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Chemistry · Ch 5 — Thermodynamics

Gibbs Energy and Spontaneity

5.6(c)

Gibbs Energy and Spontaneity

Gibbs Energy and Spontaneity

We have seen that it is the total entropy change, ΔStotal\Delta S_{\text{total}}, that decides the spontaneity of a process. But most chemical reactions occur in closed or open systems, not isolated ones. For such systems, there are changes in both enthalpy and entropy. Neither a decrease in enthalpy nor an increase in entropy alone can determine the direction of spontaneous change.

For this purpose, we define a new thermodynamic function: the Gibbs energy (or Gibbs function), GG:

G=H−TS(5.20)G = H - TS \qquad(5.20)

Gibbs energy GG is an extensive property and a state function. The change in Gibbs energy for the system, ΔGsys\Delta G_{\text{sys}}, can be written as:

ΔGsys=ΔHsys−TΔSsys−SsysΔT\Delta G_{\text{sys}} = \Delta H_{\text{sys}} - T\Delta S_{\text{sys}} - S_{\text{sys}}\Delta T

At constant temperature, ΔT=0\Delta T = 0, so:

ΔGsys=ΔHsys−TΔSsys\Delta G_{\text{sys}} = \Delta H_{\text{sys}} - T\Delta S_{\text{sys}}

Usually, we drop the subscript "system" and write simply:

ΔG=ΔH−TΔS(5.21)\Delta G = \Delta H - T\Delta S \qquad(5.21)

This is the Gibbs equation, one of the most important equations in chemistry. It combines both energy (through ΔH\Delta H) and entropy (through ΔS\Delta S) into a single criterion for spontaneity.

Dimensionally, ΔG\Delta G has units of energy because both ΔH\Delta H and TΔST\Delta S are energy terms: TΔS=(K)(J/K)=JT\Delta S = (\text{K})(\text{J/K}) = \text{J}.

Relating ΔG\Delta G to Spontaneity

We know that ΔStotal=ΔSsys+ΔSsurr\Delta S_{\text{total}} = \Delta S_{\text{sys}} + \Delta S_{\text{surr}}.

If the system is in thermal equilibrium with the surroundings, the temperature of the surroundings is the same as that of the system. Also, the increase in enthalpy of the surroundings equals the decrease in enthalpy of the system. Therefore:

ΔSsurr=ΔHsurrT=−ΔHsysT\Delta S_{\text{surr}} = \frac{\Delta H_{\text{surr}}}{T} = -\frac{\Delta H_{\text{sys}}}{T}

So:

ΔStotal=ΔSsys−ΔHsysT\Delta S_{\text{total}} = \Delta S_{\text{sys}} - \frac{\Delta H_{\text{sys}}}{T}

Rearranging:

TΔStotal=TΔSsys−ΔHsysT\Delta S_{\text{total}} = T\Delta S_{\text{sys}} - \Delta H_{\text{sys}}

For a spontaneous process, ΔStotal>0\Delta S_{\text{total}} > 0, so:

TΔSsys−ΔHsys>0T\Delta S_{\text{sys}} - \Delta H_{\text{sys}} > 0

Or:

−(ΔHsys−TΔSsys)>0-(\Delta H_{\text{sys}} - T\Delta S_{\text{sys}}) > 0

Using equation (5.21), this becomes:

Important

−ΔG>0orΔG<0(5.22)-\Delta G > 0 \quad \text{or} \quad \Delta G < 0 \qquad(5.22)

Thus, the criterion for spontaneity at constant pressure and temperature is:

  • If ΔG<0\Delta G < 0 (negative), the process is spontaneous.
  • If ΔG>0\Delta G > 0 (positive), the process is non-spontaneous.
  • If ΔG=0\Delta G = 0, the system is at equilibrium.

ΔHsys\Delta H_{\text{sys}} is the enthalpy change of the reaction, and TΔSsysT\Delta S_{\text{sys}} is the energy that is not available to do useful work. So ΔG\Delta G represents the net energy available to do useful work — it is a measure of the "free energy."

Note

If a reaction has a positive enthalpy change and a positive entropy change, it can be spontaneous when TΔST\Delta S is large enough to outweigh ΔH\Delta H. This can happen in two ways:

  • The positive entropy change of the system is "small," in which case TT must be large.
  • The positive entropy change of the system is "large," in which case TT may be small. The former is one reason why reactions are often carried out at high temperature. …