Transition State Theory
The activated complex, the Eyring equation, potential energy surfaces, and kinetic isotope effects
1. Introduction: The Activated Complex
Transition State Theory (TST), also known as Activated Complex Theory, provides a powerful framework for understanding and predicting the rates of chemical reactions. Unlike the purely empirical Arrhenius equation, TST connects macroscopic rate constants to the microscopic properties of a special molecular configuration called the transition state or activated complex.
The central idea is deceptively simple: as reactants transform into products, they must pass through a high-energy configuration β the transition state β that sits at the top of the energy barrier separating reactants from products. This configuration is not a stable intermediate; it exists for only a fleeting moment (on the order of a single molecular vibration, $\sim 10^{-13}$ s) before either proceeding to products or reverting to reactants.
Key Assumptions of TST
- β’ Quasi-equilibrium hypothesis: The activated complex is in thermodynamic equilibrium with the reactants, even though the overall reaction may be far from equilibrium.
- β’ Classical motion along the reaction coordinate: The passage over the barrier is treated as a classical translational motion along a single degree of freedom β the reaction coordinate.
- β’ No recrossing: Once the system crosses the transition state dividing surface in the forward direction, it proceeds to products without returning.
- β’ Separability: The reaction coordinate can be separated from all other molecular degrees of freedom at the transition state.
Consider a bimolecular reaction $A + B \to \text{Products}$. In the TST picture, the reaction proceeds through the formation of an activated complex $AB^{\ddagger}$:
The double arrow between reactants and the activated complex indicates the assumed quasi-equilibrium, while the single arrow from the activated complex to products represents the irreversible crossing of the barrier. The rate of reaction is then determined by the concentration of the activated complex and the frequency with which it crosses the barrier.
TST was developed independently in 1935 by Henry Eyring at Princeton and by Michael Polanyi and Meredith Gwynne Evans at Manchester. It represents one of the most successful and widely used theories in physical chemistry, providing a bridge between statistical thermodynamics and chemical kinetics that remains essential in modern computational chemistry, enzyme catalysis, and materials science.
2. Derivation: The Eyring Equation
We derive the Eyring equation from the quasi-equilibrium assumption and statistical mechanics. Consider the bimolecular reaction:
Step 1: Quasi-Equilibrium
By the quasi-equilibrium hypothesis, the activated complex $AB^{\ddagger}$ is in thermodynamic equilibrium with the reactants. We can therefore define an equilibrium constant$K^{\ddagger}$ for this pseudo-equilibrium:
This gives us the concentration of the activated complex:
Step 2: Rate of Barrier Crossing
The rate of reaction equals the concentration of the activated complex multiplied by the frequency $\nu^{\ddagger}$ at which it crosses the barrier:
To find $\nu^{\ddagger}$, we treat the motion along the reaction coordinate as a one-dimensional classical translation. The partition function for this single translational degree of freedom over a small distance $\delta$ at the barrier top is:
The average velocity of crossing in the forward direction is:
The frequency of crossing is the velocity divided by the distance:
We can factor $K^{\ddagger}$ into two parts: the partition function for the reaction coordinate $q_{\text{rc}}$ and the remaining equilibrium constant $K^{\ddagger\prime}$that excludes this degree of freedom:
Step 3: Combining the Expressions
Multiplying $\nu^{\ddagger}$ by $K^{\ddagger}$:
The $\delta$ and $\sqrt{2\pi m^{\ddagger}}$ terms cancel beautifully, leaving:
Since the rate constant $k$ is defined by $\text{Rate} = k[A][B]$, we obtain:
where we now write $K^{\ddagger}$ to mean the equilibrium constant with the reaction coordinate factored out (dropping the prime for notational convenience).
Step 4: Thermodynamic Form
From thermodynamics, the equilibrium constant is related to the standard Gibbs energy of activation:
Substituting into the Eyring equation:
Since $\Delta G^{\ddagger} = \Delta H^{\ddagger} - T\Delta S^{\ddagger}$, we can write:
This is the complete Eyring equation. It separates the rate constant into an entropic factor $\exp(\Delta S^{\ddagger}/R)$ and an enthalpic (energetic) factor $\exp(-\Delta H^{\ddagger}/RT)$, providing deep physical insight into what controls reaction rates.
3. Derivation: Thermodynamic Formulation
The Eyring equation provides a molecular interpretation of the empirical Arrhenius parameters. We now derive the precise relationships between the Arrhenius activation energy $E_a$and pre-exponential factor $A$ and the transition state quantities $\Delta H^{\ddagger}$and $\Delta S^{\ddagger}$.
Relating E$_a$ to $\Delta H^{\ddagger}$
The Arrhenius equation defines the activation energy through:
Starting from the Eyring equation, take the natural logarithm:
Differentiating with respect to temperature (treating $\Delta H^{\ddagger}$ and $\Delta S^{\ddagger}$ as approximately temperature-independent):
Multiplying both sides by $RT^2$:
This result applies to gas-phase bimolecular reactions. More generally, for a reaction involving $n$ molecules going to the transition state in a gas-phase reaction where $\Delta n^{\ddagger} = 1 - n$ (change in moles from reactants to transition state):
where $n = 1$ for gas-phase bimolecular reactions (accounting for the $\ln T$ term) and $n = 0$ for reactions in solution (where the transmission coefficient absorbs the$PV$ work terms, and concentrations rather than pressures define $K^{\ddagger}$). At 298 K, $RT \approx 2.5$ kJ/mol, which is small relative to typical activation enthalpies of 40β200 kJ/mol.
Relating A to $\Delta S^{\ddagger}$
The Arrhenius pre-exponential factor is obtained by comparing $k = A\exp(-E_a/RT)$with the Eyring equation. Substituting $E_a = \Delta H^{\ddagger} + RT$ for a bimolecular gas-phase reaction:
Writing $\Delta H^{\ddagger} = E_a - RT$ and substituting:
Comparing with $k = A\exp(-E_a/RT)$, we identify:
where $e = 2.71828...$ is Euler's number. This reveals the physical meaning of the pre-exponential factor: it encodes the entropy of activation. A large positive $\Delta S^{\ddagger}$ (loose transition state) gives a large $A$, while a highly negative $\Delta S^{\ddagger}$ (tight, ordered transition state) gives a small $A$.
Physical Interpretation
- β’ $\Delta S^{\ddagger} < 0$: The transition state is more ordered than the reactants. Common in association reactions (e.g., DielsβAlder, S$_N$2) where two molecules must adopt a specific orientation.
- β’ $\Delta S^{\ddagger} > 0$: The transition state is less ordered. Common in dissociation reactions and unimolecular decompositions where bonds loosen at the transition state.
- β’ $\Delta S^{\ddagger} \approx 0$: The transition state has similar order to the reactants. Typical for isomerization reactions and intramolecular rearrangements.
4. Derivation: Potential Energy Surfaces
The potential energy surface (PES) provides the conceptual and computational foundation for transition state theory. For a chemical reaction, the PES is a multidimensional function that gives the electronic energy as a function of all nuclear coordinates. We illustrate the key concepts using the simplest nontrivial case: a collinear atom-transfer reaction.
The Collinear A + BC Reaction
Consider the reaction $A + BC \to AB + C$ constrained to collinear geometry. The system has two independent internal coordinates: the bond distances $r_{AB}$and $r_{BC}$. The potential energy $V(r_{AB}, r_{BC})$ defines a two-dimensional surface with the following key features:
- β’ Reactant valley: Located at large $r_{AB}$ and small $r_{BC}$ (A is far from BC, which is at its equilibrium distance).
- β’ Product valley: Located at small $r_{AB}$ and large $r_{BC}$ (AB is formed, C moves away).
- β’ Saddle point: The point of highest energy along the minimum energy path connecting the two valleys. This is the transition state.
The Minimum Energy Path and Reaction Coordinate
The minimum energy path (MEP), also called the intrinsic reaction coordinate (IRC), is the path of steepest descent from the saddle point to both the reactant and product valleys. It represents the most favorable pathway for the reaction. The arc length along this path defines the reaction coordinate $s$.
At the saddle point, the Hessian matrix of second derivatives of the potential energy has a special structure. In mass-weighted coordinates:
The eigenvalues of the Hessian at the saddle point are:
- β’ One negative eigenvalue $\lambda_1 < 0$: This corresponds to the reaction coordinate direction. The curvature is negative because the saddle point is a maximum along this direction. The associated imaginary frequency is $\nu^{\ddagger} = \frac{1}{2\pi}\sqrt{|\lambda_1|/\mu}$.
- β’ All other eigenvalues positive $\lambda_i > 0$: These correspond to the vibrational modes of the activated complex perpendicular to the reaction coordinate. The frequencies are $\nu_i = \frac{1}{2\pi}\sqrt{\lambda_i/\mu_i}$.
Curvature and Vibrational Frequencies
The vibrational frequencies of the transition state are directly related to the curvature of the PES. For a nonlinear transition state with $N$ atoms, there are$3N - 7$ real vibrational frequencies (one fewer than the usual $3N - 6$because the reaction coordinate replaces one vibration). These frequencies enter the partition function of the activated complex:
The imaginary frequency along the reaction coordinate determines the width of the barrier and is crucial for estimating quantum mechanical tunneling corrections:
where $s$ is the displacement along the reaction coordinate from the saddle point. A larger $|\lambda_1|$ means a sharper, narrower barrier, which enhances tunneling.
The LEPS Potential
A commonly used analytic form for the PES of atom-transfer reactions is the LondonβEyringβPolanyiβSato (LEPS) potential. For the collinear $A + BC \to AB + C$ reaction, the LEPS potential is:
where $Q_{ij}$ and $J_{ij}$ are the Coulomb and exchange integrals for each diatomic pair, expressed in terms of Morse potential parameters and Sato parameters that control the barrier height. The Coulomb integral for pair $ij$ is:
and the exchange integral is:
where $E_{\text{singlet}} = D_{ij}(e^{-2\beta_{ij}(r-r_e)} - 2e^{-\beta_{ij}(r-r_e)})$is the Morse potential and $E_{\text{triplet}} = \tfrac{1}{2}D_{ij}(e^{-2\beta_{ij}(r-r_e)} + 2e^{-\beta_{ij}(r-r_e)})$is the anti-Morse (triplet repulsion) curve.
5. Derivation: Kinetic Isotope Effects
One of the most powerful experimental tests of transition state theory is the kinetic isotope effect (KIE). When an atom in the reacting bond is replaced by a heavier isotope (most commonly H replaced by D), the rate constant changes. TST provides a quantitative framework for predicting these changes.
Primary KIE from Zero-Point Energy Differences
The primary kinetic isotope effect arises primarily from differences in zero-point energies (ZPE) between the light and heavy isotopologues. The zero-point energy of a vibrational mode with frequency $\nu$ is:
where $k_f$ is the force constant and $\mu$ is the reduced mass. Since $\mu_D > \mu_H$ for CβD vs CβH, the CβD bond has a lower vibrational frequency and therefore a lower zero-point energy.
In the transition state, the bond being broken has a significantly reduced force constant (the bond is partially broken), so the ZPE difference between H and D isotopologues is smaller at the TS than in the reactant. The activation energy difference is:
where $\Delta E_{\text{ZPE}} = E_{\text{ZPE}}^H - E_{\text{ZPE}}^D$. Since the ZPE difference in the reactant is larger than at the transition state (where the bond is nearly broken), $\Delta E_a > 0$ and $k_H > k_D$.
The KIE from TST is therefore:
where $\Delta E_{\text{ZPE},H}$ and $\Delta E_{\text{ZPE},D}$ represent the ZPE changes (TS minus reactant) for the H and D isotopologues respectively.
Estimating the CβH/CβD KIE
For a typical CβH stretching frequency of $\sim 3000$ cm$^{-1}$and a CβD frequency of $\sim 2150$ cm$^{-1}$ (scaled by $\sqrt{\mu_H/\mu_D} \approx 1/\sqrt{2}$), the ZPE difference in the reactant is:
If the bond is completely broken at the transition state (maximum KIE), the ZPE difference at the TS is zero, giving:
In practice, the transition state retains some CβH(D) vibrational character in bending modes, reducing the maximum KIE. Observed primary KIEs for CβH/CβD typically fall in the range 2 to 7 at room temperature. Values significantly above 7 suggest quantum mechanical tunneling.
Wigner Tunneling Correction
Quantum mechanical tunneling allows the system to pass through the barrier rather than over it, enhancing the rate constant. The simplest correction is the Wigner tunneling correction:
where $\nu^{\ddagger}$ is the magnitude of the imaginary frequency at the transition state. Since the lighter isotope (H) has a higher $\nu^{\ddagger}$, it tunnels more effectively, further increasing the KIE:
The Wigner correction is a first-order approximation valid when tunneling is modest. For deep or narrow barriers (particularly at low temperatures), more sophisticated treatments such as the Eckart barrier model or semiclassical instanton methods are required. Observed KIEs exceeding the semiclassical maximum of $\sim 7$ are strong evidence for significant tunneling contributions.
6. Applications of Transition State Theory
Enzyme Catalysis
Enzymes are nature's catalysts, accelerating reactions by factors of $10^{6}$ to$10^{17}$. TST explains this enormous rate enhancement through the concept of transition state stabilization. An enzyme lowers$\Delta G^{\ddagger}$ by binding the transition state more tightly than the ground state substrate. Pauling first proposed this idea in 1946, and it has been confirmed by the success of transition state analog inhibitors β stable molecules that mimic the geometry of the transition state and bind tightly to the enzyme active site. Many clinically important drugs (protease inhibitors for HIV, statins for cholesterol) are designed as transition state analogs.
Atmospheric Reactions
TST is essential for predicting rate constants of atmospheric reactions where direct measurement may be difficult. The reactions governing ozone depletion, smog formation, and climate chemistry involve radical species and unusual transition states. For example, the reaction $\text{OH} + \text{CH}_4 \to \text{H}_2\text{O} + \text{CH}_3$ controls the atmospheric lifetime of methane. Computational TST with tunneling corrections provides rate constants in excellent agreement with experiment over wide temperature ranges.
Drug Design
Modern computational drug design leverages TST through free energy perturbation calculations. By computing$\Delta G^{\ddagger}$ for enzymatic reactions with different substrate modifications, medicinal chemists can predict how structural changes affect reaction rates and binding affinities. The concept of the transition state is central to understanding enzyme mechanism and designing effective inhibitors.
Catalytic Converters
Heterogeneous catalysis in automotive catalytic converters involves reactions on metal surfaces (Pt, Pd, Rh). TST applied to surface reactions explains how the catalyst lowers$\Delta G^{\ddagger}$ for the oxidation of CO and hydrocarbons and the reduction of NO$_x$. The Eyring equation, adapted for surface reactions using two-dimensional gas models for adsorbed species, successfully predicts turnover frequencies and selectivity patterns observed in experiments.
7. Historical Context
The development of transition state theory represents one of the great achievements of twentieth-century theoretical chemistry, weaving together quantum mechanics, statistical mechanics, and thermodynamics into a unified framework for understanding chemical reactivity.
8. Python: LEPS Potential Energy Surface
This simulation constructs a two-dimensional LEPS potential energy surface for a collinear A + BC $\to$ AB + C reaction. The contour plot reveals the reactant and product valleys connected by the minimum energy path (MEP), with the transition state located at the saddle point. The energy profile along the MEP shows the activation barrier.
LEPS Potential Energy Surface and Minimum Energy Path
PythonComputes a 2D PES for collinear atom-transfer, identifies the transition state saddle point, and plots the energy along the reaction coordinate
Click Run to execute the Python code
Code will be executed with Python 3 on the server
9. Fortran: Eyring Rate Constants & Kinetic Isotope Effects
This Fortran program computes Eyring rate constants for CβH and CβD bond breaking across a range of temperatures. It calculates both the semiclassical kinetic isotope effect (from zero-point energy differences alone) and the tunneling-corrected KIE using the Wigner correction. The results demonstrate why primary H/D KIEs typically fall in the range 2β7 at room temperature and increase at lower temperatures.
Eyring Rate Constants and Kinetic Isotope Effects
FortranComputes k_H and k_D via the Eyring equation with ZPE corrections, and applies Wigner tunneling corrections to predict KIE across temperatures
Click Run to execute the Fortran code
Code will be compiled with gfortran and executed on the server