Nuclephile Substitution CH3Cl - mMD3: Difference between revisions
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[[File:TimeEvol CH3Cl mMD3.jpg|500px]] | [[File:TimeEvol CH3Cl mMD3.jpg|500px]] | ||
From this plot we very nicely see that at the beginning the two collective variables run parallel to each other, staying at the same side at approximately the same distance from the centre atom. At the | |||
=== 2D free-energy profile === | === 2D free-energy profile === | ||
Revision as of 11:17, 30 September 2019
Task
In this example the nucleophile substitution of a Cl- by another Cl- in CH3Cl via meta dynamics is simulated using two collective variables simultaneously.
Input
POSCAR
1.00000000000000
9.0000000000000000 0.0000000000000000 0.0000000000000000
0.0000000000000000 9.0000000000000000 0.0000000000000000
0.0000000000000000 0.0000000000000000 9.0000000000000000
C H Cl
1 3 2
Direct
0.1570348572197245 0.2904054711139102 0.1422643997559632
0.1466469234176954 0.4066467848992589 0.1077433527138946
0.0469134772399311 0.2399491465236156 0.1544210764126938
0.2197893311177821 0.2820094213788985 0.2462070949679763
0.9809163623144840 0.4723904404063168 0.3674924467383788
0.2601754409903839 0.1874592103557934 0.9964911656110944
KPOINTS
Automatic 0 Gamma 1 1 1 0. 0. 0.
- For isolated atoms and molecules interactions between periodic images are negligible (in sufficiently large cells) hence no Brillouin zone sampling is necessary.
INCAR
PREC=Low EDIFF=1e-6 LWAVE=.FALSE. LCHARG=.FALSE. NELECT=22 NELMIN=4 LREAL=.FALSE. ALGO=VeryFast ISMEAR=-1 SIGMA=0.0516 ############################# MD setting ##################################### IBRION=0 # MD simulation NSW=1000 # number of steps POTIM=1 # integration step TEBEG=600 # simulation temperature MDALGO=11 # metaDynamics with Andersen thermostat ANDERSEN_PROB=0.10 # collision probability HILLS_BIN=50 # update the time-dependent bias # potential every 50 steps HILLS_H=0.005 # height of the Gaussian HILLS_W=0.05 # width of the Gaussian ##############################################################################
ICONST
R 1 5 5 R 1 6 5
- In contrast to the previous examples two collective variables are used simultaneously (and no combination of them).
PENALTYPOT
5.00000 1.00000 9.00000 0.50000 5.00000 2.00000 9.00000 0.50000 5.00000 3.00000 9.00000 0.50000 5.00000 4.00000 9.00000 0.50000 5.00000 5.00000 9.00000 0.50000 1.00000 5.00000 9.00000 0.50000 2.00000 5.00000 9.00000 0.50000 3.00000 5.00000 9.00000 0.50000 4.00000 5.00000 9.00000 0.50000
Calculation
Sometimes it is difficult to find one single parameter that approximates the reaction coordinate well but it is often possible to identify a small set of parameters that form a basis for the reaction coordinate. These parameters (collective variables) can be used in meta dynamics to determine free-energy surface. In this example we use two C-Cl distances as collective variables in the ICONST file. We still want to avoid the dissociation of the vdW complexes, which is an undesired process, hence we define an initial bias potential whose role is to ensure that no C-Cl distance becomes longer than (defined in the PENALTYPOT file).
Running the calculation
The mass for hydrogen in this example is set 3.016 a.u. corresponding to the tritium isotope. This way larger timesteps can be chosen for the MD.
The bias potential is specified in the PENALTYPOT file.
For practical reasons, we split our (presumably long) meta dynamics calculation into shorter runs of length of 1000 fs (NSW=1000; POTIM=1). At the end of each run the HILLSPOT file (containing bias potential generated in previous run) must be copied to the PENALTYPOT file (the input file with bias potential) - this is done automatically in the script run which looks as follows:
#!/bin/bash runvasp="mpirun -np x executable_path" # ensure that this sequence of MD runs is reproducible cp POSCAR.init POSCAR cp INCAR.init INCAR rseed="RANDOM_SEED = 311137787 0 0" echo $rseed >> INCAR i=1 while [ $i -le 100 ] do # start vasp $runvasp # ensure that this sequence of MD runs is reproducible rseed=$(grep RANDOM_SEED REPORT |tail -1) cp INCAR.init INCAR echo $rseed >> INCAR # use bias potential generated in previous mMD run cp HILLSPOT PENALTYPOT # use the last configuration generated in the previous # run as initial configuration for the next run cp CONTCAR POSCAR # backup some important files cp REPORT REPORT.$i cp vasprun.xml vasprun.xml.$i let i=i+1 done
- The user has to adjust the runvasp variable, which holds the command for the executable command.
- Please run this script by typing:
bash ./run
Time evolution of distance
During the simulation, the time evolution of collective variable can be monitored using the script timeEv.sh:
#!/bin/bash
rm timeEvol1.dat timeEvol2.dat
i=1
while [ $i -le 1000 ]
do
if test -f REPORT.$i
then
grep fic REPORT.$i |awk '{if (NR%2==1) {print $2} }' >>timeEvol1.dat
grep fic REPORT.$i |awk '{if (NR%2==0) {print $2} }' >>timeEvol2.dat
fi
let i=i+1
done
To execute this script type:
bash ./timeEv.sh
This script creates two files timeEvol1.dat and timeEvol2.dat, which hold the time evolution of the C-Cl distances for both Cl atoms. To visualize that file execute the following command:
gnuplot -e "set terminal jpeg; set xlabel 'timestep'; set ylabel 'Collective variable (Ang)'; set style data lines; plot 'timeEvol1.dat', 'timeEvol2.dat'" > timeEvol.jpg
The obtained time evolution of the collective variables should look like the following:
From this plot we very nicely see that at the beginning the two collective variables run parallel to each other, staying at the same side at approximately the same distance from the centre atom. At the