# Open SourceMolecular Dynamics

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exercises:2017_ethz_mmm:pythonmd

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 exercises:2017_ethz_mmm:pythonmd [2017/03/02 15:16]dpasserone created exercises:2017_ethz_mmm:pythonmd [2017/03/03 16:38] (current)dpasserone 2017/03/03 16:38 dpasserone 2017/03/03 16:37 dpasserone 2017/03/03 11:03 dpasserone 2017/03/03 05:55 dpasserone 2017/03/03 05:54 dpasserone 2017/03/03 05:50 dpasserone 2017/03/03 05:48 dpasserone 2017/03/03 05:26 dpasserone 2017/03/03 05:25 dpasserone 2017/03/03 04:47 dpasserone 2017/03/02 16:14 dpasserone 2017/03/02 15:16 dpasserone created Next revision Previous revision 2017/03/03 16:38 dpasserone 2017/03/03 16:37 dpasserone 2017/03/03 11:03 dpasserone 2017/03/03 05:55 dpasserone 2017/03/03 05:54 dpasserone 2017/03/03 05:50 dpasserone 2017/03/03 05:48 dpasserone 2017/03/03 05:26 dpasserone 2017/03/03 05:25 dpasserone 2017/03/03 04:47 dpasserone 2017/03/02 16:14 dpasserone 2017/03/02 15:16 dpasserone created Line 1: Line 1: - <​code> ​STAMI ​ + ====== 38 atom Lennard-Jones cluster: molecular dynamics with python ====== + ===== + In this exercise you will perform molecular dynamics with a python program that you may inspect and modify directly. Then, you will perform the same kind of dynamics using cp2k and compare the performance. ===== + + + + All files of this exercise be downloaded from the wiki: {{e2_bis.zip|}} + Download the exercise into your $HOME folder and unzip it. + + <​code>​ + you@eulerX ~$ wget http://​www.cp2k.org/​_media/​exercises:​2017_ethz_mmm:​e2_bis.zip + you@eulerX ~$unzip exercises:​2017_ethz_mmm:​e2_bis.zip + you@eulerX ~$ cd exercise_2 + ​ + + ​ + + The instructions for loading the appropriate modules in .bashrc: + <​code>​ + > cd + > nano .bashrc + module load new gcc/4.8.2 python/​2.7.12 # include this line in the file + > . .bashrc + ​ + To visualize an **xyz** file: + <​code>​ + > ipython + + In [1]: from ase.io import read + In [2]: from ase.visualize import view + In [3]: s=read("​file.xyz"​) + In [4]: view(s) + + ​ + At this point you can rotate the structure, select an atom, then two (you get the distance) or three (you get the angle)... + ​ + + + In the repository you will find the program “**md.py**” and the geometry file “**fcc_r.xyz**” + The program md.py can perform a MD simulation for a system of Ar atoms interacting via Lennard-Jones potential. + + Executing the command + + <​code>​ + >python md.py + ​ + the program will ask you to provide + + + - the name of a geometry file + - the timestep to be used for the simulation in [fs] + - the total number of steps of dynamics to be performed + - the initial temperature desired for the system in [K] + ​ + + At this point a window like that should open: + + {{:​exercises:​2017_ethz_mmm:​screen_shot_2017-03-03_at_05.47.25.png?​nolink&​600|}} + + The program will show two graphs wile the MD simulation is running. The graph on the left contains the total energy of the system **Etot** that should remain constant along the simulation and the potential energy of the system “Epot”. + **Etot=Epot+Ekin** where Ekin is the kinetic energy of the system. + + At the end of execution the plot will be saved in the working directory as **plots.png**. You can visualize it by giving the command + <​code>​ + > display plots.png + ​ + + and data for the energy and temperature at each step will be saved on the file **data.out**. You can visualize the graphs using **gnuplot**:​ + for the time vs. temperature:​ + <​code>​ + > gnuplot + gnuplot> plot '​data.out'​ u 2:7 w l + ​ + + + ​ + - **TASK 1** Execute the program with input parameters:​ + * 0.5 as timestep + * 1000 as total number of steps + * 20 as initial temperature for the system + + Is the total energy conserved?​ + Is the temperature of the system conserved?​ + + - **TASK 2** Execute the program with input parameters + * 1.8 as timestep + * 1000 as total number of steps + * 80 as initial temperature for the system + + + Is the total energy conserved?​ + ​ + + Copy the program **md.py** into **md_original.py** and edit the file **md.py** (using **nano**). Have a look at the structure of the program + At the beginning two functions are defined: + + **ekin(m,​v)** needs as input the mass of each atom and its velocity; computes the kinetic energy of the system. + + **forces_pot(pos,​sigma,​epsilon)** needs as input the positions and the Lennard-Jones parameters to compute the potential energy of the system and the force on each atom. Then the program will: + + * define the input parameters + * define atomic units and convert input data into atomic units + * initialize randomly velocities and rescale them to the desired initial temperature ​ * + * define variables used for the graphs + + Finally the main loop of the dynamics starts, and it contains a final block needed to produce the graphs. + + Have a look at the function to compute the forces and the potential energy. A potentially very slow version of the algorithm is commented “#” (it would be very slow in an efficient fortran or C code that is compiled without optimization). + The active version of the algorithm is supposed to be faster. + Deactivate printing of data and production of the graphs by setting to **False** the two variables + ​graphs=“False” + prints=“False”​ + execute three or four times the program and write down the execution time that you get as the only output. + Now comment the lines for the “efficient” algorithm and uncomment the lines of the ”unefficient” one. Execute 3-4 times. + Is the execution time longer? Why do you think you get such a result? + + ​ + - **TASK 3** Initializing randomly the velocities of a finite system, the system will have a non zero total linear momentum and total angular momentum. + In the code we remove the total linear momentum after the initialization. + + Find the section of the code that removes the initial linear momentum. What could you do to remove the initial angular momentum? (no need to write down the code, just think how you could do) + ​ + + + ---- + + ====== Molecular dynamics using CP2K ====== + In this second part of the exercise, the same kind of dynamics will be performed with **cp2k**. You will find in the repository (zip file) the input file **md.inp**, where the **&​MOTION** section is different from the last lecture exercise. + + <​code>​ + &​MOTION + &​PRINT + &​RESTART_HISTORY OFF + &END + &​RESTART + &EACH + MD 5000 + &END + &END + &​TRAJECTORY + &EACH + MD 100 + &END + &END + &END + &MD + ENSEMBLE NVE + STEPS 10000 + TIMESTEP 0.5 + TEMPERATURE 10.0 + &END MD + &END MOTION + ​ + + ​ + - Run the code + <​code>​ + > cp2k.popt -i md.inp > md.out + ​ + Compare the performance with the one of the python code. What do you notice? + Plot the energy by using the file **MD-1.ener** and **gnuplot** + -  What is the value of the total energy? Is it conserved?​ + -  Increase the time step to 3 fs, and run it again. What happens to the total energy? + - Note: to visualize a trajectory you can use the code (look inside it!) traj.py in the directory:​ + <​code>​python traj.py​ + ​ + + ​Here an example of [[http://​users.mccammon.ucsd.edu/​~dzhang/​energy-unit-conv-table.html|energy conversion table]]. ​ + + +
exercises/2017_ethz_mmm/pythonmd.1488467813.txt.gz · Last modified: 2017/03/02 15:16 by dpasserone