Gibbs free energy - Definition


Gibbs free energy - Definition

In thermodynamics the Gibbs free energy is a state function of any system defined as

G = H − T·S

where

G is the Gibbs free energy, measured in joules

H is the enthalpy, measured in joules

T is the temperature, measured in kelvins

S is the entropy, measured in joules per kelvin

The Gibbs free energy is one of the most important thermodynamic functions for the characterization of a system.

The Gibbs free energy determines outcomes such as the voltage of an electrochemical cell, and the equilibrium constant for a reversible reaction. Gibbs free energy also determines how much work is attainable for any given process.

Any natural process occurs spontaneously if and only if the associated change in G for the system is negative (<math>\Delta G<math> < 0). Likewise, equilibrium is reached when the associated change in G for the system is zero (<math>\Delta G<math> = zero). And, no spontaneous process will occur if the final value of G is positive, or, greater than zero.

It is named after American chemist Willard Gibbs.

Contents

1 Useful identities

2 Derivation of Gibbs Free Energy

2.1 Back to Entropy

3 See also

Useful identities

<math>\Delta G = \Delta H - T \Delta S \,<math>

<math>\Delta G = -R T \ln K \,<math>

<math>\Delta G = -nF \Delta E \,<math>

and rearranging gives

<math>nF\Delta E = RT \ln K \,<math>

which relates the electrical potential of a reaction to the equilibrium coefficient for that reaction.

where

ΔG = change in Gibbs free energy

ΔH = change in enthalpy

T = temperature

ΔS = change in entropy

R = gas constant

ln = natural logarithm

K = equilibrium constant

n = number of electrons/mole product

F = Faraday constant (coulombs/mole)

ΔE = electrical potential of the reaction

Derivation of Gibbs Free Energy

Let S_tot be the total entropy of a thermally closed system. A closed system cannot exchange heat with its surroundings. Total entropy is only defined for a closed system, an open system has internal entropy instead.

The second law of thermodynamics states that if a process is possible, then

<math> \Delta S_{tot} \ge 0 \,<math>

and if <math> \Delta S_{tot} = 0 \,<math> then the process is reversible.

Since the heat transfer ΔQ vanishes for a closed system, then any reversible process will be adiabatic, and an adiabatic process is also isentropic <math> \left( {\Delta Q \over T} = \Delta S = 0 \right) \,<math>.

Now consider an open system. It has internal entropy S_int, and the system is thermally connected to its surroundings, which have entropy S_ext.

The entropy form of the second law does not apply directly to the open system, it only applies to the closed system formed by both the system and its surroundings. Therefore a process is possible iff

<math> \Delta S_{int} + \Delta S_{ext} \ge 0 \,<math>.

We will try to express the left side of this inequation entirely in terms of internal state functions. ΔS_ext is defined as:

<math> \Delta S_{ext} = - {\Delta Q \over T} \,<math>

Temperature T is the same both internally and externally, since the system is thermally connected to its surroundings. Also, ΔQ is heat transferred to the system, so -ΔQ is heat transferred to the surroundings, and −ΔQ/T is entropy gained by the surroundings. We now have:

<math> \Delta S_{int} - {\Delta Q \over T} \ge 0 \,<math>

Multiply both sides by T:

<math> T \Delta S_{int} - \Delta Q \ge 0 \,<math>

ΔQ is heat transferred to the system; if the process is now assumed to be isobaric, then ΔQ = ΔH:

<math> T \Delta S_{int} - \Delta H \ge 0\, <math>

ΔH is the enthalpy change of reaction (for a chemical reaction at constant pressure and temperature). Then

<math> \Delta H - T \Delta S_{int} \le 0 \,<math>

for a possible process. Let the change ΔG in Gibbs free energy be defined as

<math> \Delta G = \Delta H - T \Delta S_{int} \,<math> (1)

Notice that it is not defined in terms of any external state functions, such as ΔS_ext or ΔS_tot. Then the second law becomes:

<math> \Delta G < 0 \,<math> irreversible reaction

<math> \Delta G = 0 \,<math> reversible reaction

<math> \Delta G > 0 \,<math> impossible reaction

Gibbs free energy G itself is defined as

<math> G = H - T S_{int} \,<math> (2)

but notice that to obtain equation (2) from equation (1) we must assume that T is constant.

Thus, Gibbs free energy is most useful for thermochemical processes at constant temperature and pressure: both isothermal and isobaric. Such processes do not seem to move on a P-V diagram; they do not seem to be dynamic at all. However, chemical reactions do undergo changes in chemical potential, which is a state function. Thus, thermodynamic processes are not confined to the two dimensional P-V diagram. There is at least a third dimension for n, the quantity of gas.

Back to Entropy

If a closed system (ΔQ = 0) is at constant pressure (ΔQ = ΔH), then

<math> \Delta H = 0 \,<math>

Therefore the Gibbs free energy of a closed system is:

<math> \Delta G = -T \Delta S \,<math>

and if <math> \Delta G \le 0 \,<math> then this implies that <math> \Delta S \ge 0 \,<math>, back to where we started the derivation of ΔG.