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1.4 Arrhenius Equation and Activation Energy

1.4 Arrhenius Equation and Activation Energy

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

The Arrhenius equation connects reaction rate constants to temperature and activation energy, giving you a quantitative framework for predicting how fast reactions proceed under different conditions. In a Physical Chemistry course, this is where thermodynamic concepts meet kinetic observables, so getting comfortable with both the equation's derivation and its practical application is essential.

Arrhenius Equation and Reaction Rates

Temperature Dependence of Reaction Rates

The Arrhenius equation is:

k=AeEa/RTk = Ae^{-E_a/RT}

where kk is the rate constant, AA is the pre-exponential factor, EaE_a is the activation energy, RR is the gas constant (8.314J mol1K18.314 \, \text{J mol}^{-1} \text{K}^{-1}), and TT is the absolute temperature in Kelvin.

The exponential term eEa/RTe^{-E_a/RT} represents the fraction of molecules with sufficient energy to overcome the activation barrier. Because this term is exponential, even modest temperature increases produce large changes in kk. A common rule of thumb: a 10 K increase in temperature roughly doubles or triples the rate constant for many reactions near room temperature.

The physical basis comes from the Maxwell-Boltzmann distribution. At any temperature, molecular kinetic energies follow a distribution. As TT increases, the high-energy tail of this distribution extends further, meaning a larger fraction of molecules have energy Ea\geq E_a. That shift in the population above the energy threshold is what drives the rate increase.

Determining Activation Energy from Experimental Data

Taking the natural log of both sides of the Arrhenius equation gives the linearized form:

ln(k)=ln(A)EaR1T\ln(k) = \ln(A) - \frac{E_a}{R} \cdot \frac{1}{T}

This has the form y=b+mxy = b + mx, where:

  • y=ln(k)y = \ln(k)
  • x=1/Tx = 1/T
  • slope =Ea/R= -E_a/R
  • intercept =ln(A)= \ln(A)

Plotting ln(k)\ln(k) vs. 1/T1/T (an Arrhenius plot) should yield a straight line if EaE_a is approximately constant over the temperature range studied. You can extract EaE_a directly from the slope without knowing the reaction mechanism or the value of AA.

The underlying assumption is rooted in collision theory: a reaction occurs when molecules collide with (1) energy equal to or exceeding EaE_a and (2) proper geometric orientation. The Arrhenius equation captures the energy requirement through the Boltzmann factor, while orientation effects are folded into AA.

Activation Energy in Reactions

Temperature Dependence of Reaction Rates, Activation Energy and Temperature Dependence | Chemistry [Master]

Energy Barrier and Transition State

Activation energy (EaE_a) is the minimum energy required for reactants to reach the transition state, the highest-energy point along the reaction coordinate. The transition state is not a stable species; it's a transient configuration where old bonds are partially broken and new bonds are partially formed.

EaE_a equals the energy difference between the reactants and the transition state. A few things to keep in mind:

  • Higher EaE_a means fewer molecules have enough energy to react at a given temperature, so the reaction is slower.
  • EaE_a is always positive for an elementary step (you always need some energy to distort bonds into the transition state geometry).
  • The activation energy for the forward reaction differs from that of the reverse reaction by the overall reaction enthalpy: Ea,forwardEa,reverse=ΔHrxnE_{a,\text{forward}} - E_{a,\text{reverse}} = \Delta H_{\text{rxn}}.

For example, the combustion of gasoline has a relatively low EaE_a compared to the combustion of wood, which is why gasoline ignites more readily.

Catalysts and Activation Energy

A catalyst increases the reaction rate by providing an alternative pathway with a lower activation energy. The catalyst is not consumed and does not change the thermodynamics (ΔG\Delta G, ΔH\Delta H) of the overall reaction. It only changes the kinetics.

  • Enzymes are biological catalysts that can lower EaE_a by hundreds of kilojoules per mole, enabling reactions to proceed rapidly at body temperature.
  • On an energy diagram, a catalyzed reaction has the same reactant and product energy levels but a lower peak (transition state).

The Arrhenius equation also tells you that reactions with high EaE_a are more sensitive to temperature changes. You can see this from the equation: the larger EaE_a is, the more the exponential term eEa/RTe^{-E_a/RT} changes for a given change in TT. So catalysis (lowering EaE_a) not only speeds up a reaction but also makes its rate less temperature-dependent.

Activation Energy Calculation

Temperature Dependence of Reaction Rates, Activation energy, Arrhenius law

Arrhenius Plot Method

This is the most reliable method when you have rate data at multiple temperatures.

  1. Measure kk at several different temperatures.
  2. Calculate ln(k)\ln(k) and 1/T1/T for each data point.
  3. Plot ln(k)\ln(k) (y-axis) vs. 1/T1/T (x-axis).
  4. Perform a linear regression. The slope equals Ea/R-E_a/R.
  5. Solve for EaE_a: Ea=slope×RE_a = -\text{slope} \times R.

Worked example: If the slope of your Arrhenius plot is 5000K-5000 \, \text{K}, then:

Ea=(5000K)×8.314J mol1K1=41,570J mol141.6kJ mol1E_a = -(-5000 \, \text{K}) \times 8.314 \, \text{J mol}^{-1} \text{K}^{-1} = 41{,}570 \, \text{J mol}^{-1} \approx 41.6 \, \text{kJ mol}^{-1}

If the plot is noticeably curved, that's a sign EaE_a or AA may be temperature-dependent, and the simple Arrhenius model may not fully apply over that range.

Two-Point Method

When you only have rate constants at two temperatures, you can use the two-point form derived by subtracting the linearized Arrhenius equation at T1T_1 from that at T2T_2:

ln ⁣(k2k1)=EaR(1T11T2)\ln\!\left(\frac{k_2}{k_1}\right) = \frac{E_a}{R}\left(\frac{1}{T_1} - \frac{1}{T_2}\right)

Rearranging to solve for EaE_a:

Ea=Rln(k2/k1)1/T11/T2E_a = \frac{R \cdot \ln(k_2/k_1)}{1/T_1 - 1/T_2}

Worked example:

Given k1=2.5×103s1k_1 = 2.5 \times 10^{-3} \, \text{s}^{-1} at T1=300KT_1 = 300 \, \text{K} and k2=1.2×102s1k_2 = 1.2 \times 10^{-2} \, \text{s}^{-1} at T2=320KT_2 = 320 \, \text{K}:

  1. Compute the ratio: k2/k1=1.2×102/2.5×103=4.8k_2/k_1 = 1.2 \times 10^{-2} / 2.5 \times 10^{-3} = 4.8

  2. Take the natural log: ln(4.8)=1.569\ln(4.8) = 1.569

  3. Compute the reciprocal temperature difference: 1/3001/320=3.333×1033.125×103=2.083×104K11/300 - 1/320 = 3.333 \times 10^{-3} - 3.125 \times 10^{-3} = 2.083 \times 10^{-4} \, \text{K}^{-1}

  4. Solve: Ea=8.314×1.5692.083×104=62,600J mol162.6kJ mol1E_a = \frac{8.314 \times 1.569}{2.083 \times 10^{-4}} = 62{,}600 \, \text{J mol}^{-1} \approx 62.6 \, \text{kJ mol}^{-1}

A common mistake: make sure your temperatures are in Kelvin, not Celsius. Using °C will give you a completely wrong answer.

Pre-Exponential Factor Interpretation

Collision Frequency and Orientation

The pre-exponential factor AA captures everything about the rate other than the Boltzmann energy factor. In the context of collision theory, AA reflects two things:

  • Collision frequency (ZZ): how often reactant molecules collide per unit time per unit volume.
  • Steric factor (pp): the fraction of collisions that have the correct geometric orientation for reaction. This is always 1\leq 1.

So you can think of ApZA \approx p \cdot Z. Typical values of AA for gas-phase bimolecular reactions are on the order of 101010^{10} to 1011L mol1s110^{11} \, \text{L mol}^{-1} \text{s}^{-1}, while unimolecular reactions often have AA values around 1013s110^{13} \, \text{s}^{-1} (comparable to molecular vibrational frequencies).

A notably small AA relative to these benchmarks suggests significant steric requirements: the molecules need to be oriented in a very specific way for reaction to occur.

Entropy of Activation

Transition state theory (TST) provides a more rigorous interpretation of AA. In TST, the pre-exponential factor is related to the entropy of activation (ΔS\Delta S^\ddagger):

A=kBTheΔS/RA = \frac{k_B T}{h} \cdot e^{\Delta S^\ddagger / R}

where kBk_B is the Boltzmann constant and hh is Planck's constant.

  • A positive ΔS\Delta S^\ddagger means the transition state is more disordered than the reactants (e.g., a bond-breaking process), giving a larger AA.
  • A negative ΔS\Delta S^\ddagger means the transition state is more ordered (e.g., two molecules coming together into a rigid complex), giving a smaller AA.

Note that this TST expression introduces a weak temperature dependence into AA through the TT in the prefactor. For most practical purposes over moderate temperature ranges, this dependence is small compared to the exponential term and is often neglected. However, over very wide temperature ranges, deviations from strict Arrhenius linearity can sometimes be attributed to this effect.

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