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Van 't Hoff equation

Relation between temperature and the equilibrium constant of a chemical reaction

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Through Equilibrium constant, Temperature and Standard enthalpy of reaction

The Van 't Hoff equation has been widely utilized to explore the changes in state functions in a thermodynamic system. The Van 't Hoff plot, which is derived from this equation, is especially effective in estimating the change in enthalpy and entropy of a chemical reaction.

Equation

Summary and uses

The standard pressure, P0, is used to define the reference state for the Van 't Hoff equation, which is

ddTln⁡Keq=ΔrH⊖RT2

where ln denotes the natural logarithm, Keq is the thermodynamic equilibrium constant, and R is the ideal gas constant. This equation is exact at any one temperature and all pressures, derived from the requirement that the Gibbs free energy of reaction be stationary in a state of chemical equilibrium.

In practice, the equation is often integrated between two temperatures under the assumption that the standard reaction enthalpy ΔrH⊖ is constant (and furthermore, this is also often assumed to be equal to its value at standard temperature). Since in reality ΔrH⊖ and the standard reaction entropy ΔrS⊖ do vary with temperature for most processes, the integrated equation is only approximate. Approximations are also made in practice to the activity coefficients within the equilibrium constant.

A major use of the integrated equation is to estimate a new equilibrium constant at a new absolute temperature assuming a constant standard enthalpy change over the temperature range. To obtain the integrated equation, it is convenient to first rewrite the Van 't Hoff equation as

dln⁡Keqd1T=−ΔrH⊖R.

The definite integral between temperatures T1 and T2 is then

ln⁡K2K1=ΔrH⊖R(1T1−1T2).

In this equation K1 is the equilibrium constant at absolute temperature T1, and K2 is the equilibrium constant at absolute temperature T2.

Development from thermodynamics

Combining the well-known formula for the Gibbs free energy of reaction

ΔrG⊖=ΔrH⊖−TΔrS⊖,

where S is the entropy of the system, with the Gibbs free energy isotherm equation:

ΔrG⊖=−RTln⁡Keq,

we obtain

ln⁡Keq=−ΔrH⊖RT+ΔrS⊖R.

Differentiation of this expression with respect to the variable T while assuming that both ΔrH⊖and ΔrS⊖ are independent of T yields the Van 't Hoff equation. These assumptions are expected to break down somewhat for large temperature variations.

Provided that ΔrH⊖ and ΔrS⊖ are constant, the preceding equation gives ln K as a linear function of ⁠1/T⁠ and hence is known as the linear form of the Van 't Hoff equation. Therefore, when the range in temperature is small enough that the standard reaction enthalpy and reaction entropy are essentially constant, a plot of the natural logarithm of the equilibrium constant versus the reciprocal temperature gives a straight line. The slope of the line may be multiplied by the gas constant R to obtain the standard enthalpy change of the reaction, and the intercept may be multiplied by R to obtain the standard entropy change.

Van 't Hoff isotherm

The Van 't Hoff isotherm can be used to determine the temperature dependence of the Gibbs free energy of reaction for non-standard state reactions at a constant temperature:

(dGdξ)T,p=ΔrG=ΔrG⊖+RTln⁡Qr,

where ΔrG is the Gibbs free energy of reaction under non-standard states at temperature T, ΔrG⊖ is the Gibbs free energy for the reaction at (T,P0), ξ is the extent of reaction, and Qr is the thermodynamic reaction quotient. Since ΔrG⊖=−RTln⁡Keq, the temperature dependence of both terms can be described by Van t'Hoff equations as a function of T. This finds applications in the field of electrochemistry. particularly in the study of the temperature dependence of voltaic cells.

The isotherm can also be used at fixed temperature to describe the Law of Mass Action. When a reaction is at equilibrium, Qr = Keq and ΔrG=0. Otherwise, the Van 't Hoff isotherm predicts the direction that the system must shift in order to achieve equilibrium; when ΔrG < 0, the reaction moves in the forward direction, whereas when ΔrG > 0, the reaction moves in the backwards direction. See Chemical equilibrium.

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