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Temperature Dependence of Equilibrium Constants: The van ’t Hoff Equation and Applications to Functional Oxides

Thermodynamics
Functional Oxides
Defect Chemistry
Materials Science
Understand how equilibrium constants change with temperature, derive and apply the van ’t Hoff equation, account for heat-capacity effects, and interpret oxidation, reduction, and hydration equilibria in functional oxides.
Author

Mostafa Elkady

Published

November 5, 2026

THERMODYNAMICS OF FUNCTIONAL MATERIALS · FUNDAMENTALS 06

Temperature Dependence of Equilibrium Constants: The van ’t Hoff Equation and Applications to Functional Oxides

An equilibrium constant is not generally a fixed number for a chemical reaction. It is defined at a specified temperature, and its temperature dependence determines how the equilibrium composition shifts when a material is heated or cooled.

For functional oxides, this dependence matters in oxygen nonstoichiometry, oxidation and reduction, hydration of proton-conducting ceramics, phase stability, and processing under controlled atmospheres. The van ’t Hoff equation provides a quantitative connection between the equilibrium constant and the standard reaction enthalpy.

This article develops that connection, explains the assumptions behind the familiar linear van ’t Hoff plot, and shows how to use the equation without confusing equilibrium thermodynamics with reaction kinetics.

1. Why does the equilibrium constant depend on temperature?

For a reaction at equilibrium,

[ _rG^=-RTK ]

The standard reaction Gibbs energy is related to standard reaction enthalpy and entropy by

[ _rG=_rH-T_rS^ ]

Combining the two expressions gives

[ -RTK=_rH-T_rS ]

or

[ K=- + ]

Both reaction enthalpy and reaction entropy can depend on temperature. Over a sufficiently narrow temperature interval, it is often reasonable to approximate the reaction enthalpy as constant. Under that approximation, the temperature dependence of (K) is described by the van ’t Hoff equation.

A key point is that (K) describes the equilibrium state for a specified reaction and standard-state convention. It does not specify how quickly that state is reached.

2. Derivation of the differential van ’t Hoff equation

Start from

[ K=- ]

Using the Gibbs–Helmholtz relation at constant pressure,

[ _p =- ]

and differentiating the equilibrium relation gives

[ ]

This is the differential van ’t Hoff equation.

It relates the slope of (K) against temperature to the standard reaction enthalpy. The enthalpy is positive for an endothermic forward reaction and negative for an exothermic forward reaction.

The equation is written for a dimensionless thermodynamic equilibrium constant. The logarithm must not be taken of a dimensional quantity.

3. Integrated van ’t Hoff equation

If (_rH^) is approximately constant between two temperatures, integrate:

[ {K_1}^{K_2}dK = {T_1}{T_2}\frac{dT}{T2} ]

Since

[ =- ]

the result is

[ ]

Equivalently,

[ ]

All temperatures must be absolute temperatures in kelvin. The reaction enthalpy and gas constant must use compatible energy units.

This integrated expression is especially useful when an equilibrium constant is known at one reference temperature and is required at another.

4. Interpreting the sign: endothermic and exothermic reactions

The differential equation is

[ = ]

Because (R) and (T^2) are positive, the sign of the slope is determined by (_rH^).

Endothermic forward reaction

If

[ _rH^>0 ]

then

[ >0 ]

The equilibrium constant increases as temperature increases. Under the same standard-state convention, higher temperature favours products relative to reactants for this reaction.

Exothermic forward reaction

If

[ _rH^<0 ]

then

[ <0 ]

The equilibrium constant decreases as temperature increases. Higher temperature favours reactants relative to products for the forward reaction as written.

This interpretation is consistent with the thermodynamic response to heat, but the van ’t Hoff equation provides the quantitative relationship rather than only a qualitative rule.

5. Worked calculation: estimating an equilibrium constant at a new temperature

Suppose an endothermic reaction has:

  • (K_1=2.0^{-4}) at (T_1=700 K);
  • standard reaction enthalpy (_rH=+85.0 \mathrm{kJ,mol{-1}});
  • target temperature (T_2=800 K).

Assume the reaction enthalpy is constant over this interval.

Use

[ () = - (-) ]

Convert the enthalpy to joules per mole:

[ _rH \mathrm{J,mol{-1}} ]

Substitute:

[ () = - (-) ]

The right-hand side is approximately

[ 1.82 ]

Therefore,

[ K_2=2.0^{-4}(1.82) ]

and

[ ]

The equilibrium constant increases by approximately a factor of 6.2 between 700 and 800 K. This is the expected direction for an endothermic forward reaction.

The calculation predicts a change in equilibrium constant. It does not by itself give the final concentrations or phase fractions: those require the reaction quotient, mass balance, and any relevant charge- or site-balance constraints.

6. The van ’t Hoff plot

The integrated equation can be rearranged as

[ K = - +C ]

where (C) is constant if the reaction enthalpy and entropy are effectively constant over the selected temperature interval.

A plot of (K) against (1/T) is then approximately linear:

[ y=mx+b ]

with

[ m=- ]

and

[ b ]

Thus, the reaction enthalpy can be estimated from the slope:

[ ]

The entropy estimate from the intercept is meaningful only when the standard-state convention and the constant-enthalpy approximation are appropriate.

Practical interpretation

  • A negative slope corresponds to an endothermic forward reaction.
  • A positive slope corresponds to an exothermic forward reaction.
  • Curvature can indicate temperature-dependent reaction enthalpy, changing reaction mechanisms, non-ideal activities, or a change in the dominant phase or defect regime.

A straight line should not be forced through data spanning different thermodynamic regimes without checking the underlying assumptions.

7. Estimating reaction enthalpy from equilibrium measurements

If equilibrium constants are measured at several temperatures, a linear fit can be used over a temperature interval where the constant-(_rH^) approximation is justified.

A practical procedure is:

  1. Establish the reaction and write its activity-based equilibrium expression.
  2. Measure or infer equilibrium compositions at several controlled temperatures.
  3. Convert the measured compositions into dimensionless activities using a consistent activity model.
  4. Calculate (K) at each temperature.
  5. Plot (K) against (1/T).
  6. Fit the linear region and obtain its slope.
  7. Calculate (_rH^=-mR).
  8. Inspect residuals and compare the fitted enthalpy with independent thermochemical data where available.

The largest experimental challenge is often not the regression. It is demonstrating that the sample reached equilibrium and that the calculated activities represent the actual material state.

For oxide ceramics, equilibration can be limited by gas exchange, bulk diffusion, surface exchange, slow hydration or dehydration, and phase transformations. A measurement taken before equilibrium is reached may produce an apparent temperature dependence that is not the equilibrium van ’t Hoff relation.

8. When reaction enthalpy changes with temperature

The constant-enthalpy approximation can fail over broad temperature intervals. The temperature dependence of reaction enthalpy is determined by the standard reaction heat-capacity change:

[ _rC_p^ = _iiC{p,i}^ ]

At constant pressure,

[ =_rC_p^ ]

If (_rC_p^) is approximately constant over the interval,

[ _rH^(T) = _rH^(T_0) +_rC_p^(T-T_0) ]

Substituting this temperature-dependent enthalpy into the differential van ’t Hoff equation and integrating from (T_0) to (T) gives

[ () = (-) + ]

This expression assumes constant (_rC_p^). If heat capacities vary significantly with temperature, they should be integrated using suitable heat-capacity functions or thermochemical databases.

A curved van ’t Hoff plot may therefore be physically meaningful. It can reflect heat-capacity effects even when the same reaction remains dominant.

9. Application to oxygen loss in functional oxides

Consider the reduction reaction written in Kröger–Vink notation:

[ ]

Its standard reaction enthalpy determines the temperature dependence of the corresponding equilibrium constant:

[ = ]

If the forward oxygen-loss reaction is endothermic over the temperature interval, its equilibrium constant increases with temperature. At a fixed oxygen activity, the equilibrium defect concentrations must then adjust to satisfy the mass-action expression together with charge neutrality and site balance.

This does not mean that oxygen-vacancy concentration is always a simple function of (K_{}) alone. The observed concentration also depends on oxygen partial pressure, electronic compensation, dopant concentration, defect association, and the validity of the dilute-defect approximation.

A useful experimental distinction is between: - the equilibrium temperature dependence at fixed oxygen chemical potential; - the response to changing oxygen partial pressure at fixed temperature; - the transient response while the sample approaches equilibrium.

These are different measurements and should not be conflated.

10. Application to hydration in proton-conducting oxides

A common hydration reaction is

[ ]

For this reaction,

[ = ]

Hydration of many acceptor-doped perovskite oxides is exothermic over relevant temperature ranges. If (rH{}^<0), the hydration equilibrium constant decreases as temperature rises. At fixed water activity, the equilibrium generally shifts toward the dehydrated side at higher temperature.

At lower temperature, hydration can become more favourable thermodynamically, but the measured proton uptake may still be limited by slow water incorporation or bulk diffusion. Conversely, at high temperature the material may equilibrate rapidly while the equilibrium proton concentration is lower.

This distinction is important when interpreting thermogravimetric measurements, conductivity-humidity experiments, and proton uptake measurements. A conductivity maximum or minimum cannot be interpreted from equilibrium thermodynamics alone because proton mobility and microstructural contributions also vary with temperature.

11. Equilibrium constant, reaction quotient, and operating conditions

The equilibrium constant is a function of temperature for a specified reaction and standard-state convention:

[ K=K(T) ]

The reaction quotient depends on the current composition:

[ Q=Q({a_i}) ]

The reaction Gibbs energy combines both:

[ _rG=RT() ]

This form is especially useful when temperature and composition both change.

  • If (Q<K), the forward reaction has a negative reaction Gibbs energy.
  • If (Q>K), the reverse reaction has a negative reaction Gibbs energy.
  • If (Q=K), the system is at equilibrium for that reaction.

When temperature changes, (K) changes. If the composition has not yet responded, (Q) initially retains its previous value and the system is no longer at equilibrium. The subsequent reaction and transport processes move the composition toward the new equilibrium state.

For a gas-solid system, changing temperature can also change gas activities through pressure and volume changes. Those effects must be accounted for separately rather than attributed entirely to the temperature dependence of (K).

12. Common experimental and calculation errors

  • Using Celsius in the van ’t Hoff equation. All temperatures must be in kelvin.
  • Mixing joules and kilojoules. Use compatible units for (_rH^) and (R).
  • Taking the logarithm of a dimensional equilibrium constant. Use dimensionless activities and a dimensionless (K).
  • Reversing the sign. The slope of (K) against (1/T) is (-_rH^/R).
  • Assuming constant enthalpy over any temperature range. Check heat-capacity effects and possible phase or defect-regime changes.
  • Treating non-equilibrium measurements as equilibrium data. Verify reversibility, time independence, and sufficient equilibration.
  • Ignoring the activity model. Concentration-based expressions may be inadequate for non-ideal solid solutions or concentrated defect populations.
  • Interpreting equilibrium as a transport property. The van ’t Hoff equation does not provide ionic mobility, diffusion coefficients, or conductivity.

13. Practical checklist

Before using a van ’t Hoff analysis for a functional material, confirm:

  • The reaction is balanced and its direction is explicitly defined.
  • The equilibrium constant is dimensionless.
  • Standard states and activity conventions are consistent across temperatures.
  • The measured compositions correspond to equilibrium.
  • The same reaction and phase assemblage remain relevant across the fitted range.
  • The assumed reaction enthalpy is sufficiently constant, or heat-capacity corrections are included.
  • Temperature is measured at the sample and reported in kelvin.
  • The fitted slope, uncertainty, and residuals are reported.
  • Any defect-chemistry interpretation also satisfies charge neutrality and site balance.

14. Summary

The van ’t Hoff equation links the temperature dependence of an equilibrium constant to the standard reaction enthalpy:

[ ]

For approximately constant reaction enthalpy,

[ ]

An endothermic forward reaction has an equilibrium constant that increases with temperature, while an exothermic forward reaction has an equilibrium constant that decreases with temperature.

For functional oxides, this framework helps interpret oxygen loss, oxidation and reduction, and hydration of proton-conducting ceramics. Quantitative analysis still requires a suitable activity model, verified equilibrium, and the additional constraints imposed by mass balance, charge neutrality, and site occupancy.

Further reading

  • D. R. Gaskell and D. E. Laughlin, Introduction to the Thermodynamics of Materials, 6th ed., CRC Press.
  • H. B. Callen, Thermodynamics and an Introduction to Thermostatistics, 2nd ed., Wiley.
  • P. Atkins, J. de Paula, and J. Keeler, Atkins’ Physical Chemistry, Oxford University Press.
  • A. R. West, Solid State Chemistry and its Applications, 2nd ed., Wiley.