To obtain the true thermodynamic equilibrium of systems of anisotropic mole
cules is difficult because of the complicated potential lanscape. There is
a high probability that simulated system may be caught in one of the many l
ocal minima. Especially, simulated systems of anisotropic molecules often y
ield anisotropic pressure under periodic boundary conditions. The situation
is especially critical for high density phases such as crystal and smectic
.
We discuss how to simulate the thermodynamic equilibrium under hydrostatic
pressure, and investigate the properties of crystal-smectic transition.