Step 1: Identify ensemble constraints.
The ensemble has fixed:
• Number of particles,
• Pressure,
• Temperature (N, P, T).
Step 2: Connect constraints to thermodynamic potentials.
Each ensemble is described by a thermodynamic potential that is minimised under its natural variables:
• Helmholtz free energy $F$ → natural variables $(T, V)$,
• Gibbs free energy $G$ → natural variables $(T, P)$,
• Enthalpy $H$ → natural variables $(S, P)$.
Step 3: Compare with given ensemble.
Since the ensemble is at fixed $(T,P)$, the appropriate potential is Gibbs free energy $G=H-TS$.
Step 4: Conclusion.
The thermodynamic function describing such an ensemble is the Gibbs free energy.
