How to Derive a Thermodynamic Relation from Helmholtz Free Energy
At a glance
- 1. Write the differential
For a fixed-composition, simple compressible system, use dF = −S dT − P dV.
- 2. Read off derivatives
Identify entropy and pressure as derivatives of Helmholtz free energy with respect to temperature and volume.
- 3. Differentiate internal energy
Use U = F + TS, then differentiate with respect to volume at constant temperature.
- 4. Apply a Maxwell relation
Equality of mixed derivatives gives (∂S/∂V)T = (∂P/∂T)V, yielding the desired identity.
The Helmholtz free energy is a useful thermodynamic potential when temperature and volume are the natural variables. Its differential gives direct formulas for entropy and pressure. From those formulas, you can derive a frequently used identity connecting the volume dependence of internal energy to the temperature dependence of pressure:
This relation applies to an equilibrium, simple compressible system with fixed composition. The derivation also shows why it gives zero for an ideal gas and a nonzero result for a van der Waals gas.
Start with the Helmholtz free energy
Define the Helmholtz free energy as
where is internal energy, is absolute temperature, and is entropy. For a fixed amount of a simple compressible substance, the first law in differential form is
Differentiate :
Substituting the first-law expression for cancels the terms, leaving
Thus, when is regarded as a function of its natural variables and ,
These are the entropy and pressure identities for the Helmholtz free energy.
Derive the internal-energy relation
Rearrange the definition of to write the internal energy as
At fixed temperature, differentiate with respect to volume:
The first term is . To rewrite the second term, use the fact that the mixed second derivatives of a well-behaved state function are equal. From the entropy and pressure identities,
This is a Maxwell relation. Substituting it gives
The right-hand side uses the equation of state: how pressure varies with temperature when volume is held fixed. The left-hand side is the change in internal energy per change in volume at fixed temperature.
Worked example: a van der Waals gas
For moles, the van der Waals equation of state is
where and are constants describing intermolecular attraction and excluded volume. Differentiate with respect to temperature at fixed volume:
Now substitute this and the equation of state into the derived identity:
So at fixed temperature, increasing the volume increases the internal energy in this model. Integrating with respect to gives
where is an undetermined function of temperature. The equation of state alone determines the volume-dependent part, not the full temperature-dependent contribution.
Check: the ideal gas
For an ideal gas, , so
Therefore : the internal energy of an ideal gas depends only on temperature, not volume. This is a result of the ideal-gas equation of state, not a general rule for all gases.
Common mistakes
- Dropping the minus sign in the pressure identity: Since , pressure is .
- Holding the wrong variable fixed: The pressure derivative in the result is at constant volume; the internal-energy derivative is at constant temperature.
- Assuming the ideal-gas result applies to every substance: Real-gas interactions can make internal energy depend on volume even at fixed temperature.
- Confusing Helmholtz and Gibbs free energy: Helmholtz free energy has natural variables ; Gibbs free energy has natural variables for a simple compressible system.
References
- Thermodynamics and an Introduction to Thermostatistics — Herbert B. Callen
- Heat and Thermodynamics — Mark W. Zemansky and Richard H. Dittman
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