This section explores Gibbs Free Energy, a thermodynamic quantity used to predict the spontaneity or feasibility of a chemical reaction under constant temperature and pressure.
Gibbs free energy () is a measure of the amount of useable energy (or work-potential) in a system at constant temperature and pressure. It is also known as "Available Energy." It was conceptualized by the American scientist Josiah Willard Gibbs in 1876.
The Gibbs free energy of a system is defined by the equation:
Where:
Gibbs free energy is a state function, meaning its value depends only on the current state of the system, not on the path taken to reach that state.
For a chemical process, we are interested in the change in Gibbs free energy (). The change is given by the Gibbs-Helmholtz equation for a process at constant temperature:
Where:
The sign and magnitude of determine whether a reaction is spontaneous (feasible), non-spontaneous, or at equilibrium. A feasible reaction is one that, once started, will proceed to completion without a continuous supply of external energy.
The three possible conditions are:
| Value of | Description | Characteristics |
|---|---|---|
| (negative) | Spontaneous / Feasible | The reaction proceeds in the forward direction. The system releases free energy. |
| (positive) | Non-spontaneous / Not Feasible | The reaction does not proceed in the forward direction. Energy must be supplied for it to occur. The reverse reaction is spontaneous. |
| At Equilibrium | The rates of the forward and reverse reactions are equal. There is no net change in the system. |
The feasibility of a reaction depends on the balance between enthalpy () and entropy ().
is also useful for understanding phase transitions, such as the melting of ice into liquid water.
Reaction:
The standard free energy change is related to the equilibrium constant of a reaction by the following expression: Or in terms of base 10 logarithm: