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Revision as of 13:50, 25 November 2007
Manual 01 for MD++
Introduction to MD++
Keonwook Kang and Wei Cai
Contents |
Overview
MD++ is a molecular dynamics simulation package written in C++. It is originally developed by Wei Cai when he was a graduate student at MIT and still being updated to include more features. MD++ is supposed to run in a Unix/Linux environment. However, if you have cygwin,<ref>For download and installation, visit http://www.cygwin.com/. You must download and install the full package of cygwin. See http://micro.stanford.edu/~caiwei/Forum/2004-12-12-MD++/cygwin.html for installation instructions.</ref> a linux-like environment installed in your Windows machine, you can also enjoy MD++ there. Currently, this code is designed mainly for studying the atomic behavior in solid crystal materials. It can also be extended to study other systems, such as fluids, polymers and bio-molecules. This document is the first of a series of manuals written for those new to MD simulations. These manuals explain how to use MD++ with simple examples.
Installation
The latest version of MD++ code can be downloaded from the web site,
http://micro.stanford.edu/~caiwei/Forum/2004-12-12-MD++/.
Here we assume that the reader is familiar with basic Unix/Linux shell
commands.<ref>For those who are not familiar with Unix/Linux
environment, we suggest the book A practical guide to Linux
commands, editors and shell programming by Mark G. Sobell. You can
also easily find several good web sties about the shell
commands.</ref> Before you download MD++ code, we recommend
that you make a sub-directory Codes in your home directory.
$ mkdir Codes $ cd Codes
Save the MD++ package in this directory(~/Codes). Suppose the downloaded file is md++-2007-01-07.tar.gz, then we can extract it by,
$ tar -zxvf md++-2007-01-07.tar.gz
This command creates the MD++ sub-directory and extracts all the files into it. Go to the MD++ directory and make a runs directory if it does not exist.
$ cd MD++; mkdir runs
To compile the codes in release(R) mode <ref>If build=R, MD++ is compiled with the -O3 option. By default(build=D), MD++ compiles as debug mode with the -g option. In release mode, the executabale files run faster but the compilation time is slightly longer than debug mode</ref> in a Linux system, type
$ make all build=R
In order to compile MD++ In a different system (such as Windows), you can specify the SYS variable in the command line, such as
$ make all build=R SYS=cygwin
provided that cygwin is installed. You can also compile MD++ code in an Apple/Machintosh computer, using
$ make all SYS=mac build=R
By default, SYS=gpp which corresponds to the GNU c++ compiler. If you have the intel c/c++ compiler icc in your system, use SYS=intel to activate icc, which produces much faster executables than GNU c++ compiler. For more SYS values, take a look at the file ~/Codes/MD++/src/Makefie.base. You may get an TCL-related error during compilation. You can bypass this error using, e.g.
$make SYS=cygwin TCL=no
by suppressing TCL option. After compilation, you have executable files such as fs_gpp, eam_gpp, and sw_gpp in the bin directory.<ref>If you use SYS=cygwin, the executable files would be fs_cygwin.exe, eam_cygwin.exe, etc.</ref> If you just want to compile one executable file, such as fs_gpp, use
$ make fs build=R
The name of each execution file stands for the potential model that will be used in the atomisitic simulation. For example, fs stands for the Finnis-Sinclair (FS) potential<ref>M. W. Finnis and J. E. Sinclair, Philos. Mag. A. 50 45 (1984)</ref> , lj for the Lennard-Jones (LJ) pair potential,<ref>J. E. Lennard-Jones, "Cohesion" Proceedings of the Physical Society 43 461-482 (1931)</ref> eam for the embedded-atom method (EAM) potential,<ref>M. S. Daw and M. I. Baskes, "Embedded-atom method: Derivation and application to impurities, surfaces, and
other defects in metals", Phys. Rev. B 29 6443 (1984)</ref> and sw
for the Stillinger-Weber (SW) potential.<ref>F. H. Stillinger and T. A. Weber, "Computer simulation of local order in condensed phases of silicon", Phys. Rev. B 31 5262 (1985)</ref><ref>H. Balamane, T. Halicioglu, and W. A. Tiller, "Comparative study of silicon empirical interatomic potentials", Phys. Rev. B 46 2250 (1992)</ref> Each potential model is applicable to a group of atomic species. For example, the FS potential was designed for body-centered-cubic (BCC) metals such as Mo, Ta and W. The SW potential was designed for diamond-cubic semiconductors such as Si and Ge. By the way, the executable md_gpp does not contain any potential model. Hence it cannot be used to compute any material properties but it can still be used to display atomic structures.
If you modify the source code (in the src directory), you need to recompile MD++. we recommend you to clean the previous executables and rebuild by typing,
$ make clean; make all build=R
To see more help on make, type
$ make help
To check if you successfully install and compile MD++, try to run one of example scripts in the Examples directory, e.g.
$ bin/fs_gpp scripts/Examples/example01-mo.script
If you want to stop MD++ running, press ctrl+c or close the visualization window.
MD++ Directories
After installation, the MD++ directory will contain the
following sub-directories.<ref>The new version of MD++ may have
different directories, but the main structure is still almost same.</ref>
| $ ls | |||||
| bin | Doc | makefile | potentials | scripts | Tools |
| CSD-book | Examples | matlab | README | src |
The contents in each directory are described below.
| src | source codes |
| bin | binary executable files generated by make |
| Doc | manuals |
| scripts | input script files for running MD++ |
| runs | where the simulation outputs are stored |
| potentials | potential files to read in |
| Examples | some example input script files |
| Tools | pre/post-simulation tools such as atomeye for visualization |
| matlab | useful Matlab codes. |
Script File
To execute a molecular simulation, the MD++ code reads an input script file, which contains a series of commands to run and variables to be assigned for the simulation. To create or modify a script file in a Unix/Linux environment, you can use vi, emacs, nedit or any of your favorite editors. For example,
$ vi scripts/example01-mo.script
or
$ emacs scripts/example01-mo.script &
You can see what is the format by opening one of example script files. All script files have a common head region,
# -*-shell-script-*- setnolog # No log file saved setoverwrite # Overwrite a log file dirname = runs/mo-example # Specify output directory
In a script file, you can commnet out a line
or a part of the line by the pound sign, #. You can use
# to leave your own comment or explanation anywhere in the
script.
The first line tells the Emacs editor to use the shell-script
mode to display the file.
The setnolog command tells MD++ not to create a log file and the outputs will be printed on the screen.
If setnolog is commented out, then the outputs will be redirected to a log file A.log in the output directory specified by the variable dirname.
The simulation stops whenever it reaches the quit
command. Sometimes it is useful to put sleep before the
quit command, such as
sleep quit # System gets sleep for 600 sec before quit.
The sleep command keeps the visualization window alive for a while during which we can look at the atomic structure. Other commands and variables in the scripts file will be explained in more detail later.
Visualization Window Control
Bibliography
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