Thermodynamic integration

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Thermodynamic integration is used to calculate the difference in the Helmholtz energy function, , 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)

Isothermal integration

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

Isobaric integration

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

where is the Gibbs energy function and is the enthalpy.

Isochoric integration

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

where is the internal energy.

See also

References

  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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