Optical constants
Refractive index of PtSe2 (Platinum diselenide)
Tharrault et al. 2025: 3L film; n,k 0.416–1.54 µm
- Data
- tabulated nk
- Range
- 0.4154–1.54 µm
- Points
- 108
- State
- crystalline
- Licence
- CC0-1.0
Plot
Click the plot to set the calculator wavelength.
At one wavelength
- Refractive index n
- 4.79219
- Extinction coefficient k
- 2.7885
- Permittivity ε1
- 15.1893
- Permittivity ε2
- 26.7261
- Absorption coefficient α
- 596347 cm⁻¹
- Penetration depth δ = λ/(2πk)
- 33.5375 nm
- Abbe number Vd
- —
- Chromatic dispersion dn/dλ
- 0.388087 µm⁻¹
- Group index ng
- 4.56415
- 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: 3L film; n,k 0.416–1.54 µm
ptse2 = ls.fetch_refractiveindex("main", "PtSe2", "Tharrault-3L", ref="c5c2f188e848453def5970e347399d653df2ffc2")
print(ptse2.range_nm) # (415.36, 1539.99) 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_2cf98053b562/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-2025-3l).
# ... 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=416, 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
108 rows as published| λ (µm) | n | k |
|---|---|---|
| 0.41536 | 4.58532 | 1.96277 |
| 0.41816 | 4.52479 | 2.00773 |
| 0.421 | 4.52653 | 2.02785 |
| 0.42388 | 4.50592 | 2.05252 |
| 0.4268 | 4.44679 | 2.1146 |
| 0.42975 | 4.44824 | 2.13208 |
| 0.43275 | 4.4435 | 2.18573 |
| 0.4358 | 4.46173 | 2.19921 |
| 0.43888 | 4.449 | 2.23343 |
| 0.44201 | 4.4096 | 2.29396 |
| 0.44519 | 4.43978 | 2.29003 |
| 0.44841 | 4.44303 | 2.30648 |
| 0.45167 | 4.43651 | 2.33359 |
| 0.45499 | 4.44977 | 2.33892 |
| 0.45835 | 4.46363 | 2.34516 |
| 0.46177 | 4.47763 | 2.35042 |
| 0.46523 | 4.47591 | 2.38086 |
| 0.46875 | 4.49177 | 2.39039 |
| 0.47232 | 4.52579 | 2.37747 |
| 0.47595 | 4.5441 | 2.39097 |
| 0.47963 | 4.57096 | 2.38822 |
| 0.48337 | 4.54137 | 2.44467 |
| 0.48717 | 4.58187 | 2.42662 |
| 0.49103 | 4.57667 | 2.45977 |
| 0.49495 | 4.56389 | 2.4999 |
| 0.49893 | 4.59331 | 2.50275 |
| 0.50298 | 4.62592 | 2.49113 |
| 0.50709 | 4.60505 | 2.53663 |
| 0.51128 | 4.63885 | 2.54007 |
| 0.51553 | 4.63122 | 2.5683 |
| 0.51985 | 4.6551 | 2.57191 |
| 0.52425 | 4.65012 | 2.59995 |
| 0.52872 | 4.63072 | 2.64262 |
| 0.53327 | 4.68374 | 2.60142 |
| 0.53789 | 4.66325 | 2.62892 |
| 0.5426 | 4.6688 | 2.64455 |
| 0.54739 | 4.70438 | 2.61323 |
| 0.55227 | 4.67349 | 2.66254 |
| 0.55723 | 4.69545 | 2.66588 |
| 0.56229 | 4.69043 | 2.69232 |
| 0.56743 | 4.71365 | 2.69732 |
| 0.57268 | 4.74841 | 2.71109 |
| 0.57801 | 4.7328 | 2.75428 |
| 0.58346 | 4.79058 | 2.75554 |
| 0.589 | 4.79273 | 2.79965 |
| 0.59465 | 4.79731 | 2.86958 |
| 0.60041 | 4.75725 | 2.9861 |
| 0.60628 | 4.68987 | 3.15478 |
| 0.61227 | 4.73385 | 3.20073 |
| 0.61838 | 4.78952 | 3.23471 |
| 0.62461 | 4.88073 | 3.22954 |
| 0.63096 | 4.92916 | 3.26498 |
| 0.63745 | 5.01494 | 3.25271 |
| 0.64407 | 5.10284 | 3.22333 |
| 0.65084 | 5.11434 | 3.26771 |
| 0.65774 | 5.19525 | 3.22593 |
| 0.66479 | 5.0783 | 3.34174 |
| 0.672 | 5.16585 | 3.27741 |
| 0.67937 | 5.18938 | 3.26358 |
| 0.68689 | 5.25604 | 3.22798 |
| 0.69459 | 5.29802 | 3.21237 |
| 0.70246 | 5.39267 | 3.15314 |
| 0.71051 | 5.45641 | 3.12764 |
| 0.71875 | 5.54901 | 3.07674 |
| 0.72718 | 5.62797 | 3.04094 |
| 0.73581 | 5.72177 | 2.97575 |
| 0.74465 | 5.79781 | 2.9199 |
| 0.7537 | 5.86626 | 2.86211 |
| 0.76298 | 5.91658 | 2.7969 |
| 0.77249 | 5.96498 | 2.72391 |
| 0.78223 | 6.01556 | 2.63161 |
| 0.79223 | 6.04704 | 2.52803 |
| 0.80249 | 6.04808 | 2.44437 |
| 0.81301 | 6.03581 | 2.37498 |
| 0.82382 | 6.04959 | 2.28136 |
| 0.83491 | 6.0667 | 2.16742 |
| 0.84631 | 6.07819 | 2.05163 |
| 0.85802 | 6.11898 | 1.90134 |
| 0.87006 | 6.07865 | 1.82765 |
| 0.88245 | 6.0699 | 1.73158 |
| 0.89519 | 6.02956 | 1.65328 |
| 0.90831 | 5.99854 | 1.57671 |
| 0.92182 | 5.97344 | 1.49932 |
| 0.93573 | 5.93803 | 1.45071 |
| 0.95007 | 5.90694 | 1.38365 |
| 0.96486 | 5.91776 | 1.30934 |
| 0.98011 | 6.15049 | 1.06587 |
| 0.99586 | 6.15528 | 1.02746 |
| 1.01212 | 6.1782 | 0.97049 |
| 1.02891 | 6.18924 | 0.93382 |
| 1.08283 | 6.15653 | 0.76358 |
| 1.10208 | 6.17026 | 0.71978 |
| 1.12203 | 6.15176 | 0.66661 |
| 1.14271 | 6.18056 | 0.60429 |
| 1.16417 | 6.16871 | 0.51434 |
| 1.18645 | 6.13611 | 0.46844 |
| 1.2096 | 6.10118 | 0.41772 |
| 1.23367 | 6.04211 | 0.38751 |
| 1.2586 | 5.9764 | 0.35281 |
| 1.28468 | 5.93319 | 0.32817 |
| 1.31186 | 5.87875 | 0.30467 |
| 1.34022 | 5.82628 | 0.30329 |
| 1.36984 | 5.84747 | 0.2867 |
| 1.40079 | 5.72028 | 0.276 |
| 1.43318 | 5.63368 | 0.2985 |
| 1.46709 | 5.65001 | 0.28402 |
| 1.50266 | 5.70571 | 0.24026 |
| 1.53999 | 5.68513 | 0.22021 |
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
- —
3L 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.