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=Ta=Tb, i.e. thermal equilbirum.
  • Equal pressure in both phases p=pa=pb, i.e. mechanical equilbrium.
  • Equal chemical potentials for the components μi=μia=μib, i.e. material equilibrium.

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

Example: phase equilibria of one-component system

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

  • Consider that at given conditions of T,p,λ two phases of the systems are at equilibrium, this implies:
μa(T,p,λ)=μb(T,p,λ)

Given the thermal equilibrium we can also write:

βμa(β,βp,λ)=βμb(β,βp,λ)

where

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

d(βμ)=[∂(βμ)∂β]βp,λdβ+[∂(βμ)∂(βp)]β,λd(βp)+[∂(βμ)∂λ]β,βpdλ.

Taking into account that μ is the Gibbs free energy per particle

d(βμ)=ENdβ+VNd(βp)+[∂(βμ)∂λ]β,βpdλ.

where:

  • E is the internal energy
  • V is the volume
  • N is the number of particles

E,V are the mean values of the energy and volume for a system of N particles in the isothermal-isobaric ensemble

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

L¯≡[∂(βμ)∂λ]β,βp

Again, let us suppose that we have a phase coexistence at a point given by [β0,(βp)0,λ0] and that we want to modify slightly the conditions. In order to keep the system at the coexistence conditions:

d[βμa−βμb]=0

Therefore, to keep the system on the coexistence conditions, the changes in the variables β,(βp),λ are constrained to fulfill:

(ΔE¯)dβ+(ΔV¯)d(βp)+(ΔL¯)dλ=0

whrere for any porperty X we can define: ΔX≡Xa−Xb (i.e. the difference between the values of the property in the phases). Taking a path with, for instance constante β, the coexistence line will follow the trajectory produced by the solution of the differential equation:

d(βp)=−ΔL¯ΔV¯dλ. (Eq. 1)

The Gibbs-Duhem integration technique, for this example, will be a numerical procedure covering the following tasks:

  • Computer simulation (for instance using Metropolis Monte Carlo in the NpT ensemble) runs to estimate the values of L¯,V¯ for both

phases at given values of [β,βp,λ].

  • A procedure to solve numerically the differential equation (Eq.1)

Peculiarities of the method (Warnings)

  • A good initial point must be known to start the procedure
  • The integrand of the differential equation is computed with some numerical uncertainty
  • Care must be taken to reduce (and estimate) possible departures from the correct coexistence lines

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)