# Thermodynamics of Solid and Fluid Surfaces

Entry by Emily Redston, AP 226, Spring 2012

Work in Progress

## Reference

*Thermodynamics of Solid and Fluid Surfaces* by J. W. Cahn. Segregation to Interfaces, ASM Seminar Series (1978) pp. 3-23.

## Keywords

## Introduction

In this paper, Cahn provides a slightly different take on Gibbs' original development of the thermodynamics of fluid and solid surfaces. His goal was to develop a mathematical system that was physically equivalent to Gibbs' formulation while being more easily applicable. The key change he made is that he concentrated on the system rather than defining excess quantities by comparing the actual system to a hypothetical system not containing the surface. This avoids problems with the identification of the location of the dividing surface.

## Plane Fluid Interfaces - Area Work Term

For surfaces between fluids, Gibbs defined surface tension <math>\sigma</math> in a work term. The quantity <math>\sigma</math> is taken as a force per unit length of surface perimeter. When a portion of the perimeter moves an infinitesimal distance in the place of the surface, the area change <math>dA</math> is the product of perimeter length and distance moved. Thus <math>\sigma dA</math> is a forces-times-distance work term, and it appears in the combined first and second laws of thermodynamics as follows:

Strictly speaking, <math>\sigma</math> is defined as the change in internal energy when the area is reversibly increase at constant entropy and volume in a closed system.

Gibbs then went on to show that, in equilibrium, temperature and chemical potentials are constant everywhere within the system. For the special case of plane boundaries at equilibrium, pressure is also constant. For a system containing a plane surface, Equation 1 is readily integrated to give:

This can be rearranged to give <math>\sigma</math>, the excess free energy due to the presence of the surface.

Here <math>U - TS + PV</math> is the Gibbs free energy of the system with the interface, and <math>\displaystyle \sum_{i} \mu_i dN_i</math> is the Gibbs free energy without the interface.

Equations [2] and [3] pertain to the entire system. Because most of this system is occupied by homogeneous phases, it is convenient to subtract out their contribution. Thus for homogeneous phases <math>\alpha</math> and <math>\beta</math>, we have: