: 2.11001 eV

ε = (n + ik)², α = 4πk/λ, n_g = 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

# Mo (Molybdenum): Werner et al. 2009: n,k 0.01759–2.480 µm
mo = ls.fetch_refractiveindex("main", "Mo", "Werner", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(mo.range_nm)  # (17.586, 2479.68) nm
eps = mo.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_3e0e9aaed9af/lightsmith"
mo = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(mo.source)  # citation and provenance travel with the data

Any dataset here, as the library's Tabulated material (mo/werner-2009).

# ... load mo as above, then:
sim = ls.Simulation(
    particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=mo)],
    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"]).

Materials guide Open a sphere of it in Studio Quick start Ask the community

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

Experimental data: Derived from reflection electron energy-loss spectroscopy (REELS) spectra.

References

W. S. M. Werner, K. Glantschnig, C. Ambrosch-Draxl. Optical constants and inelastic electron-scattering data for 17 elemental metals. J. Phys Chem Ref. Data 38, 1013-1092 (2009)

doi:10.1063/1.3243762 Optical Constants and Inelastic Electron-Scattering Data for 17 Elemental Metals, Journal of Physical and Chemical Reference Data (2009)

Cite

Wolfgang S. M. Werner, Kathrin Glantschnig and Claudia Ambrosch-Draxl. Optical Constants and Inelastic Electron-Scattering Data for 17 Elemental Metals. Journal of Physical and Chemical Reference Data, 38, 1013-1092 (2009), doi:10.1063/1.3243762; Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)

Data

150 rows as published

CSV comma separated TXT tab separated YAML n, k Full database record original YAML All quantities CSV JSON metadata

Mo (Molybdenum), Werner et al. 2009: n,k 0.01759–2.480 µm: n and k versus wavelength
λ (µm)	n	k
0.017586	0.8525	0.0276
0.017712	0.8496	0.0288
0.017839	0.8467	0.0301
0.017969	0.8438	0.032
0.0181	0.8409	0.0333
0.018233	0.838	0.0346
0.018368	0.8345	0.0366
0.018505	0.8316	0.0385
0.018644	0.828	0.0405
0.018785	0.8245	0.0424
0.018929	0.821	0.0445
0.019074	0.8174	0.0471
0.019222	0.8139	0.0491
0.019373	0.8104	0.0518
0.019525	0.8068	0.0545
0.01968	0.8027	0.0573
0.019837	0.7992	0.0607
0.019997	0.7951	0.0641
0.02016	0.7909	0.067
0.020325	0.7874	0.0705
0.020493	0.7833	0.0747
0.020664	0.7792	0.0783
0.020838	0.7751	0.0826
0.021014	0.7704	0.087
0.021194	0.7664	0.0913
0.021377	0.7617	0.0958
0.021562	0.7565	0.1011
0.021752	0.7518	0.1057
0.021944	0.7467	0.1118
0.02214	0.7408	0.1174
0.022339	0.7352	0.1245
0.022543	0.7289	0.1317
0.022749	0.7223	0.1405
0.02296	0.7159	0.1502
0.023175	0.7099	0.1613
0.023393	0.7038	0.1741
0.023616	0.699	0.1888
0.023843	0.6965	0.2053
0.024075	0.6961	0.2227
0.024311	0.7	0.2407
0.024551	0.707	0.2567
0.024797	0.7166	0.2693
0.025047	0.7274	0.2777
0.025303	0.7354	0.2808
0.025564	0.7387	0.2823
0.02583	0.734	0.2841
0.026102	0.7198	0.2952
0.02638	0.7012	0.3444
0.026663	0.827	0.3604
0.026953	0.781	0.2932
0.027249	0.7504	0.3052
0.027552	0.7365	0.3279
0.027862	0.7341	0.3535
0.028178	0.7403	0.3782
0.028502	0.7529	0.3985
0.028834	0.7665	0.4129
0.029173	0.7767	0.4223
0.02952	0.7814	0.4332
0.029876	0.7824	0.4518
0.03024	0.7869	0.4829
0.030613	0.8073	0.5252
0.030996	0.854	0.565
0.031388	0.9236	0.5798
0.031791	0.9896	0.5553
0.032204	1.0208	0.5099
0.032627	1.0165	0.482
0.033062	1.0127	0.4996
0.033509	1.0726	0.5408
0.033968	1.189	0.4958
0.03444	1.2234	0.3711
0.034925	1.1744	0.2831
0.035424	1.0973	0.283
0.035937	1.2157	0.2682
0.036466	1.1363	0.165
0.03701	1.0768	0.1435
0.037571	1.0329	0.1341
0.038149	0.9959	0.1295
0.038745	0.963	0.1277
0.03936	0.932	0.1288
0.039995	0.9024	0.1313
0.040651	0.8737	0.1356
0.041328	0.8457	0.1419
0.042029	0.8183	0.1503
0.042753	0.7897	0.1602
0.043503	0.7615	0.1727
0.04428	0.7337	0.1881
0.045085	0.7054	0.2063
0.04592	0.6766	0.2276
0.046786	0.6494	0.2525
0.047686	0.6235	0.2823
0.048621	0.5995	0.3153
0.049594	0.5789	0.3524
0.050606	0.5621	0.3923
0.05166	0.5497	0.4338
0.052759	0.5419	0.4761
0.053906	0.5382	0.5184
0.055104	0.5369	0.5588
0.056356	0.5374	0.5982
0.057667	0.5388	0.6366
0.05904	0.5408	0.6749
0.06048	0.5417	0.7144
0.061992	0.5426	0.7566
0.063582	0.5454	0.8022
0.065255	0.5506	0.851
0.067018	0.5593	0.9038
0.06888	0.5745	0.9592
0.070848	0.5961	1.0166
0.072932	0.6261	1.0733
0.075142	0.6636	1.128
0.07749	0.7101	1.1774
0.07999	0.7626	1.2188
0.082656	0.8195	1.2496
0.085506	0.8751	1.2672
0.08856	0.9233	1.2737
0.09184	0.9566	1.2748
0.095372	0.9723	1.2862
0.099187	0.9907	1.3385
0.10332	1.1337	1.4196
0.107812	1.2876	1.1785
0.112713	1.098	1.0347
0.11808	0.9268	1.0644
0.123984	0.7987	1.1575
0.13051	0.7056	1.2876
0.13776	0.6453	1.4413
0.145864	0.6143	1.6101
0.15498	0.6097	1.7871
0.165312	0.6276	1.968
0.17712	0.663	2.1477
0.190745	0.7067	2.322
0.20664	0.7408	2.4911
0.225426	0.7408	2.6713
0.247968	0.6895	2.9028
0.261019	0.6467	3.0555
0.27552	0.5974	3.2414
0.291728	0.5472	3.4658
0.30996	0.5009	3.7324
0.330625	0.4625	4.0454
0.354241	0.4353	4.4099
0.38149	0.4219	4.8341
0.413281	0.4253	5.3305
0.450852	0.4501	5.9171
0.495937	0.5043	6.622
0.551041	0.6032	7.487
0.619921	0.7797	8.5785
0.708481	1.1106	10.0036
0.826561	1.8114	11.9264
0.991874	3.5874	14.3933
1.239842	7.4102	15.0566
1.653123	5.1146	13.818
2.479684	1.8025	23.8449

Optical transmission calculator

Free-standing sample in vacuum, normal incidence

Transmittance T: —
Reflectance R: —

Fresnel reflection calculator

R_p: —
R_s: —
R = (R_p+R_s)/2: —
Phase φ_p: —
Phase φ_s: —
Brewster angle θ_B: —
Critical angle θ_C: —

Mo (Molybdenum): all datasets

Experimental data

Models and simulations

Werner et al. 2009: DFT calculations; n,k 0.0176–2.48 µm n,k 0.01759–2.48 µm

About Mo (Molybdenum)

Molybdenum (Mo) is a silver-white, hard, transition metal. Known for its high melting points, strength, and resistance to corrosion, especially at high temperatures, it is invaluable in applications that demand materials capable of withstanding intense heat, such as in the production of furnace equipment and as filaments for light bulbs. In optics, molybdenum mirrors are favored for their robustness and durability, especially in high-power laser applications. The metal's reflective properties make it suitable for use as a coating for certain wavelengths, particularly in the deep ultraviolet spectral region.

More about Mo (Molybdenum) →

Provenance

Version: 1 (snapshot c5c2f18)
Source page: refractiveindex.info
Original file: database/data/main/Mo/nk/Werner.yml
ID: ds_3e0e9aaed9af
API: /v1/datasets/ds_3e0e9aaed9af

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