Gibbs-Duhem integration

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History

The so-called Gibbs-Duhem Integration referes to a number of methods that couple molecular simulation techniques with thermodynamic equations in order to draw phase coexistence lines.

The method was proposed by Kofke (Ref 1-2).

Basic Features

Consider two thermodynamic phases: $a$ and $b$, at thermodynamic equilibrium at certain conditions. The thermodynamic equilibrium implies:

• Equal temperature in both phases: $T=T_a=T_b$, i.e. thermal equilbirum.
• Equal pressure in both phases $p=p_a=p_b$, i.e. mechanical equilbrium.
• Equal chemical potentials for the components ${\mu }_i={\mu }_{ia}={\mu }_{ib}$, i.e. material equilibrium.

In addition if we are dealing with a statistical mechanics model, with certain parameters that we can represent as $\lambda$ , the model should be the same in both phases.

Example: phase equilibria of one-compoment system

Notice: The derivation that follows is just a particular route to perform the integration

• Consider that at given conditions of $T,p,\lambda$ two phases of the systems are at equilibrium, this implies:

${\mu }_a(T,p,\lambda )={\mu }_b(T,p,\lambda )$

Given the thermal equilibrium we can also write:

$\beta {\mu }_a(\beta ,\beta p,\lambda )=\beta {\mu }_b(\beta ,\beta p,\lambda )$

where

• $\beta =1/k_{B}T$, where $k_B$ is the Boltzmann constant

When a differential change of the conditions is performed we wil have for any phase:

$d(\beta \mu )={[\frac{\partial (\beta \mu )}{\partial \beta }]}_{\beta p,\lambda }d\beta +{[\frac{\partial (\beta \mu )}{\partial (\beta p)}]}_{\beta ,\lambda }d(\beta p)+{[\frac{\partial (\beta \mu )}{\partial \lambda }]}_{\beta ,\beta p}d\lambda .$

Taking into account that $\mu$ is the Gibbs free energy per particle

$d(\beta \mu )=\frac{E}{N}d\beta +\frac{V}{N}d(\beta p)+{[\frac{\partial (\beta \mu )}{\partial \lambda }]}_{\beta ,\beta p}d\lambda .$

Let us use a bar to design quantities divided by the number of particles: e.g. $\overline{E}=E/N;\overline{V}=V/N$; and taking into account the definition:

$\overline{L}\equiv \frac{1}{N}{[\frac{\partial (\beta \mu )}{\partial \lambda }]}_{\beta ,\beta p}$

Again, let us suppose that we have a phase coexistence at a point given by $[{\beta }_0,(\beta p{)}_0,{\lambda }_0]$ and that we want to modify slightly the conditions. In order to keep the system at the coexistence conditions:

$d[\beta {\mu }_a-\beta {\mu }_b]=0$

Therefore, to keep the system on the coexistence conditions, the changes in the variables $\beta ,(\beta p),\lambda$ are constrained to fulfill:

$(\mathrm{\Delta }\overline{E})d\beta +(\mathrm{\Delta }\overline{V})d(\beta p)+(\mathrm{\Delta }\overline{L})d\lambda =0$

References

1. David A. Kofke, Gibbs-Duhem integration: a new method for direct evaluation of phase coexistence by molecular simulation, Mol. Phys. 78 , pp 1331 - 1336 (1993)
2. David A. Kofke, Direct evaluation of phase coexistence by molecular simulation via integration along the saturation line, J. Chem. Phys. 98 ,pp. 4149-4162 (1993)