# Chemiluminescence in Hydro-Carbon Flames — CH* and OH* ## Overview Chemiluminescence in flames arises when chemical reactions produce **excited radicals** that emit photons as they relax. The two most important species for combustion diagnostics are: - CH* (≈ 431 nm, blue) - OH* (≈ 310 nm, UV) These are not just “present radicals” — they are **selectively excited products of specific reactions**, and their relative intensity encodes combustion chemistry. --- ## Key Reactions ### CH* Formation (fuel breakdown zone) CH* is associated with hydrocarbon fragmentation and early flame chemistry. Typical pathways: $$ \mathrm{C_2H + O \rightarrow CH^* + CO} $$ $$ \mathrm{CH_2 + O \rightarrow CH^* + OH} $$ $$ \mathrm{C + H_2 \rightarrow CH^* + H} $$ These reactions dominate in **fuel-rich or near-front regions** of the flame. --- ### OH* Formation (oxidation zone) OH* is associated with high-temperature oxidation chemistry. Typical pathways: $$ \mathrm{H + O_2 \rightarrow OH^* + O} $$ $$ \mathrm{O + H \rightarrow OH^*} $$ $$ \mathrm{H_2 + O \rightarrow OH^* + H} $$ These reactions dominate in **lean or well-oxidised regions**. --- ## Why Excited States Are Produced A chemical reaction releases energy: $$ \mathrm{A + B \rightarrow C + D + energy} $$ This energy can be distributed into: - Translational motion (heat) - Vibrational energy - Rotational energy - **Electronic excitation** If enough energy is deposited into the electronic degree of freedom: $$ \mathrm{OH^* \rightarrow OH + h\nu} $$ $$ \mathrm{CH^* \rightarrow CH + h\nu} $$ The emitted photon is what we detect. --- ## Non-Equilibrium Nature These reactions occur under: - High temperature - Fast radical–radical collisions - Non-equilibrium conditions Therefore: > Products are often formed **directly in excited states**, rather than being thermally excited. --- ## Why Only Certain Species Emit Strongly Not all reactions produce visible/UV light. Strong chemiluminescence requires: - Sufficient reaction energy (~2–5 eV) - Good overlap between reaction geometry and excited state (Franck–Condon principle) - Fast radiative decay CH* and OH* satisfy these conditions. --- ## Energy Scale Typical photon energies: $$ E = h\nu $$ CH* emission (~431 nm): $$ E \approx 2.9 \text{ eV} $$ OH* emission (~310 nm): $$ E \approx 4.0 \text{ eV} $$ --- ## Spatial Structure of the Flame - CH* peaks in the **reaction front** (fuel breakdown) - OH* peaks slightly downstream in the **oxidation zone** Thus, they probe different regions of the flame. --- ## The OH*/CH* Ratio Define: $$ R = \frac{OH^*}{CH^*} $$ This ratio reflects: $$ R \propto \frac{\text{oxidation rate}}{\text{fuel fragmentation rate}} $$ --- ### Interpretation - Fuel-rich: - High CH* - Lower OH* - $$R \text{ small}$$ - Lean: - High OH* - Lower CH* - $$R \text{ large}$$ - Stoichiometric: - Balanced - $$R \text{ intermediate}$$ --- ## Why the Ratio is Useful Absolute intensity depends on: - Optical alignment - Flame size - Window fouling - Sensor gain But the ratio: $$ \frac{OH^*}{CH^*} $$ cancels many of these effects and provides a **robust indicator of combustion state**. --- ## Physical Interpretation - CH* → “fuel is still breaking apart” - OH* → “oxidation is occurring” So: > The ratio indicates where the flame sits between **fuel-dominated** and **oxidation-dominated** chemistry. --- ## Deeper Insight Even though both species arise from excited states: - CH* is fed by **hydrocarbon radical pathways** - OH* is fed by **oxidation pathways** Thus the ratio is not just energy-related — it reflects: > **Which chemical pathways dominate locally** --- ## Summary - Chemiluminescence arises from **excited radicals formed during reactions** - CH* and OH* originate from **different parts of the combustion network** - Their ratio provides a **real-time optical measure of stoichiometry and flame structure** ---