Radical Chain Reactions: Initiation, Propagation, Termination

Overview to revise: A single UV photon striking a bromine molecule can trigger the destruction of a trillion molecules of methane before the chain finally dies. This is the astonishing arithmetic of a radical chain reaction. Unlike the polar, two-electron world of nucleophiles attacking electrophiles, radical chemistry runs on unpaired electrons. It uses single-barbed "fishhook" arrows and a self-sustaining cycle. Once lit, this cycle propagates almost for free. Understanding why some C–H bonds break preferentially over others requires care. So does understanding why chlorination is messy while bromination is clean. Explaining why a chain eventually stops requires tracking every electron individually rather than in pairs. This matters because radical chain mechanisms are not a curiosity confined to gas-phase halogenations in textbooks. They govern industrial cracking of petroleum and the combustion chemistry inside every engine. They drive the autoxidation that turns cooking oil rancid and drugs unstable on a shelf. They also govern the vulcanization and degradation of rubber. Most importantly for a working chemist, they underlie the radical chain mechanisms deliberately harnessed in Radical Polymerization. These mechanisms make polyethylene, PVC, and countless polymers. The same logic of initiation–propagation–termination reappears whenever an unpaired electron needs a productive, catalytic pathway. Otherwise, it would simply annihilate itself. The big picture is a kinetic one. A radical chain is a closed loop of elementary steps. A reactive radical is consumed in one step, and exactly one new radical is regenerated in a subsequent step. So the total radical population (ideally) never runs out. It continues until an accidental radical–radical encounter kills it. Whether a given C–H bond is attacked, and how selectively, is not decided by overall thermodynamics. Instead, it is decided by the height of a specific transition state in the propagation cycle. This is a distinction between thermodynamic favorability and kinetic selectivity. Radical halogenation illustrates this distinction better than almost any other reaction class. This article builds the mechanism from first principles. It explains what initiation, propagation, and termination actually are in electron-pushing terms. It shows why Hammond-postulate reasoning explains the wildly different selectivities of Cl• versus Br•. It also shows how bond dissociation energies (BDEs) let you compute, quantitatively, whether each propagation step is exothermic or endothermic. Three fully worked problems anchor the theory to numbers you can check by hand. These are a foundational halogenation, an applied selectivity/stereochemistry problem, and a competition-level relative-rate calculation.

Key takeaways
  • A radical chain has three phases: initiation (radicals created, usually by homolysis), propagation (radicals consumed and regenerated in a repeating cycle), termination (two radicals combine and the chain dies).
  • Fishhook (single-barbed) arrows track one electron at a time; every propagation step must be a bimolecular elementary step with one radical in and one radical out.
  • Each propagation step's enthalpy is ΔH=BDE(bond broken)−BDE(bond formed)\Delta H = \text{BDE(bond broken)} - \text{BDE(bond formed)}; summing the two propagation steps gives the overall reaction enthalpy.
  • Selectivity is controlled by the rate-determining H-abstraction step, not by the thermodynamics of the overall halogenation — governed by the Hammond postulate.
  • Chlorination (low barrier, early/reactant-like TS) is fast but poorly selective; bromination (high barrier, late/product-like TS) is slow but highly selective — the reactivity–selectivity principle.
  • Key idea: a radical chain is a catalytic cycle for atoms, not electrons — each propagation step trades one radical for another of nearly identical energy, and only the transition-state energies, not the endpoints, decide which C–H bond reacts.

Where this lives today

Radical chain mechanisms are the operating principle behind industrial free-radical polymerization of ethylene, vinyl chloride, styrene, and acrylates, in which an initiator (peroxide or azo compound) generates the first radical and a propagating polymer-chain radical adds monomer thousands of times before termination — the direct scale-up of exactly the initiation/propagation/termination framework built here, elaborated further in Radical Polymerization. Autoxidation, the slow radical chain oxidation of fats, oils, rubber, and plastics by atmospheric O₂, follows the identical logic with a peroxyl radical (ROO•) as the chain carrier, and is why antioxidants (radical-trapping phenols like BHT or vitamin E) are added to foods and polymers — they intercept the chain by donating a very weak O–H bond to the peroxyl radical, generating a resonance-stabilized, unreactive phenoxyl radical that cannot efficiently continue the chain, effectively acting as inhibitors that shorten chain length dramatically. Combustion chemistry, atmospheric ozone-depletion chemistry (chlorofluorocarbon photolysis generating Cl• that catalytically destroys ozone in an analogous propagation loop), and industrial halogenation processes for making chlorinated solvents all run on the same three-phase mechanism. In synthesis, radical brominations with NBS (Wohl–Ziegler conditions) remain a standard method for allylic and benzylic functionalization, and radical chain thinking is the conceptual gateway to understanding reactive intermediates more broadly, including the electron-counting and orbital arguments used for Carbenes: Structure and Generation, where analogous single-electron and two-electron bookkeeping recurs in a different guise.

Ask the tutor: How does the Evans–Polanyi principle quantitatively connect bond dissociation energies to activation energies across a whole series of radical abstractions, and how would you use it to predict a rate ratio you haven't measured?

The physical picture

A radical is a species with an unpaired electron in a nonbonding or partially bonding orbital — highly reactive because that orbital wants to pair up. Homolysis of a weak bond (Cl–Cl, Br–Br, O–O in a peroxide, or a C–C bond in an initiator like AIBN) supplies the first radicals; from then on, the chemistry is dictated by two facts about radicals that differ fundamentally from ions. First, radicals are usually not stabilized or destabilized by solvent polarity the way ions are, so radical reactions tolerate nonpolar, aprotic conditions (CCl₄, gas phase) where ionic mechanisms would be hopelessly slow. Second, a radical reacting with a closed-shell molecule can only do one of a few things: abstract an atom (usually H or halogen), add to a π bond, or fragment — and in each case exactly one new radical is produced, conserving the total spin. The defining topology of a chain reaction is that propagation steps link together so that the radical consumed by step nn is exactly the radical produced by step n−1n{-}1. Draw the two propagation steps of methane chlorination stacked vertically and you see immediately that Cl• is regenerated:

Cl∙+CH4⟶HCl+∙CH3\text{Cl}^{\bullet} + \text{CH}_4 \longrightarrow \text{HCl} + {}^{\bullet}\text{CH}_3
∙CH3+Cl2⟶CH3Cl+Cl∙{}^{\bullet}\text{CH}_3 + \text{Cl}_2 \longrightarrow \text{CH}_3\text{Cl} + \text{Cl}^{\bullet}

Add these two equations and the radicals cancel, leaving the observed stoichiometry CH4+Cl2→CH3Cl+HCl\text{CH}_4 + \text{Cl}_2 \rightarrow \text{CH}_3\text{Cl} + \text{HCl} — but that overall equation tells you nothing about why one C–H bond reacts faster than another. That information lives entirely in the first propagation step's transition state.

Figure
Anatomy of a radical chain: initiation, propagation loop, termination
Radical chain mechanism — CH₄ + Cl₂ → CH₃Cl + HCl Initiation (hν or Δ, once per chain) Cl–Cl --hν--> Cl• + •Cl Propagation cycle (repeats ~10³–10⁴ times) Cl• + CH₄ → HCl + •CH₃ (ΔH ≈ +1 kJ/mol) •CH₃ + Cl₂ → CH₃Cl + Cl• (ΔH ≈ −101 kJ/mol) Cl• regenerated •CH₃ carried forward Termination (rare, radical + radical) Cl• + •CH₃ → CH₃Cl •CH₃ + •CH₃ → CH₃CH₃ Cl• + Cl• → Cl₂ Net: overall ΔH = (+1) + (−101) = −100 kJ/mol per cycle — but selectivity is set by step 1's barrier, not this sum.

Look closely at the numbers in the figure: step 1 (Cl• abstracting H from methane) is almost thermoneutral, while step 2 (methyl radical grabbing Cl from Cl₂) is strongly exothermic. This asymmetry is the rule, not the exception, in halogenation: the first propagation step, generating the carbon radical, is the slow, selectivity-determining step, while the second step, regenerating the halogen radical, is fast and essentially indiscriminate. Selectivity is decided at the first transition state, and the Hammond postulate tells you what that transition state looks like. The Hammond postulate states that a transition state resembles whichever adjacent species (reactant or product) it is closer to in energy. For an endothermic elementary step, the TS is product-like (a "late" TS, close in structure and energy to the radical intermediate); for an exothermic step, the TS is reactant-like ("early", little radical character developed). Because H-abstraction by Cl• is nearly thermoneutral (small ΔH\Delta H, low barrier, ~4 kJ/mol for a typical secondary C–H), the TS is early and barely distinguishes between primary, secondary, and tertiary C–H bonds — chlorination is unselective. H-abstraction by Br• is substantially endothermic (barrier ~50–75 kJ/mol), so the TS is late and product-like, meaning it already "feels" most of the stability difference between a primary and a tertiary radical — bromination is highly selective.

Figure
Hammond postulate: why Br• is selective and Cl• is not
Reaction coordinate for X• + R–H → HX + R• Cl• abstraction (ΔH ≈ 0, low Ea) early TS (reactant-like) R–H + Cl• R• + HCl Br• abstraction (ΔH large +, high Ea) late TS (product-like, radical character developed) R–H + Br• R• + HBr reaction coordinate → potential energy

The core ideas

Every propagation step's enthalpy follows directly from bond dissociation energies (BDEs), which are tabulated, measurable, and additive:

ΔHstep=BDE(bond broken)−BDE(bond formed)\Delta H_{\text{step}} = \text{BDE}(\text{bond broken}) - \text{BDE}(\text{bond formed})

where: BDE(bond broken) is the homolytic bond strength of the bond in the starting material of that step, and BDE(bond formed) is the strength of the new bond created in the product of that step; both are measured as positive numbers (energy required to homolyze), so a step is exothermic when it forms a stronger bond than it breaks. Summing the two propagation-step enthalpies gives the overall reaction enthalpy, since the radical intermediate's bond terms cancel:

ΔHoverall=ΔHstep 1+ΔHstep 2\Delta H_{\text{overall}} = \Delta H_{\text{step 1}} + \Delta H_{\text{step 2}}

where: ΔHoverall\Delta H_{\text{overall}} must equal the BDE of the bonds broken in reactants (C–H and X–X) minus BDE of bonds formed in products (H–X and C–X), independent of any radical intermediate. Selectivity between two C–H bonds (say tertiary vs. primary) is expressed as a rate ratio, computed from the Arrhenius form applied to the rate-determining H-abstraction step:

k3∘k1∘=A3∘A1∘exp⁡ ⁣(−Ea,3∘−Ea,1∘RT)\frac{k_{3^\circ}}{k_{1^\circ}} = \frac{A_{3^\circ}}{A_{1^\circ}}\exp\!\left(-\frac{E_{a,3^\circ}-E_{a,1^\circ}}{RT}\right)

where: AA are pre-exponential (frequency/steric) factors, often assumed comparable per C–H bond for a first approximation, EaE_a are the experimental activation energies for abstraction from each type of C–H bond, R=8.314 J mol−1K−1R = 8.314\ \text{J mol}^{-1}\text{K}^{-1}, and TT is the absolute temperature. Because statistical (number of equivalent H's) and electronic (bond-strength/radical-stability) effects both matter, the observed product ratio is:

product from nA H’sproduct from nB H’s=nA kAnB kB\frac{\text{product from }n_A\text{ H's}}{\text{product from }n_B\text{ H's}} = \frac{n_A \, k_A}{n_B \, k_B}

where: nA,nBn_A, n_B are the number of chemically equivalent hydrogens of each type on the substrate, and kA,kBk_A, k_B are the per-hydrogen rate constants for abstraction of that type.

Derivation AMechanism 1 — Radical chlorination of methane: initiation, propagation, termination with fishhook arrows

Goal. Construct, arrow by arrow, every elementary step of CH4+Cl2→hνCH3Cl+HCl\text{CH}_4 + \text{Cl}_2 \xrightarrow{h\nu} \text{CH}_3\text{Cl} + \text{HCl}, and verify the enthalpy of each step from BDEs (BDE Cl–Cl = 242 kJ/mol, BDE CH₃–H = 439 kJ/mol, BDE H–Cl = 431 kJ/mol, BDE CH₃–Cl = 350 kJ/mol).

Step 1 — Initiation (photolytic homolysis). A photon of UV light (roughly 250–400 nm, matching the weak, 242 kJ/mol Cl–Cl σ bond) is absorbed by Cl₂. The bonding σ electron pair splits symmetrically: two fishhook arrows, each starting at the midpoint of the Cl–Cl bond and pointing to one chlorine nucleus, show one electron going to each atom.

Cl ⁣− ⁣Cl→hνCl∙+∙Cl\text{Cl}\!-\!\text{Cl} \xrightarrow{h\nu} \text{Cl}^{\bullet} + {}^{\bullet}\text{Cl}

This step consumes energy equal to the Cl–Cl BDE (242 kJ/mol) — it is strongly endothermic and occurs only because photon energy, not thermal energy, supplies the activation. Initiation happens only a tiny number of times relative to the propagation cycles that follow; it is not part of the repeating loop.

Step 2 — Propagation, part A: chlorine radical abstracts hydrogen. The chlorine radical's half-filled 3p orbital attacks a C–H σ bond of methane. Two fishhook arrows are drawn: one from the C–H bonding pair to the H nucleus forming the new H–Cl bond, and one from Cl•'s unpaired electron to the same H, so that the two electrons pair into the new H–Cl bond while the C–H bonding pair's other electron is left behind on carbon as the new radical. More carefully: fishhook 1 goes from the midpoint of the C–H bond toward the incoming Cl atom (this electron ends up paired with Cl's electron in the new H–Cl bond); fishhook 2 is Cl•'s own unpaired electron, arrow drawn from the Cl radical dot to the forming bond. The transition state is a near-linear C···H···Cl three-center, three-electron array.

Cl∙+H3C ⁣− ⁣H⟶Cl ⁣− ⁣H+∙CH3\text{Cl}^{\bullet} + \text{H}_3\text{C}\!-\!\text{H} \longrightarrow \text{Cl}\!-\!\text{H} + {}^{\bullet}\text{CH}_3

Enthalpy: bond broken is C–H (439 kJ/mol), bond formed is H–Cl (431 kJ/mol).

ΔHstep 2=439−431=+8 kJ/mol\Delta H_{\text{step 2}} = 439 - 431 = +8\ \text{kJ/mol}

Slightly endothermic — consistent with an early, reactant-like TS by Hammond's postulate, and consistent with chlorination's low selectivity.

Step 3 — Propagation, part B: methyl radical abstracts chlorine from Cl₂. The methyl radical's unpaired electron (in a nearly planar, sp²-like orbital on carbon) attacks one chlorine atom of Cl₂. Fishhook 1: from •CH₃'s unpaired electron to the near Cl atom, forming the new C–Cl bond. Fishhook 2: from the Cl–Cl bonding pair, one electron moves onto the far chlorine atom, regenerating a chlorine radical.

∙CH3+Cl ⁣− ⁣Cl⟶CH3 ⁣− ⁣Cl+Cl∙{}^{\bullet}\text{CH}_3 + \text{Cl}\!-\!\text{Cl} \longrightarrow \text{CH}_3\!-\!\text{Cl} + \text{Cl}^{\bullet}

Enthalpy: bond broken is Cl–Cl (242 kJ/mol), bond formed is C–Cl (350 kJ/mol).

ΔHstep 3=242−350=−108 kJ/mol\Delta H_{\text{step 3}} = 242 - 350 = -108\ \text{kJ/mol}

Strongly exothermic, fast, essentially barrierless in comparison to step 2 — this step is never rate- or selectivity-limiting.

Step 4 — Sum the propagation steps. Adding steps 2 and 3, the Cl• and •CH₃ intermediates cancel exactly (one Cl• is consumed in step 2, one is produced in step 3; one •CH₃ is produced in step 2, one is consumed in step 3):

ΔHoverall=(+8)+(−108)=−100 kJ/mol\Delta H_{\text{overall}} = (+8) + (-108) = -100\ \text{kJ/mol}

This matches the direct BDE calculation for the overall reaction, BDE(C–H)+BDE(Cl–Cl)−BDE(H–Cl)−BDE(C–Cl)=439+242−431−350=−100\text{BDE(C–H)} + \text{BDE(Cl–Cl)} - \text{BDE(H–Cl)} - \text{BDE(C–Cl)} = 439 + 242 - 431 - 350 = -100 kJ/mol, confirming internal consistency: propagation steps sum to the correct overall thermodynamics regardless of how many times the cycle repeats.

Step 5 — Termination (chain-breaking, radical–radical combination). Any two radicals that happen to encounter each other can combine without a barrier, since pairing two unpaired electrons into a new bond is barrierless (no activation energy is needed to form a bond from two radicals — the "barrier" for radical recombination is essentially zero). Three possible termination events, each shown with a single fishhook arrow from each radical's unpaired electron converging into the new bond:

Cl∙+∙Cl→Cl2,∙CH3+∙CH3→CH3CH3,Cl∙+∙CH3→CH3Cl\text{Cl}^{\bullet} + {}^{\bullet}\text{Cl} \rightarrow \text{Cl}_2, \qquad {}^{\bullet}\text{CH}_3 + {}^{\bullet}\text{CH}_3 \rightarrow \text{CH}_3\text{CH}_3, \qquad \text{Cl}^{\bullet} + {}^{\bullet}\text{CH}_3 \rightarrow \text{CH}_3\text{Cl}

Termination is intrinsically rare relative to propagation because radical concentrations are minuscule (steady-state, typically 10−910^{-9}–10−1110^{-11} M) — the probability of two radicals meeting each other is far lower than a radical meeting the vastly more abundant closed-shell substrate (CH₄ or Cl₂, present at molar concentrations). This concentration mismatch, not any intrinsic slowness of radical–radical bonding, is what keeps chains long (often 10310^3–10410^4 propagation cycles per initiation event).

Go deeper · Derivation B · 2 minMechanism 2 — Selectivity in bromination of 2-methylbutane: Hammond postulate quantified with relative rates
Derivation BMechanism 2 — Selectivity in bromination of 2-methylbutane: Hammond postulate quantified with relative rates

Goal. Show mechanistically why Br• abstracts a tertiary hydrogen from 2-methylbutane far more selectively than Cl• would, and compute the actual product ratio using standard per-hydrogen relative rates (1°:2°:3° = 1:82:1600 for bromination at 25 °C, versus 1:3.8:5 for chlorination).

Step 1 — Draw the substrate and count H environments. 2-Methylbutane, (CH3)2CH–CH2–CH3(\text{CH}_3)_2\text{CH–CH}_2\text{–CH}_3, has four distinct hydrogen environments: 6 equivalent primary H's on the two methyls of the isopropyl-like end (C1, C1′), 1 tertiary H on C2, 2 secondary H's on C3, and 3 primary H's on C4 (a terminal methyl distinct from C1/C1′ by connectivity — though for a first pass we group all primary H's as similar for illustration, chemists usually track each site separately). For clarity, label them explicitly:

H3C⏟C1: 3H−CH⏟C2: 1H(CH3)−CH2⏟C3: 2H−CH3⏟C4: 3H\underbrace{\text{H}_3\text{C}}_{\text{C1: 3H}}-\underbrace{\text{CH}}_{\text{C2: 1H}}(\text{CH}_3)-\underbrace{\text{CH}_2}_{\text{C3: 2H}}-\underbrace{\text{CH}_3}_{\text{C4: 3H}}

with the branch methyl contributing another 3 equivalent primary H's, giving 9 primary H total (C1 + branch + C4), 2 secondary H (C3), and 1 tertiary H (C2).

Step 2 — Mechanism of the selectivity-determining step. In the propagating H-abstraction, Br∙+R–H→HBr+R∙\text{Br}^{\bullet} + \text{R–H} \rightarrow \text{HBr} + \text{R}^{\bullet}, the fishhook arrows are exactly analogous to Mechanism 1: one arrow from the C–H bonding pair to hydrogen (forming H–Br), one arrow from Br•'s unpaired electron into the same forming bond. Because ΔH\Delta H for this step is large and positive (bromination of a 3° C–H: BDE(3° C–H) ≈ 400 kJ/mol, BDE(H–Br) = 366 kJ/mol, giving ΔH≈+34\Delta H \approx +34 kJ/mol), the Hammond postulate places the TS late, structurally and energetically close to the free tertiary radical.

Step 3 — Why "late" means "selective". A late TS has substantial radical character already developed at carbon. The relative stability of 3° > 2° > 1° free radicals (due to hyperconjugative donation from adjacent C–H σ bonds into the singly-occupied p orbital, and modest inductive stabilization from alkyl groups) is therefore already partly felt in the transition state itself, lowering EaE_a for tertiary abstraction much more than for primary. This is why the experimental EaE_a differences for Br• are large enough to give a 1600:1 per-hydrogen rate advantage for 3° over 1°, while for Cl• (early TS, little radical character yet) the same effect gives only a 5:1 advantage.

Step 4 — Compute the statistically corrected product ratio for bromination. Using per-hydrogen rate ratios 1° : 2° : 3° = 1 : 82 : 1600 and hydrogen counts n1°=9n_{1°}=9, n2°=2n_{2°}=2, n3°=1n_{3°}=1:

ratio (1°:2°:3° products)=(9×1):(2×82):(1×1600)=9:164:1600\text{ratio (1°:2°:3° products)} = (9 \times 1) : (2 \times 82) : (1 \times 1600) = 9 : 164 : 1600

Total weight =9+164+1600=1773= 9 + 164 + 1600 = 1773, so the tertiary bromide alone constitutes

16001773×100%≈90.2%\frac{1600}{1773} \times 100\% \approx 90.2\%

of the monobromination product mixture — overwhelming selectivity for a single tertiary C–H out of twelve total hydrogens, despite that hydrogen being statistically the least abundant.

Step 5 — Contrast with chlorination of the same substrate. Using 1°:2°:3° = 1:3.8:5 for Cl• and the same H counts:

(9×1):(2×3.8):(1×5)=9:7.6:5(9 \times 1) : (2 \times 3.8) : (1 \times 5) = 9 : 7.6 : 5

Total =21.6= 21.6, giving the tertiary chloride only

521.6×100%≈23%\frac{5}{21.6}\times 100\% \approx 23\%

of the product — chlorination gives a nearly statistical mixture of all four isomeric chlorides, confirming Mechanism 1's conclusion that Cl•'s early, low-barrier TS is nearly blind to radical stability, while Br•'s late, high-barrier TS is exquisitely sensitive to it. This is the reactivity–selectivity principle in its cleanest experimental form.

Worked examples

Example 1 (foundational): Enthalpy and feasibility of propagation steps in bromination of methane. Given BDE(Br–Br) = 193 kJ/mol, BDE(CH₃–H) = 439 kJ/mol, BDE(H–Br) = 366 kJ/mol, BDE(CH₃–Br) = 293 kJ/mol, evaluate whether a Br• chain for methane bromination is thermally sustainable. Initiation: Br₂ homolysis requires 193 kJ/mol (weaker than Cl–Cl, so Br₂ initiates more easily, e.g. thermally or with visible light). Propagation step A, Br∙+CH4→HBr+∙CH3\text{Br}^{\bullet} + \text{CH}_4 \rightarrow \text{HBr} + {}^{\bullet}\text{CH}_3:

ΔHA=439−366=+73 kJ/mol\Delta H_A = 439 - 366 = +73\ \text{kJ/mol}

This is substantially endothermic — much more so than the analogous chlorination step (+8 kJ/mol) — and this large positive ΔH\Delta H is exactly why bromination is slower overall than chlorination, and why it needs a persistently higher temperature or continuous illumination to keep the chain alive; a chain with a strongly endothermic, high-barrier propagation step turns over less often per unit time. Propagation step B, ∙CH3+Br2→CH3Br+Br∙{}^{\bullet}\text{CH}_3 + \text{Br}_2 \rightarrow \text{CH}_3\text{Br} + \text{Br}^{\bullet}:

ΔHB=193−293=−100 kJ/mol\Delta H_B = 193 - 293 = -100\ \text{kJ/mol}

Overall:

ΔHoverall=73+(−100)=−27 kJ/mol\Delta H_{\text{overall}} = 73 + (-100) = -27\ \text{kJ/mol}

The reaction is exothermic overall but far less so than chlorination's −100-100 kJ/mol, precisely because step A costs so much more. As a limiting-case check: if step A's ΔH\Delta H ever exceeded the exothermicity available from step B (i.e., if ΔHA>100\Delta H_A > 100 kJ/mol), the overall reaction would become endothermic and the chain thermodynamically nonviable at ordinary temperatures — this is exactly why radical fluorination (with an enormous, explosively exothermic step B but also a huge step A cost that turns out smaller than F₂'s tiny BDE) is dangerously fast, while radical iodination fails altogether, as shown next.

Example 2 (applied): Why iodination of alkanes does not proceed as a useful chain reaction. Given BDE(I–I) = 151 kJ/mol, BDE(CH₃–H) = 439 kJ/mol, BDE(H–I) = 297 kJ/mol, BDE(CH₃–I) = 234 kJ/mol. Propagation step A, I∙+CH4→HI+∙CH3\text{I}^{\bullet} + \text{CH}_4 \rightarrow \text{HI} + {}^{\bullet}\text{CH}_3:

ΔHA=439−297=+142 kJ/mol\Delta H_A = 439 - 297 = +142\ \text{kJ/mol}

This is a huge endothermicity for an elementary bimolecular step — by the Hammond postulate the TS is not just "late" but essentially beyond the product in character, with an activation energy so high (well above 140 kJ/mol, since Ea≥ΔHE_a \geq \Delta H for an endothermic step) that at ordinary temperatures this step simply does not turn over at a useful rate. This single fact — not the overall thermodynamics — is why "radical iodination" is not a synthetically useful reaction, even though the second propagation step remains favorable:

ΔHB=151−234=−83 kJ/mol\Delta H_B = 151 - 234 = -83\ \text{kJ/mol}

giving an overall ΔHoverall=142−83=+59\Delta H_{\text{overall}} = 142 - 83 = +59 kJ/mol — the overall reaction is endothermic, consistent with (and reinforcing) the kinetic failure of step A. This is the clearest illustration in this entire family of reactions that a chain's feasibility is set by its slowest, most endothermic elementary step, not by whether the total reaction happens to be downhill — indeed here both diagnoses agree, but Examples 1 and this one together show the two criteria (kinetic step-by-step, thermodynamic overall) must both be checked, since they can in principle disagree (as they do for bromination's exothermic-overall-but-kinetically-sluggish first step).

Example 3 (competition-level): Stereochemistry and rate ratio in allylic bromination with NBS. Predict the product distribution (ignoring stereochemistry first, then addressing it) when 4-methylcyclohexene undergoes radical allylic bromination with N-bromosuccinimide (NBS), and explain why the allylic radical intermediate scrambles the position of substitution. Mechanism. NBS serves as a slow, continuous low-concentration source of Br₂ (via reaction with trace HBr, keeping [Br2][\text{Br}_2] low enough to favor the radical chain over ionic addition — the "Wohl–Ziegler" conditions). The propagating radical is still Br•, which abstracts one of the two allylic C–H bonds (weaker than ordinary sp³ C–H, roughly 360–370 kJ/mol, because the resulting radical is resonance-stabilized). Fishhook arrows: one from the allylic C–H bonding pair to the incoming H (forming H–Br), one from Br•'s unpaired electron into that same bond — identical topology to Mechanism 1's step 2, but now the resulting carbon radical is allylic, i.e., delocalized. Once formed, the allylic radical is best drawn as a resonance hybrid with unpaired spin density on both termini of the original allyl system: two fishhook-connected resonance structures,

∙Ca ⁣= ⁣Cb ⁣− ⁣Cc  ⟷  Ca ⁣= ⁣Cb ⁣− ⁣∙Cc{}^{\bullet}\text{C}_a\!=\!\text{C}_b\!-\!\text{C}_c \;\longleftrightarrow\; \text{C}_a\!=\!\text{C}_b\!-\!{}^{\bullet}\text{C}_c

drawn with a curved arrow from the p orbital bearing the radical, through the adjacent π bond, shifting the double bond and relocating the unpaired electron. This delocalization is why radical allylic bromination characteristically gives a mixture of the "direct" substitution product and the "transposed" (allylic-shift) product: the second propagation step, ∙Ca=Cb−Cc (or resonance partner)+Br2→product+Br∙{}^{\bullet}\text{C}_a{=}\text{C}_b{-}\text{C}_c \text{ (or resonance partner)} + \text{Br}_2 \rightarrow \text{product} + \text{Br}^{\bullet}, can deliver bromine to either terminus of the delocalized radical, because Br₂ can approach either lobe of the SOMO with comparable ease. For 4-methylcyclohexene, abstraction occurs preferentially at C3 (or equivalently C6 by symmetry), generating an allylic radical delocalized over C1–C2–C3 (numbering the alkene carbons C1=C2), and Br delivery at the less hindered terminus is typically favored, but both allylic bromides (direct and transposed double-bond-shifted product) are observed experimentally in ratios that depend on sterics and the stability of the resulting alkene (Zaitsev-type stabilization of the more substituted double bond in the product often biases the ratio). The key exam point: the regiochemical scrambling is a direct, structural consequence of spin delocalization in the intermediate, not a separate mechanism — it is built into the resonance structure of the radical itself, exactly as allylic cation scrambling is built into carbocation resonance in SN1S_N1/SN1′S_N1' chemistry, but here the delocalized species is a radical rather than a cation, so no external nucleophile or solvent effect is needed to see both products form.

Limiting cases, scope & common traps

SituationWhat actually happensWhy
Highly exothermic propagation step (e.g., R• + Br₂)Fast, low EaE_a, early TS, unselective in that stepHammond postulate: exothermic step ⇒ reactant-like TS
Highly endothermic propagation step (e.g., Br• + R–H)Slow, high EaE_a, late TS, highly selective in that stepHammond postulate: endothermic step ⇒ product-like TS
Overall ΔHoverall<0\Delta H_{\text{overall}} < 0 but one propagation step is very endothermicChain can still be thermally impractical (e.g., iodination borderline; F₂ dangerously fast)Rate is set by the slowest step's EaE_a, not by overall ΔH\Delta H
Very low radical concentration (steady state)Chains are long; termination is rareTermination requires two radicals to meet; propagation only needs one radical + one abundant closed-shell molecule
Radical adjacent to π system (allylic, benzylic)Resonance-delocalized radical; product mixtures from both terminiSpin density spread over multiple carbons in the SOMO
Chiral center at the radical carbonRacemization at that carbon (if it becomes the radical)sp³ → sp² radical is planar (or rapidly pyramidally inverting), destroying the original stereocenter

The chemist behind it

The systematic understanding of chain reactions — the concept that a single initiating event could multiply into thousands of product-forming cycles via a self-propagating loop — emerged from the study of gas-phase kinetics and combustion in the 1920s–30s, most famously through the work of Nikolay Semyonov and Cyril Hinshelwood, who shared the 1956 Nobel Prize in Chemistry for elucidating the mechanism of chemical chain reactions, including the branched chains responsible for explosive combustion. Their insight — that reaction rates in many gas-phase and combustion systems could not be explained by simple bimolecular collision theory alone, but required a self-multiplying radical mechanism with distinct initiation, propagation, and (for explosions) branching steps — reshaped physical organic chemistry's entire vocabulary for describing radical processes, the same vocabulary (fishhook arrows, chain length, inhibitor) used for organic halogenation, autoxidation, and polymerization chemistry ever since.

Origins · 1 minNikolay Nikolaevich Semyonov and how this was discovered
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Nikolay Nikolaevich Semyonov
1896–1986 · Soviet physical chemist, pioneer of chain-reaction kinetics and combustion theory

Semyonov developed the theory of branched-chain reactions to explain why certain gas mixtures ignite explosively above a sharply defined pressure and temperature threshold, rather than reacting at a smooth, gradually increasing rate. He showed that when a propagation step can generate more than one new radical (branching), the radical population grows exponentially rather than staying constant, producing the sudden ignition limits observed in real combustion — a phenomenon inexplicable by ordinary (unbranched) chain kinetics of the kind seen in simple halogenations.

History
- 1913 — Max Bodenstein proposes chain mechanisms to explain anomalously large quantum yields in the H₂/Cl₂ photoreaction.
- 1925–1928 — Semyonov and Hinshelwood independently develop branched-chain theory to explain explosion limits in gas-phase oxidation.
- 1929–1934 — Friedrich Paneth's mirror experiments provide direct physical evidence for free alkyl radicals as real, detectable intermediates.
- 1937 — M. S. Kharasch and Frank Mayo explain the "peroxide effect" (anti-Markovnikov HBr addition) as a radical chain mechanism, cementing radical chains in organic synthesis.
- 1956 — Semyonov and Hinshelwood awarded the Nobel Prize in Chemistry for mechanisms of chemical reactions, centered on chain-reaction theory.
What exactly is a "fishhook" arrow and how does it differ from a normal curved arrow?

A fishhook arrow has a single barb and represents the movement of one electron, used exclusively in radical mechanisms. A normal curved (two-barbed) arrow represents movement of an electron pair, used in polar/ionic mechanisms. In a homolysis step, two fishhook arrows point outward from the bond, one to each resulting atom, showing the pair splitting one-electron-each; in a radical addition or abstraction, you typically need two fishhooks together (one from the radical's unpaired electron, one from the bond being broken) to correctly show that the new bond gets one electron from each source while a new radical is left over.

Why does chlorination give a mixture of products while bromination gives one dominant product?

The first propagation step (halogen radical abstracting a C–H hydrogen) is the selectivity-determining step. For Cl•, this step is close to thermoneutral, so by the Hammond postulate the transition state is early and reactant-like, showing little of the developing radical's stability — so all C–H bonds react at similar rates, statistically weighted mostly by how many hydrogens of each type exist. For Br•, the same step is strongly endothermic, giving a late, product-like transition state that already reflects most of the stability difference between primary, secondary, and tertiary radicals, so the more stable radical's pathway dominates overwhelmingly.

Does a radical chain reaction ever stop on its own, and why doesn't it go on forever?

Yes — it stops when two radicals collide and combine in a termination step, which permanently removes two chain carriers from the system without regenerating any. Because radical concentrations during propagation are extremely low (often 10⁻⁹–10⁻¹¹ M), such radical–radical encounters are statistically rare compared to a radical meeting an abundant substrate molecule, so a chain can run through many thousands of propagation cycles before termination finally occurs. Chains also stop early if an inhibitor (like a phenolic antioxidant or O₂ itself in some contexts) intercepts a chain-carrying radical and converts it into an unreactive species.

How can I quickly tell whether a given step is initiation, propagation, or termination?

Count radicals on each side of the elementary equation. Initiation: zero radicals in, two (or more) radicals out — net radical creation, usually needs external energy (heat or light) since it breaks a bond without forming a compensating one. Propagation: exactly one radical in, exactly one radical out — this is what keeps a chain "alive" indefinitely and is always drawn as an ongoing repeating cycle. Termination: two radicals in, zero radicals out (a closed-shell product) — this is the only step that destroys chain carriers.

Why is radical fluorination of alkanes so violent, and radical iodination essentially impossible?

Both extremes trace back to the same enthalpy bookkeeping. Fluorination's first propagation step (F• + R–H → HF + R•) is enormously exothermic because the H–F bond formed (~565 kJ/mol) is far stronger than the C–H bond broken (~439 kJ/mol), giving a huge negative ΔH and an essentially barrierless, extremely fast, poorly controllable reaction — often explosive. Iodination's analogous step (I• + R–H → HI + R•) is strongly endothermic (+142 kJ/mol for methane) because the H–I bond formed (~297 kJ/mol) is much weaker than the C–H bond broken, giving a prohibitively high activation energy that the reaction essentially never surmounts at ordinary temperatures, so the chain never gets going in a useful way.

Does the Hammond postulate apply only to radical reactions?

No — the Hammond postulate is a completely general statement about transition-state structure that applies to any elementary step, ionic, pericyclic, or radical: an exothermic step has an early, reactant-like TS, and an endothermic step has a late, product-like TS. It happens to be unusually easy to illustrate with radical halogenation because the two propagation steps have such starkly different thermicities (one nearly neutral or endothermic, one strongly exothermic) and because the selectivity consequence (statistical vs. radical-stability-driven product ratios) is so experimentally clean and quantifiable.

What role does bond dissociation energy play beyond predicting ΔH of each step?

BDEs also directly predict relative rates through the Evans–Polanyi/Bell–Evans–Polanyi principle, a linear free-energy relationship stating that for a series of structurally similar H-abstraction steps, activation energy correlates linearly with the reaction enthalpy of that step: weaker C–H bonds (lower BDE, more stable resulting radical) correlate with lower activation energies. This is precisely why tertiary C–H bonds (BDE ≈ 400 kJ/mol, weaker than primary's ≈ 421 kJ/mol) are abstracted preferentially by Br•: the weaker bond both makes that step more exothermic (or less endothermic) and — via Evans–Polanyi — lowers its barrier, reinforcing the selectivity already predicted by the Hammond postulate.

Where this leads