Optical constants
Refractive index of PtSe2 (Platinum diselenide)
Tharrault et al. 2025: 7L 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
- 4.34262
- Extinction coefficient k
- 2.98448
- Permittivity ε1
- 9.95125
- Permittivity ε2
- 25.9209
- Absorption coefficient α
- 638258 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 31.3353 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 1.71454 µm⁻¹
- Group index ng
- 3.33515
- 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: 7L film; n,k 0.416–1.55 µm
ptse2 = ls.fetch_refractiveindex("main", "PtSe2", "Tharrault-7L", 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_ee113ec821c4/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-2025-7l).
# ... 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 | 4.09431 | 2.22117 |
| 0.41887 | 4.05966 | 2.27528 |
| 0.42171 | 4.06564 | 2.29063 |
| 0.4246 | 4.04232 | 2.33835 |
| 0.42753 | 4.02382 | 2.37785 |
| 0.4305 | 4.02797 | 2.40381 |
| 0.43351 | 4.05586 | 2.41113 |
| 0.43656 | 4.06296 | 2.43584 |
| 0.43966 | 4.04233 | 2.48988 |
| 0.4428 | 4.05092 | 2.5194 |
| 0.44599 | 4.05283 | 2.55105 |
| 0.44922 | 4.04783 | 2.58508 |
| 0.4525 | 4.06085 | 2.60553 |
| 0.45582 | 4.05433 | 2.64395 |
| 0.4592 | 4.06096 | 2.65918 |
| 0.46263 | 4.07171 | 2.67955 |
| 0.46611 | 4.06182 | 2.71906 |
| 0.46964 | 4.07028 | 2.73911 |
| 0.47322 | 4.06501 | 2.77138 |
| 0.47686 | 4.0829 | 2.77786 |
| 0.48056 | 4.09473 | 2.78869 |
| 0.48431 | 4.09162 | 2.81262 |
| 0.48813 | 4.09973 | 2.8265 |
| 0.492 | 4.11454 | 2.82802 |
| 0.49594 | 4.10221 | 2.85651 |
| 0.49994 | 4.11995 | 2.85903 |
| 0.504 | 4.1317 | 2.86049 |
| 0.50813 | 4.10819 | 2.9032 |
| 0.51233 | 4.12446 | 2.90457 |
| 0.5166 | 4.13239 | 2.912 |
| 0.52094 | 4.14231 | 2.91823 |
| 0.52536 | 4.13438 | 2.9486 |
| 0.52985 | 4.14526 | 2.95745 |
| 0.53441 | 4.16443 | 2.95492 |
| 0.53906 | 4.16879 | 2.96885 |
| 0.54379 | 4.17785 | 2.97969 |
| 0.5486 | 4.2033 | 2.97622 |
| 0.5535 | 4.20904 | 2.9899 |
| 0.55849 | 4.23447 | 2.98108 |
| 0.56356 | 4.26528 | 2.96584 |
| 0.56873 | 4.27497 | 2.98033 |
| 0.574 | 4.30581 | 2.96648 |
| 0.57937 | 4.32526 | 2.97088 |
| 0.58483 | 4.33787 | 2.97727 |
| 0.5904 | 4.34742 | 2.99176 |
| 0.59608 | 4.36641 | 3.00313 |
| 0.60187 | 4.43242 | 2.98138 |
| 0.60777 | 4.46909 | 2.97953 |
| 0.61378 | 4.47502 | 3.01269 |
| 0.61992 | 4.49344 | 3.03988 |
| 0.62618 | 4.50576 | 3.07706 |
| 0.63257 | 4.53349 | 3.10219 |
| 0.63909 | 4.55299 | 3.13827 |
| 0.64575 | 4.60175 | 3.15613 |
| 0.65255 | 4.63657 | 3.18109 |
| 0.65949 | 4.64384 | 3.23206 |
| 0.66658 | 4.62452 | 3.30295 |
| 0.67383 | 4.67951 | 3.30603 |
| 0.68123 | 4.7264 | 3.30599 |
| 0.6888 | 4.74925 | 3.33311 |
| 0.69654 | 4.81077 | 3.31132 |
| 0.70446 | 4.8522 | 3.30741 |
| 0.71255 | 4.90602 | 3.29254 |
| 0.72084 | 4.94073 | 3.30417 |
| 0.72932 | 4.99971 | 3.28735 |
| 0.738 | 5.02927 | 3.30039 |
| 0.74689 | 5.08149 | 3.31893 |
| 0.756 | 5.14577 | 3.34364 |
| 0.76533 | 5.20714 | 3.38434 |
| 0.7749 | 5.3212 | 3.39215 |
| 0.78471 | 5.41786 | 3.419 |
| 0.79477 | 5.5367 | 3.42051 |
| 0.80509 | 5.64549 | 3.41405 |
| 0.81569 | 5.76609 | 3.38663 |
| 0.82656 | 5.89559 | 3.32203 |
| 0.83773 | 6.00144 | 3.25775 |
| 0.84921 | 6.12625 | 3.14858 |
| 0.861 | 6.21865 | 3.04674 |
| 0.87313 | 6.29595 | 2.93981 |
| 0.8856 | 6.36271 | 2.83262 |
| 0.89844 | 6.42583 | 2.70863 |
| 0.91165 | 6.47384 | 2.58965 |
| 0.92526 | 6.50338 | 2.47809 |
| 0.93927 | 6.53267 | 2.36462 |
| 0.95372 | 6.55215 | 2.2524 |
| 0.96863 | 6.56166 | 2.15068 |
| 0.984 | 6.60507 | 2.02202 |
| 0.99987 | 6.60902 | 1.89693 |
| 1.01626 | 6.62666 | 1.7424 |
| 1.0332 | 6.63326 | 1.68253 |
| 1.06883 | 6.51133 | 1.36773 |
| 1.08758 | 6.55738 | 1.30394 |
| 1.107 | 6.52735 | 1.20631 |
| 1.12713 | 6.47658 | 1.1246 |
| 1.148 | 6.44217 | 1.04271 |
| 1.16966 | 6.41199 | 0.94499 |
| 1.19216 | 6.38297 | 0.89884 |
| 1.21553 | 6.34547 | 0.82923 |
| 1.24021 | 6.31882 | 0.78095 |
| 1.26553 | 6.28293 | 0.74756 |
| 1.29191 | 6.23483 | 0.70806 |
| 1.3194 | 6.20822 | 0.63006 |
| 1.34809 | 6.16159 | 0.64132 |
| 1.37806 | 6.13915 | 0.58392 |
| 1.40939 | 6.071 | 0.57751 |
| 1.44218 | 6.0697 | 0.52359 |
| 1.47653 | 6.04325 | 0.50704 |
| 1.51256 | 6.04429 | 0.43565 |
| 1.55038 | 6.06539 | 0.4099 |
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
- —
7L 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.