Real-Time TDDFT Combined with Molecular Dynamics¶
by Ronaldo Rodrigues Pela for exciting neon
(Jupyter notebook by Mara Voiculescu and Martin Kuban)
Purpose: In this tutorial, you will learn how to run a molecular dynamics calculation with real-time time-dependent density-functional theory (RT-TDDFT) to evolve the electrons wavefunctions (also called Ehrenfest Dynamics). We consider cubic BN to illustrate it.
0. Before Starting¶
Read the following paragraphs before starting with the rest of this tutorial!
Before running any Jupyter tutorials, please refer to the 00_before_starting.md document on how to correctly set up the environment. This only needs to be done once. After which, the venv can be (re)activated from exciting's root directory:
source tools/excitingjupyter/venv/excitingvenv/bin/activate
Important note: All input parameters that will appear will be given in atomic units! For this tutorial, it can be useful to remind the conversion between a.u. and the SI for times: 1 a.u. = 0.02418884254 fs, and for forces 1 Ha/bohr = 51.42208 eV/A.
2. Ground-State Calculation¶
i) Preparation of the Input File
The first step is to create a directory for the system that we want to investigate, run_BN_Ehrenfest and a subdirectory for the ground-state calculation, GS.
%%bash
mkdir -p run_BN_Ehrenfest && cd run_BN_Ehrenfest
mkdir -p GS
cd ..
As initial condition for the time evolution done in RT-TDDFT, we need the electron density and potential from a ground-state calculation. Therefore, we create the file input.xml that could look like the following:
<input>
<title>BN Ehrenfest</title>
<structure speciespath="$EXCITINGROOT/species/">
<crystal scale="6.833">
<basevect>0.0 0.5 0.5 </basevect>
<basevect>0.5 0.0 0.5 </basevect>
<basevect>0.5 0.5 0.0 </basevect>
</crystal>
<species speciesfile="B.xml" rmt="1.32">
<atom coord="0.0 0.0 0.0"
velocity="0.0 0.0 0.0" />
</species>
<species speciesfile="N.xml" rmt="1.28">
<atom coord="0.25 0.25 0.25"
velocity="0.0 0.0 0.0"/>
</species>
</structure>
<groundstate
ngridk="6 6 6"
rgkmax="4.0"
gmaxvr="12.0"
epsengy="1e-5"
do="fromscratch"
outputlevel="high"
nempty="4"
xctype="LDA_PW">
</groundstate>
</input>
Do not forget to replace in the input.xml the actual value of the environment variable $EXCITINGROOT. You can do this by directly editing the input.xml file or by using the following command:
%%bash
cd run_BN_Ehrenfest/GS
python3 -m excitingscripts.setup.excitingroot
cd ../..
%%bash
cd run_BN_Ehrenfest
python3 -m excitingscripts.execute.single -r GS
cd ..
You can check the output files, especially the main output file INFO.OUT, for general information. In the case of a successfully finished calculation, the last lines of the INFO.OUT will contain the message
...
================================================================================
| EXCITING NEON stopped =
================================================================================
Check if this is indeed the case and if the EFERMI.OUT and STATE.OUT files are present. They contain the Fermi level and the converged electron density and potential, respectively, and are the starting point of the RT-TDDFT calculation.
Please note: To obtain reliable results it is necessary to perform careful convergence tests with respect to the k-point mesh (parameter ngridk) and the size of the basis set (parameter rgkmax). For details see the tutorial Simple convergence tests.
3. Performing an "Ehrenfest Dynamics" Calculation¶
Create a new subdirectory ehrenfest and enter it. You can prepare the input file (input.xml) of a RT-TDDFT calculation starting from the existing groundstate input file. Copy the following files to the current directory. You can perform all of this with the following commands:
%%bash
cd run_BN_Ehrenfest
mkdir -p ehrenfest && cd ehrenfest
cp ../GS/{input.xml,EFERMI.OUT,STATE.OUT} .
cd ../..
The explicit ground-state calculation can be avoided with the attribute do="skip" inside the element groundstate.
...
<groundstate
do="skip"
... >
...
</groundstate>
...
In order to perform a "Ehrenfest Dynamics" calculation, the elements xs and MD must be added to the input file inside the input element, as shown below.
...
<xs
xstype ="RT-TDDFT"
ngridk="4 4 4"
vkloff="0.0 0.0 0.0"
nosym="true"
reducek="false"
nempty="2">
<realTimeTDDFT
propagator="SE"
timeStep="0.2d0"
endTime="16.0d0"
printTimingGeneral="true"
printTimingDetailed="true"
calculateNExcitedElectrons="false"
printAfterIterations="1"
vectorPotentialSolver="improvedeuler">
<laser fieldType="total">
<sinSq amplitude="10.d0" omega="1.d0" phase="0.d0" t0="0.d0" pulseLength="16.d0" direction="x"/>
<sinSq amplitude="10.d0" omega="1.d0" phase="0.d0" t0="0.d0" pulseLength="16.d0" direction="y"/>
<sinSq amplitude="10.d0" omega="1.d0" phase="0.d0" t0="0.d0" pulseLength="16.d0" direction="z"/>
</laser>
<pmat readFromFile="false" writeToFile="false" forceHermitian="false" />
</realTimeTDDFT>
</xs>
<MD
type="Ehrenfest"
printAllForces="true"
timeStep="1.0d0"
integrationAlgorithm="HeunSimplified">
</MD>
...
The following figure illustrates $A_x(t)$, the x component of the vector potential:
In this example, we are assuming $A_x(t)= A_y(t) = A_z(t)$, i.e., one laser pulse applied along the [111] direction.
For a detailed explanation of the element realTimeTDDFT, please check the tutorial Real-time TDDFT. We go here through all attributes that appear in MD to clarify their meaning:
type: Type of MD to be performed. In Ehrenfest MD, the outputs are printed out every n steps, where n is given byprintAfterIterations.printAllForces: When set to"true", the following components of the total force acting on an ion are printed out: external, Hellmann-Feynman, core and valence corrections..timeStep: Time step $\Delta t_N$ of the MD calculation. When doing Ehrenfest MD, if $\Delta t_N$ is not a multiple of the time step $\Delta t_e$ used in the electronic evolution (RT-TDDFT evolution), it will be automatically rounded down to $n\Delta t_e$, where n is the largest integer lower or equal the ratio $\Delta t_N / \Delta t_e$.integrationAlgorithm: Algorithm employed for the trajectory of the nuclei.
All relevant parameters for an "Ehrenfest Dynamics" calculation are found in Input Reference.
%%bash
cd run_BN_Ehrenfest
python3 -m excitingscripts.execute.single -r ehrenfest
cd ..
Be aware that, depending on the computer you are using, this calculation may take several minutes.
ii) Output Files
Apart from the output files related to RT-TDDFT (explained in the tutorial Real-time TDDFT), an Ehrenfest Dynamics calculation also generates, for each atom, the output files:
ATOM_xyzw.OUT: contains 10 columns, where
- the first one has the time $t$;
- columns 2-4 have the cartesian coordinates of the atom position $x(t)$, $y(t)$ and $z(t)$ (at the given time $t$);
- columns 5-7 have the cartesian components of the atom velocity $v_x(t)$, $v_y(t)$ and $v_z(t)$;
- columns 8-10 have the cartesian components of the total force acting on that atom $F_x(t)$, $F_y(t)$ and $F_z(t)$.
FEXT_xywz.OUT, FHF_xywz.OUT, FVAL_xywz.OUT and FCR_xywz.OUT. These files are printed out only if
printAllForcesis set to"true". In each file, there are four columns, with the first one containing the time, and the other three, the cartesian components ($x$, $y$ and $z$) of the considered force:- FEXT_xywz.OUT: external force due to the applied electric field;
- FHF_xywz.OUT: Hellman-Feynman force;
- FVAL_xywz.OUT: valence corrections to the Hellman-Feynman force;
- FCR_xywz.OUT: core corrections to the Hellman-Feynman force.
In the previous list of outputs, x, y, z and w are integer numbers 0-9 and the sequence xyzw refers to the number of a specific atom as given in input.xml. For instance 0001 refers to the 1st atom, 0002, to the second, etc.
%%bash
cd run_BN_Ehrenfest/ehrenfest
python3 -m excitingscripts.plot.multitask --ylabel '$F_x$ [a.u.]' --xlabel 'Time [a.u.]' -f ATOM_0001.OUT -k 0 7 -f FEXT_0001.OUT -k 0 1 -f FHF_0001.OUT -k 0 1 -f FVAL_0001.OUT -k 0 1 -f FCR_0001.OUT -k 0 1 -c 'Total' 'Ext' 'HF' 'Valence corr.' 'Core corr.' --xlim 0. 16. --legend_position 'upper left' --plot_name 'Force'
cd ../..
The resulting figure should look like
To check the time evolution of the position of boron, you can run the command:
%%bash
cd run_BN_Ehrenfest/ehrenfest
python3 -m excitingscripts.plot.multitask --ylabel 'Position [bohr]' --xlabel 'Time [a.u.]' -f ATOM_0001.OUT -k 0 1 -f ATOM_0001.OUT -k 0 2 -f ATOM_0001.OUT -k 0 3 -c '$x(t)$' '$y(t)$' '$z(t)$' --xlim 0. 16. --legend_position 'upper left' --plot_name 'Position'
cd ../..
to obtain a figure like
5. Converging the Results¶
From the previous two figures, you can conclude that the test case analyzed here should be considered as a pedagogical example. Following remarks can be done
- The time step $\Delta t_N$ in the
MDelement needs to be smaller, to obtain a more smooth curve of the forces or the positions over time $t$. There is an optimal ratio between $\Delta t_N/\Delta t_e$ that allows for a good compromise between the computational time and accuracy (see discussion in Ref. [1]). endTimeis quite small in the example. For reallistic MD calculations, this should be on the order of fs or ps (1 fs = 41.34 a.u. and 1 ps = 41341 a.u.).- The frequency and the duration of the laser pulse here are not intended to reproduce experimental settings. Typically, the laser pulse could last for some fs. Moreover, a laser frequency closer to the phonon frequencies would lead to more pronounced atom movements.
- For better converged calculations, the following parameters should be carefully checked:
ngridkrgkmax- local-orbitals
Bibliography¶
- Ronaldo Rodrigues Pela and Claudia Draxl. "Ehrenfest dynamics implemented in the all-electron package exciting" (link).
- Ronaldo Rodrigues Pela, Claudia Draxl. "All-electron full-potential implementation of real-time TDDFT in exciting" (link).
- More information about the script
excitingscripts.plot.multitaskcan be found here.