Photochemistry Basics: Jablonski Diagram Explained

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Photochem Basics
Transitions & Laws
Jablonski Diagram
Decay Processes
Timescales & Recap

Photochem Basics

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    Defines photochemical reactions as light-induced processes, detailing the essential criteria for molecules to absorb UV or visible radiation.

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    Explains electronic transitions between molecular orbitals, focusing on the lower-energy pi to pi* and n to pi* excitations relevant to organic systems.

Basic molecular orbital theory, including the concepts of HOMO, LUMO, and electronic spin states (singlet vs. triplet states).
The quantum nature of light and electromagnetic radiation, specifically photon absorption as described by Planck's equation (E = hν).
Fundamental principles of quantum mechanics, particularly quantized energy levels in atoms and molecules.
Basic chemical kinetics and thermodynamics, including activation energy and energy reaction coordinate diagrams.
In-depth mechanisms, lifetimes, and quantum yields of radiative decay processes (fluorescence and phosphorescence).
Analysis of non-radiative deactivation pathways, such as internal conversion, vibrational relaxation, and intersystem crossing (ISC).
Intermolecular energy transfer and quenching mechanisms, including Förster Resonance Energy Transfer (FRET) and Stern-Volmer kinetics.
Applied photochemistry fields, such as photovoltaics (solar energy conversion), photocatalysis, photosynthesis, and photodynamic therapy.
355 views5likes22:57@letmeteachyouchemistryOriginal Release: 2024-10-02

Photochemical reactions are chemical processes induced by electromagnetic radiation (UV or visible light), where molecules absorb light energy causing electrons to transition from ground to excited states. The Jablonski diagram illustrates these electronic states: singlet states (S₀, S₁, S₂) with paired electrons and triplet states (T₁) with parallel spins. Key processes include internal conversion (non-radiative relaxation between vibrational levels), vibrational relaxation, intersystem crossing (spin-flip transition between singlet and triplet states), fluorescence (radiative S₁→S₀ emission, 10⁻⁹-10⁻⁶ s), and phosphorescence (radiative T₁→S₀ emission, 10⁻³-10⁰ s). The essential criteria for photochemical reactions are: (1) the molecule must absorb light, and (2) the radiation energy must match the energy difference between ground and excited states.