7.4.4 Calculation of Absorption Spectra

The absorption cross-section ${\sigma }_{ii}(\omega )$ for light polarized in the $i$ direction ($i\in \{x,y,z\}$) can be obtained from the imaginary part ($\mathrm{\Im }$) of the frequency-dependent polarizability, ${\alpha }_{ii}(\omega )$: ¹⁴⁰¹ Zhu Y., Herbert J. M.
J. Chem. Phys.
(2018), 148, pp. 044117. Link

A rotationally-averaged absorption spectrum $A(\omega )$ is then simply

within the electric dipole approximation. Components ${\alpha }_{ij}(\omega )$ of the frequency-dependent polarizability tensor $𝜶(\omega )$ are obtained from the Fourier transform ($ℱ$) of the time-dependent dipole moment component ${\mu }_i(t)$, for a perturbing field ${ℰ}_j$ in the $j$ direction: ¹⁴⁰¹ Zhu Y., Herbert J. M.
J. Chem. Phys.
(2018), 148, pp. 044117. Link

To compute the spectrum in Eq. (7.33), three separate perturbations in the $x$, $y$, and $z$ directions are required, else some excitations may be missing if their transition moment is strictly perpendicular to the applied field, causing the matrix element $⟨{\mathrm{\Psi }}_n|{ℰ}_j|{\mathrm{\Psi }}_0⟩$ to vanish. However, these three perturbations ${ℰ}_x$, ${ℰ}_y$, and ${ℰ}_z$ can be applied all at once in a single calculation, in order to generate a superposition consisting of all possible excitations out of the ground state.

Two different scripts are provided to obtain the spectrum after the TDKS simulation is completed:

• •

  $QC/bin/tools/tdks_fft.py

• •

  $QC/bin/tools/tdks_pade.py

The first of these uses the Fourier transform method in Eq. (7.34) directly while the second makes use of Padé approximants to obtain comparable spectra with shorter propagation times. The scripts can be run as follows:

$QC/bin/tools/tdks_fft.py output spectrum.txt
$QC/bin/tools/tdks_pade.py output spectrum.txt

The file spectrum.txt produced by the processing script will contain two columns: frequency (eV) and strength (arbitrary units). These data can be visualized as an $(x,y)$ plot to view the spectrum.