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exercises:2015_ethz_mmm:md_slab [2015/03/09 16:49] yakutovichexercises:2015_ethz_mmm:md_slab [2015/03/19 22:05] dpasserone
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-This exercise deals with heating a gold slab, namely the (100) reconstructed that you already simulated last time. The goal is to plot a density profile in the direction orthogonal to the slab, and to compute (using vmd) the radial distribution function g(r) at various temperatures.+This exercise deals with heating a gold slab, namely the (100) reconstructed that you already simulated last time. The goal is to plot a density profile in the direction orthogonal to the slab, and to compute (using vmd) the radial distribution function g( r ) at various temperatures.
  
 Download the 4.2 exercise into your $HOME folder and unzip it: Download the 4.2 exercise into your $HOME folder and unzip it:
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-<note important>+<note tip>
   - Explain the profile, and use the third column to draw conclusions about the surface structure.   - Explain the profile, and use the third column to draw conclusions about the surface structure.
   - Study the source of the script. Understand its behavior.    - Study the source of the script. Understand its behavior. 
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 </note> </note>
  
-Perform a simulation at T=1100 K and T=1300 K (files: 1100.inp and 1300.inp).+  * Perform **consequently** a simulation at T=1100 K and T=1300 K (files: 1100.inp and 1300.inp)
 +<code bash> 
 +you@eulerX exercise_4.2$ bsub cp2k.popt -i 1100.inp -o 1100.out 
 +you@eulerX exercise_4.2$ bsub cp2k.popt -i 1300.inp -o 1300.out 
 +</code>
  
-<note important>Discuss the differences in the density profile. What do you expect to see in vmd?+  * And again analyze these trajectories using the script histo_z: 
 +<code bash> 
 +you@eulerX exercise_4.2$ ./histo_z 1100-1-pos.xyz 
 +you@eulerX exercise_4.2$ ./histo_z 1300-1-pos.xyz 
 +</code> 
 + 
 + 
 +<note tip> 
 +Discuss the differences in the density profile. What do you expect to see in vmd?
 </note> </note>
  
-Now, use vmd to look at the trajectories. As you launch vmd,  +  * Now, use vmd to look at the trajectories. As you launch vmd,  
-you can (assignment):+in Tk console you can:
  
-<note important> +Load a pbc.vmd file which includes the definition of the periodic box 
-- source a pbc.vmd file which includes the definition of the periodic box +<code tcl> 
-- draw the box: **draw pbcbox** in the Tk console +vmd> source pbc.vmd 
-- wrap all atoms in the periodic box: **pbc wrap -first first -last last** +</code> 
-- "playwith representations: try to color the surface atoms in one color, the bulk ones in another color. +Draw the box:  
-Using the "radial distribution function" plugin from the extension menu, draw the g(r) of the system. Discuss it for 700, 1100, and 1300 K. +<code tcl>  
 +vmd> draw pbcbox 
 +</code> 
 +Wrap all atoms in the periodic box: 
 +<code tcl> 
 +vmd> pbc wrap -first first -last last 
 +</code> 
 +  * Try to play with representations: color the surface atoms in one color, the bulk ones in another color. 
 +  Using the "radial distribution function" plugin from the extension menu (Extensions>Analysis>Radial Pair Distribution Function g( r ) ), draw the g( r ) of the system. 
 + 
 +<note tip> 
 + Discuss radial distribution function for 700, 1100, and 1300 K.  
 +Here how to use the g(r) module: 
 +1) First apply pbcs (see above) 
 +2) Open the radial distribution function plugin and enter the parameters as shown (from "Utilities" you can check that your unit cell is OK) 
 +3) Click "Compute g(r)" 
 +4) From the "File" menu of the graph window, you can save as postscript file or other formats
 </note> </note>
exercises/2015_ethz_mmm/md_slab.txt · Last modified: 2020/08/21 10:15 by 127.0.0.1