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🧂Physical Chemistry II Unit 1 Review

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1.5 Collision Theory and Transition State Theory

🧂Physical Chemistry II
Unit 1 Review

1.5 Collision Theory and Transition State Theory

Written by the Fiveable Content Team • Last updated September 2025
Written by the Fiveable Content Team • Last updated September 2025
🧂Physical Chemistry II
Unit & Topic Study Guides

Chemical reactions are all about collisions and transitions. Collision Theory explains how molecules must collide with enough energy and proper orientation to react. It's like a game of bumper cars where only the right hits count.

Transition State Theory takes it further, focusing on the fleeting moment when reactants become products. This high-energy state is crucial for understanding reaction rates and mechanisms. It's the chemical equivalent of a tightrope walk between reactants and products.

Collision Theory: Principles and Rate Laws

Basic Principles

  • Collision theory states that for a reaction to occur, the reactant molecules must collide with sufficient energy (to overcome the activation energy barrier) and proper orientation (to allow for effective collision geometry)
  • The rate of a reaction depends on two key factors:
    1. The frequency of collisions between reactant molecules
    2. The fraction of those collisions that have enough energy to overcome the activation energy barrier
  • Increasing the concentration of reactants leads to more frequent collisions (higher collision frequency) and consequently, a higher reaction rate

Factors Affecting Reaction Rates

  • Increasing the temperature of the system raises the average kinetic energy of the molecules
    • This results in a greater proportion of collisions with sufficient energy to react, thus increasing the reaction rate (Arrhenius equation)
  • The presence of a catalyst lowers the activation energy barrier
    • This allows a greater fraction of collisions to result in successful reactions at a given temperature, increasing the reaction rate without being consumed in the process (heterogeneous or homogeneous catalysis)

Transition State: Concept and Significance

Definition and Characteristics

  • The transition state is a high-energy, unstable intermediate formed during a chemical reaction, representing the highest energy point along the reaction coordinate
  • It is the configuration of atoms at the top of the activation energy barrier, where the reactants are partially converted into products (bond breaking and forming occurs simultaneously)
  • The transition state is not a stable species and cannot be isolated or directly observed due to its extremely short lifetime (on the order of 10^-13 seconds)

Importance in Chemical Reactions

  • The structure of the transition state is critical in determining the rate and mechanism of a chemical reaction
    • The geometry and electronic configuration of the transition state influence the reaction pathway and stereochemical outcome (SN1 vs SN2 reactions)
  • The difference in energy between the reactants and the transition state is the activation energy, which determines the rate of the reaction (higher activation energy leads to slower rates)

Transition State Theory: Calculating Rate Constants

Quantitative Approach

  • Transition state theory (TST) provides a more quantitative approach to understanding reaction rates by considering the properties of the transition state
  • According to TST, the rate constant (k) of a reaction is proportional to the concentration of the transition state complex, [TS]^‡, and the frequency of its decomposition into products

Eyring Equation

  • The rate constant can be calculated using the Eyring equation: k=(kBT/h)exp(ΔG/RT)k = (k_B * T / h) * exp(-ΔG^‡ / RT)
    • $k_B$ is the Boltzmann constant
    • $T$ is the absolute temperature
    • $h$ is Planck's constant
    • $ΔG^‡$ is the Gibbs free energy of activation
    • $R$ is the gas constant
  • The Gibbs free energy of activation ($ΔG^‡$) is related to the enthalpy of activation ($ΔH^‡$) and the entropy of activation ($ΔS^‡$) by the equation: ΔG=ΔHTΔSΔG^‡ = ΔH^‡ - TΔS^‡
  • By determining the values of $ΔH^‡$ and $ΔS^‡$ experimentally (through Arrhenius plots or temperature-dependent kinetic studies), one can calculate the rate constant using the Eyring equation

Collision Theory vs Transition State Theory

Limitations of Collision Theory

  • Collision theory does not account for the specific orientation of molecules during collisions, which is crucial for successful reactions
    • TST addresses this limitation by considering the geometry of the transition state
  • Collision theory does not provide a quantitative relationship between the activation energy and the rate constant
    • TST offers the Eyring equation to calculate the rate constant based on the Gibbs free energy of activation

Advantages of Transition State Theory

  • TST takes into account the entropy changes associated with the formation of the transition state
    • This can have a significant impact on the reaction rate, especially for reactions involving complex molecules or solvents (bimolecular reactions, enzymatic catalysis)
  • TST allows for the calculation of rate constants for elementary reactions
    • Collision theory is more applicable to overall reaction rates
  • However, TST assumes that all molecules that reach the transition state will form products
    • This may not always be the case due to the possibility of recrossing the activation energy barrier or the presence of competing reaction pathways (non-statistical dynamics)