Optical constants
Refractive index of PtSe2 (Platinum diselenide)
Tharrault et al. 2025: 5L film; n,k 0.416–1.55 µm
- Data
- tabulated nk
- Range
- 0.416–1.55 µm
- Points
- 109
- State
- crystalline
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 4.47671
- Extinction coefficient k
- 2.93588
- Permittivity ε1
- 11.4216
- Permittivity ε2
- 26.2862
- Absorption coefficient α
- 627865 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 31.854 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 3.39856 µm⁻¹
- Group index ng
- 2.47972
- 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
# PtSe2 (Platinum diselenide): Tharrault et al. 2025: 5L film; n,k 0.416–1.55 µm
ptse2 = ls.fetch_refractiveindex("main", "PtSe2", "Tharrault-5L", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(ptse2.range_nm) # (416.05, 1550.38) nm
eps = ptse2.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_c35ed2046e56/lightsmith"
ptse2 = ls.Tabulated.model_validate(json.load(urllib.request.urlopen(url)))
print(ptse2.source) # citation and provenance travel with the data
Any dataset here, as the library's Tabulated material (ptse2/tharrault-2025-5l).
# ... load ptse2 as above, then:
sim = ls.Simulation(
particles=[ls.Particle(shape=ls.Sphere(radius_nm=50), material=ptse2)],
medium_index=1.0,
wavelengths=ls.WavelengthRange(start_nm=417, 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
- doi:10.1103/physrevlett.134.066901 Optical Absorption in Indirect Semiconductor to Semimetal <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>PtSe</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> </mml:math> Arises from Direct Transitions, Physical Review Letters (2025)
Cite
Marin Tharrault et al.. Optical Absorption in Indirect Semiconductor to Semimetal <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>PtSe</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msub> </mml:mrow> </mml:math> Arises from Direct Transitions. Physical Review Letters, 134, 066901 (2025), doi:10.1103/physrevlett.134.066901; Data from the refractiveindex.info database (M. N. Polyanskiy, Sci. Data 11, 94 (2024), doi:10.1038/s41597-023-02898-2)
Data
109 rows as published| λ (µm) | n | k |
|---|---|---|
| 0.41605 | 4.15814 | 2.14296 |
| 0.41887 | 4.14164 | 2.18119 |
| 0.42171 | 4.1451 | 2.2107 |
| 0.4246 | 4.15398 | 2.22651 |
| 0.42753 | 4.14857 | 2.26087 |
| 0.4305 | 4.15152 | 2.29113 |
| 0.43351 | 4.19519 | 2.29475 |
| 0.43656 | 4.20554 | 2.3104 |
| 0.43966 | 4.20829 | 2.33342 |
| 0.4428 | 4.23177 | 2.34194 |
| 0.44599 | 4.23976 | 2.36419 |
| 0.44922 | 4.2375 | 2.39517 |
| 0.4525 | 4.23888 | 2.42386 |
| 0.45582 | 4.25498 | 2.4398 |
| 0.4592 | 4.29667 | 2.43002 |
| 0.46263 | 4.30936 | 2.4453 |
| 0.46611 | 4.3069 | 2.4705 |
| 0.46964 | 4.30929 | 2.49191 |
| 0.47322 | 4.3138 | 2.51002 |
| 0.47686 | 4.33236 | 2.51506 |
| 0.48056 | 4.33487 | 2.52963 |
| 0.48431 | 4.33319 | 2.54724 |
| 0.48813 | 4.33218 | 2.56438 |
| 0.492 | 4.34265 | 2.56648 |
| 0.49594 | 4.33928 | 2.58225 |
| 0.49994 | 4.36452 | 2.58551 |
| 0.504 | 4.3562 | 2.60574 |
| 0.50813 | 4.33913 | 2.63487 |
| 0.51233 | 4.3431 | 2.64906 |
| 0.5166 | 4.33993 | 2.66863 |
| 0.52094 | 4.34494 | 2.68534 |
| 0.52536 | 4.34747 | 2.70237 |
| 0.52985 | 4.34282 | 2.7299 |
| 0.53441 | 4.34055 | 2.75181 |
| 0.53906 | 4.35792 | 2.75927 |
| 0.54379 | 4.35373 | 2.79122 |
| 0.5486 | 4.36066 | 2.81576 |
| 0.5535 | 4.3626 | 2.84241 |
| 0.55849 | 4.36904 | 2.86698 |
| 0.56356 | 4.39225 | 2.87135 |
| 0.56873 | 4.41793 | 2.88406 |
| 0.574 | 4.44341 | 2.89367 |
| 0.57937 | 4.46665 | 2.89823 |
| 0.58483 | 4.4673 | 2.92964 |
| 0.5904 | 4.48623 | 2.94219 |
| 0.59608 | 4.50605 | 2.96278 |
| 0.60187 | 4.54368 | 2.96677 |
| 0.60777 | 4.59715 | 2.94987 |
| 0.61378 | 4.5919 | 2.99542 |
| 0.61992 | 4.63072 | 2.99583 |
| 0.62618 | 4.64341 | 3.0233 |
| 0.63257 | 4.62623 | 3.08597 |
| 0.63909 | 4.67712 | 3.08301 |
| 0.64575 | 4.70144 | 3.10972 |
| 0.65255 | 4.7503 | 3.10885 |
| 0.65949 | 4.75748 | 3.13761 |
| 0.66658 | 4.71269 | 3.20414 |
| 0.67383 | 4.75487 | 3.20183 |
| 0.68123 | 4.77395 | 3.22185 |
| 0.6888 | 4.82925 | 3.19631 |
| 0.69654 | 4.85601 | 3.20322 |
| 0.70446 | 4.88975 | 3.20513 |
| 0.71255 | 4.89442 | 3.25841 |
| 0.72084 | 4.9432 | 3.28016 |
| 0.72932 | 5.02567 | 3.27923 |
| 0.738 | 5.08414 | 3.31227 |
| 0.74689 | 5.17354 | 3.33029 |
| 0.756 | 5.24839 | 3.36779 |
| 0.76533 | 5.36414 | 3.36473 |
| 0.7749 | 5.46401 | 3.36754 |
| 0.78471 | 5.59785 | 3.32426 |
| 0.79477 | 5.69788 | 3.28731 |
| 0.80509 | 5.78372 | 3.24235 |
| 0.81569 | 5.88973 | 3.14852 |
| 0.82656 | 5.97449 | 3.06493 |
| 0.83773 | 6.05893 | 2.95088 |
| 0.84921 | 6.13702 | 2.83146 |
| 0.861 | 6.22275 | 2.68832 |
| 0.87313 | 6.26451 | 2.58361 |
| 0.8856 | 6.31324 | 2.44752 |
| 0.89844 | 6.33859 | 2.34345 |
| 0.91165 | 6.3357 | 2.24339 |
| 0.92526 | 6.34793 | 2.12784 |
| 0.93927 | 6.3184 | 2.05234 |
| 0.95372 | 6.30072 | 1.95373 |
| 0.96863 | 6.26963 | 1.87645 |
| 0.984 | 6.26954 | 1.76814 |
| 0.99987 | 6.25224 | 1.67237 |
| 1.01626 | 6.28977 | 1.52729 |
| 1.0332 | 6.28074 | 1.48362 |
| 1.06883 | 6.1947 | 1.19857 |
| 1.08758 | 6.25134 | 1.14883 |
| 1.107 | 6.23521 | 1.03718 |
| 1.12713 | 6.2008 | 0.95922 |
| 1.148 | 6.17345 | 0.87396 |
| 1.16966 | 6.15404 | 0.80488 |
| 1.19216 | 6.15291 | 0.73404 |
| 1.21553 | 6.12971 | 0.68815 |
| 1.24021 | 6.1024 | 0.66467 |
| 1.26553 | 6.05931 | 0.65243 |
| 1.29191 | 6.03145 | 0.61329 |
| 1.3194 | 5.97653 | 0.6084 |
| 1.34809 | 5.93948 | 0.59852 |
| 1.37806 | 5.96401 | 0.56994 |
| 1.40939 | 5.95849 | 0.53686 |
| 1.44218 | 5.90086 | 0.53244 |
| 1.47653 | 5.89315 | 0.50846 |
| 1.51256 | 5.92936 | 0.4665 |
| 1.55038 | 5.96016 | 0.43373 |
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
- —
5L CVT-grown exfoliated crystal. The optical indexes are computed from the 2D surface conductivity using σ2D·Z0 = −2πi·(t/λ)·(εr−1), where Z0 is the impedance of free space, i the imaginary unit, t the equivalent layered stack thickness and λ the free space wavelength. We use t = NL t0 with t0 = 5.1 Å the single layer thickness. The measurement method accuratly determines Im{εr} = 2nk, but only Re{εr} = n2 - k2 as long as the optical absorption is non-zero.