Enthalpy and Entropy of Activation

Thermodynamic formulation of transition-state theory and Gibbs energy of activation

Lesson 3119 of 4,500 · Kinetics and Reaction Dynamics

Learning objectives

Introduction

An energy diagram often labels a single barrier height, but a reaction rate responds to a free-energy bottleneck. Reaching the transition state can require both an enthalpy cost and a change in how many configurations are accessible. Transition-state theory packages these effects into ΔG‡° = ΔH‡° − TΔS‡°. The distinction explains why two reactions with similar energetic barriers can run at very different rates and why temperature trends can reveal more than one mechanistic feature.

Core explanation

For a specified standard state, the formal activation equilibrium factor is K‡ = exp(−ΔG‡°/RT). Substituting this into the Eyring equation for an elementary unimolecular step gives k = κ(k B T/h)exp(−ΔG‡°/RT). Use the thermodynamic identity ΔG‡° = ΔH‡° − TΔS‡° to obtain k = κ(k B T/h)exp(ΔS‡°/R)exp(−ΔH‡°/RT). This form separates an entropic multiplier from an enthalpic exponential. The constants are Boltzmann's k B, Planck's h and the molar gas constant R. Temperature must be in kelvin, ΔH‡° in energy per mole and ΔS‡° in energy per mole per kelvin.

Activation enthalpy is related to energetic interactions as reactants move toward the barrier region. A positive ΔH‡° often reflects bonds stretching or unfavorable contacts, although the detailed molecular interpretation can include solvent and pressure effects. Activation entropy compares the number and distribution of accessible states in the barrier ensemble with those in the reactant ensemble. A negative ΔS‡° often accompanies a more organised arrangement or loss of independent translational and rotational freedom, as may occur when two separate molecules form a tightly oriented encounter configuration. A positive ΔS‡° can occur when the transition-state ensemble has more accessible configurations, but it does not automatically prove that a bond has broken. These signs are clues, not mechanism identifiers by themselves.

For a bimolecular reaction, the activation parameters depend on the chosen standard concentration or pressure. Association of A and B generally loses translational freedom, so a negative activation entropy is plausible. But a solvent can release ordered molecules around the reactants, and that solvent contribution may partly compensate or reverse the simple molecular-count expectation. A standard-state conversion can also shift a reported ΔS‡° while leaving the physical rate prediction unchanged when all factors are treated consistently. Therefore compare activation entropies only when their conditions and conventions are stated.

At fixed temperature, every increase in ΔG‡° of RT lowers K‡ by a factor e and thus lowers the ideal rate by the same factor. At 298 K, RT ≈ 2.48 kJ mol⁻¹. A barrier difference of roughly 5.7 kJ mol⁻¹ changes a rate by about a factor of ten because RT ln10 ≈ 5.71 kJ mol⁻¹. This is why seemingly small errors in calculated free energies can create large disagreements in predicted rate constants. The calculation also illustrates why a lower ΔH‡° is not always a faster route: a sufficiently more negative ΔS‡° can make its ΔG‡° higher.

Temperature changes both the explicit k B T/h factor and the barrier population. If ΔH‡° and ΔS‡° are approximately constant over a limited range, the equation predicts a characteristic curved rate-versus-temperature relationship when plotted naively, but a near-straight line when ln(k/T) is plotted against 1/T. The next page derives that Eyring plot. Over wide ranges, heat-capacity changes or a shifting mechanism may make the activation parameters temperature-dependent, so a fitted straight line is an approximation rather than a universal law.

The thermodynamic formulation does not replace the dynamical assumptions of page 3116. A calculated ΔG‡° can be accurate while a simple rate still overpredicts experiment if trajectories recross the dividing surface. Conversely, tunnelling can increase a measured rate relative to the classical over-barrier prediction. In complex systems, multiple conformers or parallel paths may contribute, and an experimentally inferred activation quantity can reflect a weighted effective barrier rather than one single geometry. The IUPAC terminology report on reaction-rate quantities distinguishes activation quantities and their conventions; the IUPAC discussion of reaction-rate theory describes the underlying assumptions.

Step-by-step reasoning

1. Decide whether the quoted activation parameters refer to the same reaction step, temperature and standard state. 2. Convert ΔH‡° and ΔS‡° into consistent units, such as J mol⁻¹ and J mol⁻¹ K⁻¹. 3. Calculate ΔG‡° = ΔH‡° − TΔS‡° at the requested temperature. 4. Find K‡ = exp(−ΔG‡°/RT), checking that the exponent is dimensionless. 5. Multiply by k B T/h and any stated transmission factor; add the standard-concentration conversion if the rate constant is bimolecular. 6. Interpret the result as a model prediction and check whether the assumed elementary mechanism and temperature range are appropriate.

Visual explanation

Draw two pathways from the same reactant valley to different transition-state regions. Path X reaches a low but very narrow mountain pass with few allowed orientations; path Y reaches a slightly higher but broad pass with many orientations. Label their enthalpic barrier heights on the vertical energy axis and indicate the narrow versus broad collection of configurations as an entropy difference. Beside them, write ΔG‡° = ΔH‡° − TΔS‡°. The diagram reminds readers that a single vertical energy height does not determine the full statistical bottleneck.

Real-world analogy

Suppose two exits from a crowded building lead outside. One is close but forces everyone through a strict security checkpoint; the other is farther away but has several wide lanes. Distance resembles an energy cost, while the number of allowed arrangements resembles an entropy contribution. The analogy is imperfect because enthalpy is not physical walking distance and molecular entropy is quantified from ensembles of states, not simply the number of doors.

Real-world example

In catalysis, one pathway may lower the energy needed to distort a substrate but require a highly ordered binding pose. Another pathway may have a somewhat higher enthalpic cost yet allow many orientations. Temperature-dependent rate measurements can help distinguish their effective activation parameters. Researchers still need structural, spectroscopic or product-distribution evidence before assigning a detailed transition-state geometry, because multiple mechanisms can yield similar ΔH‡° and ΔS‡° values.

Why?

Why does a negative activation entropy slow the classical Eyring prediction? Since exp(ΔS‡°/R) multiplies the rate, a negative ΔS‡° makes that factor less than one. Physically, the transition-state ensemble has fewer accessible configurations than the reference reactant ensemble under the chosen standard state, so fewer thermal reactants occupy the required bottleneck. The enthalpy term separately penalises energetically costly configurations.

Common misconception

“Activation entropy is the entropy change of the overall reaction.” It is not; it compares the transition-state ensemble with the reactant ensemble for the specified elementary step. Another mistake is claiming a negative ΔS‡° proves an associative mechanism. Solvation, conformational restriction and standard-state choice can also affect the sign. Finally, ΔG‡° must be evaluated at the actual temperature; simply comparing ΔH‡° values may rank pathways incorrectly.

Worked example

An elementary unimolecular reaction at 298 K has ΔH‡° = 50.0 kJ mol⁻¹ and ΔS‡° = −50.0 J mol⁻¹ K⁻¹. Convert enthalpy to 50,000 J mol⁻¹. Then ΔG‡° = 50,000 − 298(−50.0) = 64,900 J mol⁻¹. With R = 8.314 J mol⁻¹ K⁻¹, K‡ = exp[−64,900/(8.314 × 298)] ≈ 4.21 × 10⁻¹². Since k B T/h ≈ 6.21 × 10¹² s⁻¹ at 298 K, the ideal κ = 1 rate is k ≈ 26.1 s⁻¹. If the entropy term were mistakenly omitted, the predicted rate would be much faster; its negative value adds 14.9 kJ mol⁻¹ to the free-energy barrier at this temperature.

Quick check

1. If ΔS‡° is negative, is −TΔS‡° positive or negative at positive absolute temperature? Answer: Positive, so it raises ΔG‡° relative to ΔH‡° and lowers the ideal rate.

Exam focus

Write the complete relation k = κ(k B T/h)exp(ΔS‡°/R)exp(−ΔH‡°/RT) for a unimolecular elementary step. Keep J and kJ conversions explicit. Explain why activation and overall reaction entropies differ, and why a barrier's free energy rather than only potential energy determines its thermal population. For a bimolecular step, add the appropriate standard-concentration factor and state the convention.

Advanced insight

Activation heat capacity is ΔC p‡ = dΔH‡/dT and also equals T dΔS‡/dT at constant pressure. If ΔC p‡ is appreciable, neither activation enthalpy nor entropy remains constant over a broad temperature interval. Curvature in a temperature plot may therefore reflect heat-capacity effects, competing pathways, conformational changes or quantum tunnelling. Distinguishing them requires more than fitting a single straight line. In solution chemistry, solvent reorganisation can dominate ΔS‡° even when the reacting solute geometry looks more ordered.

Summary

The activation Gibbs energy is ΔG‡° = ΔH‡° − TΔS‡° and controls the formal transition-state population through K‡ = exp(−ΔG‡°/RT). Activation enthalpy describes an energetic contribution; activation entropy captures the relative abundance of accessible configurations under a specified standard state. Both influence rate, and their signs are interpretive clues rather than unique mechanistic proofs. The Eyring equation combines this free-energy factor with k B T/h and an appropriate transmission correction.

Practice questions

1. Find ΔG‡° at 300 K if ΔH‡° = 40 kJ mol⁻¹ and ΔS‡° = −20 J mol⁻¹ K⁻¹. Answer: Convert ΔS‡° to −0.020 kJ mol⁻¹ K⁻¹; ΔG‡° = 40 − 300(−0.020) = 46 kJ mol⁻¹.

2. Two paths have equal ΔH‡°, but path A has a more negative ΔS‡° than path B. Which has the smaller ideal Eyring rate at the same temperature? Answer: Path A, because its ΔG‡° is larger and its activation equilibrium factor is smaller.

3. Does a positive activation entropy necessarily prove that an elementary step is dissociative? Answer: No. Solvation, conformer populations and standard-state effects can influence its sign; other mechanistic evidence is needed.

4. In the worked example, what would a classical recrossing factor κ = 0.50 do to k? Answer: It would halve the ideal result from about 26.1 s⁻¹ to about 13.1 s⁻¹ without changing the stated activation thermodynamic parameters.

5. At 298 K, about how much does ΔG‡° need to rise to reduce a rate tenfold under otherwise equal conditions? Answer: RT ln10 ≈ 5.7 kJ mol⁻¹.