Thermodynamic integration

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Thermodynamic integration is used to calculate the difference in the Helmholtz energy function, A, between two states. The path must be continuous and reversible, i.e., the system must evolve through a succession of equilibrium states (Ref. 1 Eq. 3.5)

ΔA=A(λ)−A(λ0)=∫λ0λ⟨∂U(r,λ)∂λ⟩λdλ

Isothermal integration[edit]

At constant temperature (Ref. 2 Eq. 5):

A(ρ2,T)NkBT=A(ρ1,T)NkBT+∫ρ1ρ2p(ρ)kBTρ2dρ

Isobaric integration[edit]

At constant pressure (Ref. 2 Eq. 6):

G(T2,p)NkBT2=G(T1,p)NkBT1−∫T1T2H(T)NkBT2dT

where G is the Gibbs energy function and H is the enthalpy.

Isochoric integration[edit]

At constant volume (Ref. 2 Eq. 7):

A(T2,V)NkBT2=A(T1,V)NkBT1−∫T1T2U(T)NkBT2dT

where U is the internal energy.

See also[edit]

References[edit]

  1. J. A. Barker and D. Henderson "What is "liquid"? Understanding the states of matter ", Reviews of Modern Physics 48 pp. 587 - 671 (1976)
  2. C. Vega, E. Sanz, J. L. F. Abascal and E. G. Noya "Determination of phase diagrams via computer simulation: methodology and applications to water, electrolytes and proteins", Journal of Physics: Condensed Matter 20 153101 (2008) (section 4)

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