Monte Carlo simulations in the isothermal-isobaric ensemble: use of a ‘shell’ particle for simulating polyatomic fluids

Abstract

ABSTRACTThe recent reformulation of the isothermal-isobaric ensemble requires the use of a ‘shell’ particle to define uniquely the volume of the system, thereby avoiding the redundant counting of configurations. A previous modification of the Monte Carlo method, in which trial moves are generated and accepted consistent with the correct constant pressure partition function, is extended here to the case of polyatomic fluids. With a ‘shell’ molecule, either the centre of mass of the molecule or the location of any one of the atoms within the molecule can be chosen to define the system volume. Ensemble averages obtained with the use of the shell molecule differ from ensemble averages determined with the old (i.e. no shell particle) Monte Carlo algorithm, specifically for small system sizes, although both sets of averages become equal, as they must, in the thermodynamic limit. Monte Carlo simulations in the constant pressure ensemble for various Lennard-Jones polyatomic fluids, both for pure component and binary mixtures, demonstrate these differences for small systems. For mixtures, Monte Carlo simulations may include attempted identity swaps for the shell molecule, as the choice of which component serves as the shell molecule is arbitrary when periodic boundary conditions are applied.