Starting from a given configuration (in many but not in all cases a minimum energy configuration), the MATLAB function mol_Dynamics.m propagates the molecular system according to Newton's equations of motion (Langevin and/or Smoluchowski should follow soon), thereby generating a trajectory with (hopefully!) constant energy (sampling an NVE ensemble). Alternatively, a simulation for constant temperature (sampling an NVT ensemble) can be run by using a numerical "thermostat". Implementation of a "barostat" (sampling an NPT ensemble) for simulations at constant pressure coming soon ...
The initial minimum energy geometry is either constructed from model functions or it will beread from the head of an xyz-file. The time evolution of the atomic position can be written to an xyz-file named nve...xyz or nvt...xyz in certain time intervals. These results can be visualized as a movie (e.g. using JMOL or VMD software).
Note that function mol_Initialize.m has to be run previously in order to initialize all variables in use. Of particular interest are the following structures:
Generation of initial conditions
Propagators
Thermostats
Wiki: Developers.Files.xyz
Wiki: Developers.Variables.dynamics.md
Wiki: Developers.Variables.dynamics.tmp
Wiki: Developers.Variables.dynamics
Wiki: Developers.Variables.initial
Wiki: Developers.Variables.inter
Wiki: Developers.Variables.intra
Wiki: Developers.Variables.molecule
Wiki: Developers.Variables.simulation
Wiki: Users.Main
Wiki: Users.Programs.mol_Initialize