Reference: Daniel V. Schroeder, An Introduction to Thermal Physics, (Addison-Wesley, 2000) – Problem 5.1.
One of the confusing things about thermodynamics is the number of energy functions in use. We’ve already met the internal (kinetic) energy and the enthalpy, defined as
The enthalpy is the total energy required to create the system from nothing, in which the environment at constant pressure must be pushed back to create the volume in which the new system is to be stored. Thus the enthalpy is effectively the energy of the system in constant pressure environments.
The Helmholtz free energy (other sources call it ) is defined as
Schroeder’s description of this definition is rather vague, since he claims that is the work required to create a system out of nothing, if the system is in contact with a thermal reservoir so that its temperature is held constant at . This arises because for isothermal, reversible processes, the entropy absorbed from a thermal reservoir is , so is the contribution of the reservoir to the total energy ; thus the difference must be the work required to produce the system.
However, in the definition of enthalpy, the total energy of a system created at constant pressure is the sum of and the work required to make room for the system by pushing back the atmosphere. Thus it would seem that excludes the work required to make room for the system.
Other sites on the web point out that is actually the work required to create the system at constant temperature and constant volume. That is, space has already been cleared for the system, which is then placed in contact with the reservoir so it can absorb the heat . Any extra energy required to top up the total energy to the value must then be provided by doing work (for example, electrical work, which doesn’t change the volume) on the system.
The Gibbs free energy is then defined as the Helmholtz free energy plus the work required to make room for the system at constant pressure:
The four energies , , and are known as thermodynamic potentials.
As an example, we’ll look at one mole of argon gas at room temperature (298 K) and atmospheric pressure (). We’ve already worked out , and for this system:
The other potentials are
Since in practice, only differences in energy are measured, the fact that and are negative shouldn’t worry us.