exercises:2015_ethz_mmm:md_ala
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| exercises:2015_ethz_mmm:md_ala [2015/03/09 15:15] – yakutovich | exercises:2015_ethz_mmm:md_ala [2020/08/21 10:15] (current) – external edit 127.0.0.1 | ||
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| <note warning> | <note warning> | ||
| TO USE THE FUNCTION LIBRARY (VERSION UP TO DATE) IN THE INTERACTIVE SHELL: | TO USE THE FUNCTION LIBRARY (VERSION UP TO DATE) IN THE INTERACTIVE SHELL: | ||
| - | you@eulerX ~$ module load courses mmm vmd ; mmm-init | + | |
| + | you@eulerX ~$ module load courses mmm vmd | ||
| + | |||
| + | you@eulerX ~$ mmm-init | ||
| </ | </ | ||
| Line 21: | Line 24: | ||
| - | <note tip> | ||
| - | Concerning temperature control, in these exercises we will use the NOSE-HOOVER chains method. This has been briefly described in the lecture, and is presented in [[doi> | ||
| - | </ | ||
| Line 34: | Line 34: | ||
| <note tip> | <note tip> | ||
| - | All files of this exercise (**input and scripts are all commented**) can be also downloaded from the wiki: {{exercise_4.1.zip|exercise_4.1.zip}}</ | + | All files of this exercise (**all |
| + | </ | ||
| You will start from a configuration already computed in the second lecture (**inp.a.pdb**) which is included in the repository of this exercise as well. | You will start from a configuration already computed in the second lecture (**inp.a.pdb**) which is included in the repository of this exercise as well. | ||
| - | Use the file **inp.nve** for the first simulation, which is a constant energy simulation. | + | Update the following part of the file **inp.nve** for the first simulation: |
| + | |||
| <code - md_part.inp.nve> | <code - md_part.inp.nve> | ||
| & | & | ||
| - | | + | |
| - | | + | |
| - | | + | |
| - | | + | |
| &END MD | &END MD | ||
| + | </ | ||
| + | <note tip> | ||
| + | To get more information, | ||
| + | http:// | ||
| + | </ | ||
| + | |||
| + | * Perform a constant energy simulation, 100000 time steps, with a time step of 1 fs. Use 100 K as an initial temperature! | ||
| + | |||
| + | <code bash> | ||
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.nve -o out.nve | ||
| </ | </ | ||
| + | <note tip> | ||
| + | Assignments: | ||
| + | - We are performing MD at a constant energy, but why we still have to define the temperature? | ||
| + | </ | ||
| - | * Perform a constant energy simulation, 100000 time steps, with a time step of 1 fs. | + | * Make four copies of the previous input file (say inp.nve_0.1, inp.nve_2.0, inp.nve_3.0, |
| + | * Perform the simulations with all these input files: | ||
| <code bash> | <code bash> | ||
| - | you@eulerX | + | you@eulerX |
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.nve_2.0 -o out.nve_2.0 | ||
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.nve_3.0 -o out.nve_3.0 | ||
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.nve_4.0 -o out.nve_4.0 | ||
| </ | </ | ||
| - | | + | |
| - | - Access | + | <note tip> |
| - | <note important> | + | Assignments |
| + | - Do you see the energy conservation? | ||
| + | - Analyse | ||
| + | </ | ||
| - | - Perform now a constant Temperature simulation. The system is in contact with a thermostat, and the conserved quantity includes the thermostat degrees of freedom. The first simulation is done at 100 K: **inp.100** | + | <note important> |
| - | - Then, perform a simulation at 300 K, using the restart file from the previous simulation: **inp.300**. | + | Hint (plotting |
| - | - Now you have some outputs to study with vmd. | + | |
| - | The trajectory files we are going to study are | + | To plot the Kinetic energy: |
| + | <code bash> | ||
| + | gnuplot> plot " | ||
| + | </ | ||
| + | To plot the Potential energy: | ||
| + | <code bash> | ||
| + | gnuplot> plot " | ||
| + | </ | ||
| + | To plot the Temperature: | ||
| + | <code bash> | ||
| + | gnuplot> plot " | ||
| + | </ | ||
| + | |||
| + | |||
| + | </ | ||
| + | |||
| + | Now you will perform a constant Temperature simulations, | ||
| + | |||
| + | <note tip> | ||
| + | Concerning temperature control, in these exercises | ||
| + | </ | ||
| + | |||
| + | In cp2k input files you should again have a look at the following section: | ||
| + | <code - md_part.inp.300> | ||
| + | & | ||
| + | ???????? ??? ! Please specify the appropriete ensemble for you MD simulation | ||
| + | ????? ?????? | ||
| + | ???????? ??? ! Please specify the length of an integration step | ||
| + | ??????????? ??? ! Please specify the temperature of the simulation | ||
| + | &?????????? | ||
| + | &???? | ||
| + | TIMECON 50 ! Timeconstant of the thermostat chain | ||
| + | LENGTH 3 ! Length of the Nose-Hoover chain | ||
| + | YOSHIDA 3 ! Order of the yoshida integretor used for the thermostat | ||
| + | &??? | ||
| + | &??? | ||
| + | &END MD | ||
| + | </ | ||
| + | |||
| + | Edit the inp.100 file (Put there: NVT ensemble, 100000 steps of simulation, 100 K, Nose-Hoover thermostat and 1.0 fs of timestep). The first simulation is done at 100 K: | ||
| + | <code bash> | ||
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.100 -o out.100 | ||
| + | </ | ||
| + | * Then, perform another simulation, using the restart file from the previous simulation: **inp.300**. But first you have to edit it exactly like in the previous case, but **put 300 K** instead of 100 K | ||
| + | <code bash> | ||
| + | you@eulerX exercise_4.1$ bsub cp2k.popt -i inp.300 -o out.300 | ||
| + | </ | ||
| - | < | + | Now you have the following outputs to study with vmd: |
| + | < | ||
| + | nve_md-pos-1.pdb | ||
| md.100-pos-1.pdb | md.100-pos-1.pdb | ||
| md.300-pos-1.pdb | md.300-pos-1.pdb | ||
| </ | </ | ||
| - | " | + | * Open (for example) nve_md-pos-1.pdb |
| - | From the Extensions menu, you can choose the Tk console. And from there, you can enter | + | |
| - | < | + | < |
| + | vmd nve_md-pos-1.pdb | ||
| + | </ | ||
| - | which will define the two dihedrals | + | * Open Tk Console (Extensions menu > Tk console). And to define the two dihedrals |
| - | You can also pick from the extensions the "RMSD trajectory tool" and use it to align the molecule along the trajectory. Remember to replace " | + | |
| - | Using "Labels" | + | <code tcl> |
| + | vmd> source | ||
| + | </ | ||
| - | < | + | You can also pick from the extensions the "RMSD trajectory tool" and use it to align the molecule along the trajectory (Extensions> |
| + | |||
| + | * Now using " | ||
| + | - Go to Graphics > Labels | ||
| + | - In the drop-down list chose Dihedrals | ||
| + | - Chose both dihedrals in the list | ||
| + | - Go to the " | ||
| + | - Press on the " | ||
| + | - (Optional) save these graps in a text file (File > Export to ASCII matrix...) | ||
| + | |||
| + | < | ||
| + | Which differences do you notice between the nve, the 100 K and the 300 K case? Can you explain them? | ||
| + | </ | ||
exercises/2015_ethz_mmm/md_ala.1425914139.txt.gz · Last modified: (external edit)
