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First-principles modelling of infrared and Rama...

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First-principles modelling of infrared and Raman spectra

Presented at the Materials Chemistry Consortium & Faraday Institution Energy Applications and Batteries 2026 workshop on 4th March 2026.

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Jonathan Skelton

March 03, 2026
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  1. J. M. Skelton, C. Umeh, A. R. Pallipurath, L. Kiltinavicius

    and J. M. Flitcroft University of Manchester and University of Leeds ([email protected]) First-principles modelling of infrared and Raman spectra
  2. Phonopy-Spectroscopy Dr J. M. Skelton MCC/Faraday Workshop, 4th March 2026

    | Slide 2 o Motivation: Add capability to simulate infrared and Raman spectra to the Phono(3)py code: Phonopy-Spectroscopy o Design goals: • Flexible - capable of modelling routine and advanced experiments • General - easy to interface to other codes and/or implement new experiments • Efficient - extensive use of NumPy/SciPy, Numba used for “slow” processes o Features • Raman spectrum simulations for arbitrary instrument geometry and partial capture of resonance effects • Complex IR dielectric function 𝜀(𝜔) and simulations of optical spectra - can be easily repurposed for UV/vis measurements • Python API designed for easy interoperability and for implementing more advanced simulations (e.g. from Jupyter notebooks) • Additional analysis tools via API (e.g. for characterising phonon modes)
  3. Simulating Raman spectra Dr J. M. Skelton Raman polarizability tensors:

    𝜶!" (𝐸) = 1 𝑉 𝜕𝜺(𝐸) 𝜕𝑄!" ≈ 1 𝑉 ∆𝜺(𝐸) ∆𝑄!" Raman intensities: 𝐼!" = 0 𝒆# $ 2 𝑹𝜶!" 𝑹% 2 0 𝒆& ' Differential cross sections (Stokes scattering): 𝑑𝜎!" ( 𝑑Ω = 𝜎!" ( ) = ℎ 4𝜋𝑐* 𝜔& − 𝜔!" * 𝜔!" 𝑛!" + 1 𝐼!" Phonon occupation number: 𝑛!" 𝑇 = 1 exp ⁄ −ℏ𝜔!" 𝑘+ 𝑇 − 1 Raman spectrum: 𝑑𝜎(𝜔) 𝑑Ω = E " 𝜎!" ( ) 𝜋 ⁄ 𝛾!" 2 𝜔 − 𝜔!" ' + ⁄ 𝛾!" 2 ' Can partially account for resonance effects with suitable 𝜺(𝐸) Can handle complex 0 𝒆& /0 𝒆, (circularly-polarised light) Power/temperature modulation crucial for matching experiment Can include calculated linewidths (e.g. Phono3py) MCC/Faraday Workshop, 4th March 2026 | Slide 3
  4. Simulating Raman spectra Dr J. M. Skelton For powders, average

    the 𝐼!" over Euler angles: 𝐼!" = H - '. H - . H - '. 1 8𝜋' 0 𝒆, 2 𝑹(𝜙, 𝜃, 𝜓) 2 𝜶!" 2 𝑹(𝜙, 𝜃, 𝜓)% 2 0 𝒆& ' sin 𝜃 d𝜓 d𝜃 d𝜙 • Analytical formula for ”standard” measurement geometries and numerical integration for non-standard geometries Include preferred orientation with an orientation-distribution function 𝑤: 𝐼!" = H - '. H - . H - '. 𝑤 𝜙, 𝜃, 𝜓 𝐼!" 𝜙, 𝜃, 𝜓 sin 𝜃 d𝜓 d𝜃 d𝜙 • Currently implemented the March-Dollase distribution function for a single preferred orientation MCC/Faraday Workshop, 4th March 2026 | Slide 4
  5. Raman: SnSe Dr J. M. Skelton Chandrasekhar et al., Phys.

    Rev. B 15 (4), 2177 (1977) MCC/Faraday Workshop, 4th March 2026 | Slide 5
  6. Raman: Zirconolite Dr J. M. Skelton ̅ 𝑣 / cm-1

    Irrep 𝛾 / cm-1 ⁄ 𝑑𝜎 𝑑𝛺 / 10-14 Å2 sr-1 93.5 Ag 2.16 1.15 111 Bg 2.20 3.55 118 Bg 2.11 2.70 119 Ag 3.34 3.43 125 Ag 1.44 11.3 ⋯ ⋯ ⋯ ⋯ 780 Ag 23.6 16.1 800 Bg 26.5 0.23 800 Ag 26.3 1.69 807 Bg 23.2 1.13 830 Bg 23.6 0.78 MCC/Faraday Workshop, 4th March 2026 | Slide 6
  7. Simulating IR spectra Mode effective charges 𝒁!" : 𝑍!" 0

    = 𝜕𝑃0 𝜕𝑄!" = E 1,3 𝑍1 ∗,03𝑋 !",1 3 Dipole oscillator strengths 𝑺!" : 𝑆 !" 03 = 𝑍!" 0 𝑍 !" 3 Infrared dielectric function 𝜺 𝜔 : 𝜀03 𝜔 = 𝜀5 03 + 1 𝑉 E " 𝑹𝑆 !" 03𝑹% 𝜔!" ' − (𝜔 + 𝑖𝛾!" )' Dr J. M. Skelton Can include calculated linewidths (e.g. Phono3py) MCC/Faraday Workshop, 4th March 2026 | Slide 8
  8. Measurement geometry Dr J. M. Skelton o Raman: • No

    restrictions on experimental geometry o Infrared: • Implementation tightly couped to geometry • Currently assume collinear geometry, but plans to support “off-axis” reflectivity measurements including ATR soon MCC/Faraday Workshop, 4th March 2026 | Slide 9
  9. Simulating optical spectra Complex refractive index: [ 𝑛" 𝜔 =

    𝜀" 𝜔 = 𝑛" (𝜔) + 𝑖𝑘" 𝜔 Reflectivity at normal incidence: 𝑅" 𝜔 = [ 𝑛" 𝜔 − 1 [ 𝑛" 𝜔 + 1 ' Absorption coefficient: 𝛼" 𝜔 = 2𝜔 𝑐 𝑘" 𝜔 Optical conductivity: 𝜎" 𝜔 = −𝑖𝜔𝜀- 𝜀" 𝜔 − 1 Energy loss function: 𝐿" 𝜔 = Im − 1 𝜀" 𝜔 Dr J. M. Skelton Dielectric function Optical eigenmodes Diagonalise MCC/Faraday Workshop, 4th March 2026 | Slide 10
  10. Simulating optical spectra Intrinsic transmission: 𝑇" 678 𝜔 = exp

    −𝛼 𝜔 ×𝑑 Normal transmission: 𝑇" 79:; 𝜔 = 1 − 𝑅(𝜔) ' exp −𝛼 𝜔 ×𝑑 Incoherent transmission: 𝑇" 67<9= 𝜔 = 1 − 𝑅(𝜔) ' exp −𝛼 𝜔 ×𝑑 1 − 𝑅'(𝜔) exp −2𝛼 𝜔 ×𝑑 Absorption: 𝐴" = − ln 𝑇" Dr J. M. Skelton Dielectric function Optical eigenmodes Diagonalise MCC/Faraday Workshop, 4th March 2026 | Slide 11
  11. Simulating optical spectra Power coupling for incident polarisation 0 𝒆&

    : 𝑐" 𝜔 = Λ(𝜔) >? 0 𝒆& ' Mode-average properties: 𝑃 𝜔 = E " 𝑐" 𝜔 𝑃 " 𝜔 Mode-average absorbance: 𝐴 𝜔 = − ln 𝑇 𝜔 Also possible using OEs as a basis: • Jones/Airy-Jones method for polarised measurements • Berreman 4×4 method for ATR (non- collinear geometry) • Transfer-matrix method for thin-film stacks Dr J. M. Skelton Dielectric function Optical eigenmodes Optical spectrum Diagonalise Combine MCC/Faraday Workshop, 4th March 2026 | Slide 12
  12. Simulating optical spectra Effective-medium approximation (1): 𝜀@AA 𝜔 = 1

    3 Tr 𝜺 𝜔 Effective-medium approximation (2): 𝜀@AA 𝜔 = 1 3 E " 𝜀" 𝜔 Single-crystal (collinear geometry): 𝜺 𝜔 = 𝜀BB 𝜔 𝜀BC 𝜔 𝜀BD 𝜔 𝜀CB 𝜔 𝜀CC 𝜔 𝜀CD 𝜔 𝜀DB 𝜔 𝜀CD 𝜔 𝜀DD 𝜔 N. B. Could ”intercept” either EMA method and average with the 𝜀/𝜀(𝜔) of a pelleting medium - Maxwell-Garnett model Dr J. M. Skelton Dielectric function Optical eigenmodes Optical spectrum Diagonalise Combine EELS MCC/Faraday Workshop, 4th March 2026 | Slide 13
  13. IR: SnS Dr J. M. Skelton Chandrasekhar et al., Phys.

    Rev. B 15 (4), 2177 (1977) MCC/Faraday Workshop, 4th March 2026 | Slide 17
  14. IR: SnS Dr J. M. Skelton Chandrasekhar et al., Phys.

    Rev. B 15 (4), 2177 (1977) MCC/Faraday Workshop, 4th March 2026 | Slide 18
  15. Summary o Comprehensive simulations of Raman and IR spectra: •

    Raman: single crystals and powders, partial inclusion of resonance effects • IR: IR dielectric function and optical spectra • Both show generally good agreement with experiments o There’s more: • IR calculator can also calculate 𝜀6976< /𝜀E8F86< and 𝜔G9 • Analysis tools including for visualisation, classification and band unfolding o Current status: • All functionality shown today is available via the API from the develop branch of the GitHub: https://github.com/skelton-group/Phonopy-Spectroscopy/tree/develop • Plans to implement: (1) improved handling of LO/TO splitting; (2) Maxwell-Garnett model for IR measurements on pellets; (3) fully-polarised single-crystal IR measurements; and (4) ATR/off-axis IR reflectivity • Plans to have a simple CLI for common simulations - in progress and should be available soon (target: next MCC conference) Dr J. M. Skelton MCC/Faraday Workshop, 4th March 2026 | Slide 19
  16. Acknowledgements Dr J. M. Skelton Implementation (inc. maths + sanity

    checks): o Jonathan Skelton (UoM) o Anuradha Pallipurath (UoL) o Chidimma Umeh (UoM) Beta testing (i.e. bug squashing): o Joseph Flitcroft (UoM) o Guanping Li (UoM) o David Collins (UoL) … plus other collaborators too numerous to mention MCC/Faraday Workshop, 4th March 2026 | Slide 20