Promoted Density Approach for sampling initial conditions for trajectory-based nonadiabatic photodynamics
Project description
PROMDENS: Promoted Density Approach code
promdens is a Python code implementing the Promoted Density Approach (PDA) and its version for windowing (PDAW) freely available to the scientific community under MIT license.
Derivation of PDA and PDAW and its benchmark against quantum dynamics can be found at ArXiV or soon at JPCL.
Installation
The code is published on PyPI and can be installed via pip
pip install promdens
After installation, the code is available as a script via the promdens command. To print help, run:
promdens --help
The minimum supported Python version is 3.7.
The code depends on numpy and matplotlib libraries that are automatically installed by pip.
However, since pip by default installs packages into a global Python environment,
it can break previously installed packages e.g. by installing an incompatible version of numpy.
Therefore, we recommend using tools like pipx or uv which install the dependencies into an isolated Python environment but still make the promdens command globally available.
See the example for pipx
pip install pipx
pipx install promdens
and uv
pip install uv
uv tool install promdens
Usage
The code requires information about the method (PDA or PDAW), the number of excited states to consider, the number of initials conditions to be generated, and the characteristics of the laser pulse, such as the envelope type (Gaussian, Lorentzian, sech, etc.), the pulse frequency, the linear chirp parameter, and the full width at half maximum parameter. The code can be launched from a terminal with a series of flags as follows
promdens --method pda --energy_units a.u. --tdm_units debye --nstates 2 --fwhm 3 --omega 0.355 --npsamples 10 --envelope_type gauss input_file.dat
The input file should contain information about the excitation energies and magnitudes of the transition dipole moments for each pair of sampled nuclear positions and momenta (labelled by an index number). In the following, we provide an example of the input file for the first two excited states of protonated formaldimine:
#index dE12 (a.u.) mu_12 (Debye) dE13 (a.u.) mu_13 (Debye)
1 0.32479719 0.1251 0.40293672 1.351
2 0.32070472 0.2434 0.40915241 1.289
3 0.34574925 0.7532 0.38595754 1.209
4 0.33093699 0.1574 0.36679075 1.403
5 0.31860215 0.1414 0.36973886 1.377
6 0.31057768 0.0963 0.40031651 1.390
7 0.33431888 0.1511 0.40055704 1.358
8 0.31621589 0.0741 0.36644659 1.425
9 0.32905912 0.5865 0.36662982 1.277
10 0.31505412 0.2268 0.35529522 1.411
Using this input file and running the command line above, the user receives the following output file called pda.dat containing information about excitation times and initial excited states:
# Sampling: number of ICs = 10, number of unique ICs = 6
# Field parameters: omega = 3.55000e-01 a.u., linear_chirp = 0.00000e+00 a.u., fwhm = 3.000 fs, t0 = 0.000 fs, envelope type = 'gauss'
# index exc. time (a.u.) el. state dE (a.u.) |tdm| (a.u.)
3 50.98896272 1 0.34574925 0.75320000
3 -26.10280808 1 0.34574925 0.75320000
4 -68.05804034 2 0.36679075 1.40300000
4 -50.42549647 2 0.36679075 1.40300000
4 -14.77969117 2 0.36679075 1.40300000
5 -32.66188108 2 0.36973886 1.37700000
8 116.78592486 2 0.36644659 1.42500000
9 -47.47085207 2 0.36662982 1.27700000
9 -39.94428629 2 0.36662982 1.27700000
10 -92.13785801 2 0.35529522 1.41100000
Inspecting this output file shows that the code generated 10 initial conditions accounting for the effect of the laser pulse, yet only 6 unique ground-state samples (pairs nuclear were used (indexes 3, 4, and 9 were selected more than once). The initial conditions are also spread over both excited states. The user should then run only 6 nonadiabatic simulations: initiating the position-momentum pair with index 3 in the first excited state and position-momentum pairs with indexes 4, 5, 8, 9, and 10 in the second excited state.
If the same command would be used with PDAW instead of PDA (--method pdaw), the output file would look like
# Convolution: 'I(t) = exp(-4*ln(2)*(t-t0)^2/fwhm^2)'
# Parameters: fwhm = 3.000 fs, t0 = 0.000 fs
# index weight S1 weight S2
1 1.78475e-05 9.66345e-07
2 1.56842e-05 2.59858e-08
3 6.31027e-02 1.29205e-03
4 1.79107e-04 1.62817e-01
5 2.31817e-06 1.01665e-01
6 2.96548e-08 3.90152e-06
7 3.81650e-04 3.33694e-06
8 2.36147e-07 1.75628e-01
9 1.47188e-03 1.37747e-01
10 1.33347e-06 3.55670e-01
The code provides the pulse intensity and weights necessary for the convolution described in Eq. (14) in the article. Note that the intensity should be normalized before used in convolution. If only a restricted amount of trajectories can be calculated, the user should choose the indexes and initial excited states corresponding to the largest weights in the file. For example, if we could run only 10 trajectories of protonated formaldimin, we would run ground-state position-momentum pairs with indexes 3, 4, 7, and 9 starting in S$_1$ and indexes 3, 4, 5, 8, 9, and 10 starting in S$_2$.
If the user selects option --plot, the code will produce a series of plots analyzing the provided data and calculated results, e.g. the absorption spectrum calculated with the nuclear ensemble method, the pulse spectrum or the Wigner pulse transform.
The work on a more detailed manual is currently in progress. If you have any questions, do not hesitate to contact the developers.
Analytic formulas for pulse envelope Wigner transform
The code is based on the Wigner pulse transform which requires evaluating the Wigner integral
$$\mathcal{W}_E(t^\prime,\omega)=\int _{-\infty}^{\infty} E\left(t^\prime+\frac{s}{2}\right) E^*\left(t^\prime-\frac{s}{2}\right) \mathrm{e}^{-i\omega s} \mathrm{d} s$$
To simplify the integral evaluation, we implemented simpler Wigner pulse envelope transform (see the article for more details)
$$\mathcal{W}_\varepsilon(t,\omega) = \int _{-\infty}^{\infty} \varepsilon\left(t+\frac{s}{2}\right) \varepsilon\left(t-\frac{s}{2}\right) \mathrm{e}^{-i\omega s} \mathrm{d} s$$
where $\varepsilon$ is the pulse envelope. While lorentz, sin2 and sech the $\mathcal{W}_\varepsilon$ is still calculated numerically by employing the trapezoid rule for the integral, the gauss and sin envelope Wigner transforms are calculated analytically according to analytic formulas. In the following analytic formulas, we apply a substitution
$\Omega = \Delta E/\hbar - \omega$.
Gaussian envelope
$$\mathcal{W}_\varepsilon(t^\prime,\omega)=\tau\sqrt{\frac{\pi}{\ln2}}16^{-\frac{(t^\prime - t_0)^2}{\tau^2}}\exp\left(-\frac{\tau^2\omega^2}{\ln16}\right)$$
Sinusoidal envelope
- $\pi\frac{-2\tau\Omega\cos(2(t^\prime - t_0 + \tau)\Omega)\sin(\pi(t^\prime - t_0)/\tau) +\pi\cos(\pi(t^\prime - t_0)/\tau)\sin(2(t^\prime - t_0 + \tau)\Omega))}{\Omega(\pi^2 - 4\tau^2\Omega^2)}$ if $t^\prime < t_0$ and $t^\prime > t_0 - \tau $
- $\pi\frac{2\tau\Omega\cos(2(-t^\prime + t_0 + \tau)\Omega)\sin(\pi(t^\prime - t_0)/\tau) +\pi\cos(\pi(t^\prime - t_0)/\tau)\sin(2(-t^\prime + t_0 + \tau)\Omega))}{\Omega(\pi^2 - 4\tau^2\Omega^2)}$ if $t^\prime \ge t_0$ and $t^\prime < t_0 - \tau $
- $0$ elsewhere
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