Optical constants
Refractive index of PtSe2 (Platinum diselenide)
Tharrault et al. 2025: 4L 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
- 4.52677
- Extinction coefficient k
- 2.96724
- Permittivity ε1
- 11.6872
- Permittivity ε2
- 26.864
- Absorption coefficient α
- 634571 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 31.5173 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 0.213645 µm⁻¹
- Group index ng
- 4.40123
- 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: 4L film; n,k 0.416–1.55 µm
ptse2 = ls.fetch_refractiveindex("main", "PtSe2", "Tharrault-4L", 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_852345059517/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-2025-4l).
# ... 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 | 4.13224 | 2.30274 |
| 0.41887 | 4.11479 | 2.34044 |
| 0.42171 | 4.11486 | 2.36312 |
| 0.4246 | 4.10303 | 2.39868 |
| 0.42753 | 4.09722 | 2.4337 |
| 0.4305 | 4.10786 | 2.45121 |
| 0.43351 | 4.13393 | 2.44706 |
| 0.43656 | 4.13253 | 2.47377 |
| 0.43966 | 4.10983 | 2.51551 |
| 0.4428 | 4.11969 | 2.53916 |
| 0.44599 | 4.11077 | 2.57525 |
| 0.44922 | 4.11078 | 2.59945 |
| 0.4525 | 4.11677 | 2.6116 |
| 0.45582 | 4.11999 | 2.62616 |
| 0.4592 | 4.12674 | 2.62045 |
| 0.46263 | 4.12757 | 2.63817 |
| 0.46611 | 4.12766 | 2.65486 |
| 0.46964 | 4.12286 | 2.67854 |
| 0.47322 | 4.12082 | 2.69987 |
| 0.47686 | 4.13487 | 2.71229 |
| 0.48056 | 4.15559 | 2.71202 |
| 0.48431 | 4.15827 | 2.73099 |
| 0.48813 | 4.16496 | 2.7499 |
| 0.492 | 4.18137 | 2.76131 |
| 0.49594 | 4.19293 | 2.77988 |
| 0.49994 | 4.23314 | 2.77245 |
| 0.504 | 4.23434 | 2.80302 |
| 0.50813 | 4.23732 | 2.8315 |
| 0.51233 | 4.26716 | 2.83353 |
| 0.5166 | 4.26776 | 2.86335 |
| 0.52094 | 4.31154 | 2.85243 |
| 0.52536 | 4.32299 | 2.87136 |
| 0.52985 | 4.35766 | 2.86859 |
| 0.53441 | 4.38187 | 2.87543 |
| 0.53906 | 4.38241 | 2.90632 |
| 0.54379 | 4.38422 | 2.9335 |
| 0.5486 | 4.42018 | 2.92909 |
| 0.5535 | 4.43664 | 2.93795 |
| 0.55849 | 4.44608 | 2.95519 |
| 0.56356 | 4.46357 | 2.95412 |
| 0.56873 | 4.48374 | 2.95296 |
| 0.574 | 4.52198 | 2.93035 |
| 0.57937 | 4.52524 | 2.94261 |
| 0.58483 | 4.52618 | 2.9622 |
| 0.5904 | 4.52737 | 2.97233 |
| 0.59608 | 4.53535 | 2.98435 |
| 0.60187 | 4.55699 | 3.04332 |
| 0.60777 | 4.58634 | 3.05556 |
| 0.61378 | 4.62068 | 3.05303 |
| 0.61992 | 4.62181 | 3.1027 |
| 0.62618 | 4.64613 | 3.13077 |
| 0.63257 | 4.66326 | 3.1675 |
| 0.63909 | 4.68953 | 3.1918 |
| 0.64575 | 4.73108 | 3.21164 |
| 0.65255 | 4.71842 | 3.2849 |
| 0.65949 | 4.79701 | 3.2499 |
| 0.66658 | 4.76777 | 3.31754 |
| 0.67383 | 4.83799 | 3.28808 |
| 0.68123 | 4.82243 | 3.35973 |
| 0.6888 | 4.85207 | 3.38407 |
| 0.69654 | 4.94025 | 3.36541 |
| 0.70446 | 5.00903 | 3.37063 |
| 0.71255 | 5.10586 | 3.3605 |
| 0.72084 | 5.19663 | 3.36022 |
| 0.72932 | 5.2841 | 3.3607 |
| 0.738 | 5.39777 | 3.31363 |
| 0.74689 | 5.48596 | 3.29168 |
| 0.756 | 5.55355 | 3.28596 |
| 0.76533 | 5.63233 | 3.24395 |
| 0.7749 | 5.75712 | 3.13612 |
| 0.78471 | 5.84876 | 3.0575 |
| 0.79477 | 5.89209 | 3.02342 |
| 0.80509 | 5.95386 | 2.93438 |
| 0.81569 | 6.00555 | 2.85256 |
| 0.82656 | 6.08619 | 2.72939 |
| 0.83773 | 6.10682 | 2.65686 |
| 0.84921 | 6.16473 | 2.54437 |
| 0.861 | 6.18665 | 2.45439 |
| 0.87313 | 6.20913 | 2.37133 |
| 0.8856 | 6.22821 | 2.27193 |
| 0.89844 | 6.26445 | 2.14495 |
| 0.91165 | 6.28896 | 2.04926 |
| 0.92526 | 6.32223 | 1.93132 |
| 0.93927 | 6.32707 | 1.82067 |
| 0.95372 | 6.4339 | 1.64741 |
| 0.96863 | 6.42249 | 1.52728 |
| 0.984 | 6.41777 | 1.40852 |
| 0.99987 | 6.37361 | 1.32121 |
| 1.01626 | 6.38547 | 1.21373 |
| 1.0332 | 6.36254 | 1.16429 |
| 1.06883 | 6.19337 | 0.95728 |
| 1.08758 | 6.27491 | 0.94993 |
| 1.107 | 6.23144 | 0.91958 |
| 1.12713 | 6.18576 | 0.88991 |
| 1.148 | 6.17218 | 0.83655 |
| 1.16966 | 6.18761 | 0.78311 |
| 1.19216 | 6.18046 | 0.76222 |
| 1.21553 | 6.14153 | 0.74689 |
| 1.24021 | 6.13075 | 0.71542 |
| 1.26553 | 6.10641 | 0.68087 |
| 1.29191 | 6.04791 | 0.6602 |
| 1.3194 | 6.00876 | 0.6311 |
| 1.34809 | 6.00136 | 0.60251 |
| 1.37806 | 6.0241 | 0.56236 |
| 1.40939 | 5.9715 | 0.513 |
| 1.44218 | 6.05053 | 0.40492 |
| 1.47653 | 6.09349 | 0.34123 |
| 1.51256 | 6.1211 | 0.28426 |
| 1.55038 | 6.26536 | 0.22095 |
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
- —
4L 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.