Photo Chemistry Hand Written Notes Pdf

PHYSICAL • ORGANIC PHOTOCHEMISTRY

CSIR NET & GATE Photochemistry Handwritten Notes in PDF

Accelerate your competitive exam preparation with comprehensive classroom handwritten notes. Covers Jablonski diagram, fluorescence vs. phosphorescence, Stern-Volmer quenching kinetics, Norrish Type I & II reactions, and Paterno-Büchi photocycloadditions.

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100% Syllabus Coverage • High-Resolution Scanned PDF (~3 MB) • Solved PYQs
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📚 1. Document Specifications & Syllabus Weightage

In CSIR NET Chemical Science and GATE (CY), Photochemistry spans both physical and organic chemistry, contributing 12 to 18 marks across Part B and Part C. Questions test both numerical calculation (quantum yield, fluorescence lifetime, Stern-Volmer constant) and mechanistic prediction (biradical intermediates, stereochemical outcomes).

Module NamePhotochemistry Complete Classroom Notes (Organic + Physical)
Target ExaminationsCSIR UGC NET (JRF/LS), GATE Chemistry (CY), BARC, TIFR, SET
File Size & Quality~3 MB • High-contrast scanned PDF (Optimal readability on screen & print)
Authors / SourceCurated from Premier Coaching Class Notes & NET Toppers
Access Cost100% Free Direct Google Drive Download

🔬 2. Physical Photochemistry: Photophysical Pathways

A. Fundamental Laws of Photochemistry
  • Grotthuss-Draper Law: Only the radiation absorbed by a chemical system is effective in bringing about a photochemical transformation.
  • Stark-Einstein Law of Photochemical Equivalence: Each molecule taking part in a primary photochemical reaction absorbs exactly one quantum (photon) of light.
  • Lambert-Beer Law: Absorbance A = log10(I0 / I) = ε · c · l, where ε is the molar absorption coefficient.
B. Jablonski Diagram: Radiative vs. Non-Radiative Transitions
Transition NameProcess TypeSpin Multiplicity ChangeTypical Timescale (τ)Emission of Light
Internal Conversion (IC)Non-RadiativeIso-multiplicity (Sn → Sn−1)10−12 to 10−11 sNo (Heat dissipated to solvent)
Intersystem Crossing (ISC)Non-RadiativeSpin-Forbidden (S1 → T1)10−10 to 10−8 sNo (Enhanced by heavy-atom effect)
Fluorescence (F)Radiative EmissionSpin-Allowed (S1 → S0 + hνF)10−9 to 10−7 sYes (Fast emission, stops when light stops)
Phosphorescence (P)Radiative EmissionSpin-Forbidden (T1 → S0 + hνP)10−3 to several secondsYes (Delayed emission, persists after light stops)
Kasha’s Rule: Photochemical emission (fluorescence or phosphorescence) occurs with appreciable yield only from the lowest excited state of a given multiplicity (S1 or T1).
Stokes Shift: Fluorescence emission wavelength is consistently longer than absorption wavelength (λemission > λabsorption) due to rapid vibrational relaxation in S1.

⚡ 3. Stern-Volmer Quenching Kinetics & Quantum Yield

A. Quantum Yield (Φ) Definition
Quantum Yield (Φ) = (Number of molecules reacting in a given time) / (Number of photons absorbed in the same time)
• Chain reactions (e.g., H2 + Cl2): Φ ≈ 104 – 106 (Very high)
• Non-chain reactions with deactivation: Φ ≤ 1
B. The Stern-Volmer Equation

In the presence of a quencher [Q], fluorescence intensity decreases according to the Stern-Volmer relation:

I0 / I = Φ0 / Φ = 1 + KSV [Q] = 1 + kq τ0 [Q]
Where:
KSV = Stern-Volmer quenching constant (Slope of I0/I vs. [Q] plot)
kq = Bimolecular quenching rate constant (L mol−1 s−1)
τ0 = Natural fluorescence lifetime in the absence of quencher

🧪 4. Organic Photochemistry: High-Frequency Reactions

1. Norrish Type I (α-Cleavage)

Photochemical homolytic cleavage of the bond between the carbonyl carbon and the α-carbon, generating an acyl-alkyl biradical pair. Favored in strained cyclic ketones (cyclobutanone, cyclopentanone) and in the vapor phase, leading to decarbonylation (−CO).

2. Norrish Type II (γ-H Abstraction)

Carbonyl compounds containing a γ-hydrogen undergo intramolecular hydrogen abstraction through a 6-membered cyclic transition state, generating a 1,4-biradical. Leads to either fragmentation (alkene + enol) or cyclization to cyclobutanols (Yang reaction).

3. Paterno-Büchi Reaction

Photochemical [2 + 2] cycloaddition between an excited carbonyl compound and an alkene to form an oxetane ring. Singlet excited state adds stereospecifically, while triplet excited state forms a long-lived biradical yielding thermodynamically stable regioisomers.

4. Di-π-Methane Rearrangement

Molecules containing two π-systems separated by an sp3 hybridized carbon (1,4-dienes or β,γ-unsaturated ketones) undergo photochemical isomerization to produce vinylcyclopropanes or cyclopropyl ketones.

💡 5. Solved CSIR NET & GATE Practice Problems

CSIR NET Chemical Science • Physical Photochemistry

Problem 1: The fluorescence lifetime of a fluorophore in the absence of quencher is τ0 = 10 ns. In the presence of 0.02 M quencher [Q], the fluorescence intensity drops by 50% (i.e., I0 / I = 2). Calculate the bimolecular quenching rate constant (kq).

Step-by-Step Solution:

  • Apply the Stern-Volmer relation: I0 / I = 1 + kq τ0 [Q].
  • Substitute the given values:
    2 = 1 + kq × (10 × 10−9 s) × (0.02 mol L−1)
    1 = kq × (2 × 10−10 mol s L−1)
  • Solve for kq:
    kq = 1 / (2 × 10−10) = 5.0 × 109 L mol−1 s−1.
  • Conclusion: Since kq ≈ 1010 L mol−1 s−1, the process is diffusion-controlled dynamic quenching.
CSIR NET Chemical Science • Organic Photochemistry

Problem 2: Predict the major photoproducts when 2-hexanone [CH3COCH2CH2CH2CH3] is irradiated with UV light (λ = 313 nm).

Step-by-Step Mechanism:

  • 2-Hexanone possesses γ-hydrogens on the butyl chain: CH3−C(=O)−CH2(α)−CH2(β)−CH2(γ)−CH3.
  • Upon photoexcitation, the carbonyl oxygen in the (n, π*) state abstracts a γ-hydrogen via a 6-membered cyclic chair-like transition state, producing a 1,4-biradical.
  • Path A (Fragmentation): The α,β-bond cleaves, yielding propene (CH3CH=CH2) and an enol [CH2=C(OH)CH3], which tautomerizes rapidly to acetone (CH3COCH3). This is the dominant Norrish Type II process.
  • Path B (Cyclization): Radical recombination forms 1-methyl-2-propylcyclobutanol (Yang cyclization product).

🖼️ 6. Handwritten Notes Page Preview

Below is a sample preview from the high-resolution scanned PDF notes:

CSIR NET Photochemistry Handwritten Notes PDF Preview
Figure 1: High-contrast sample page from Photochemistry classroom handwritten notes (~3 MB).

❓ 7. Frequently Asked Questions (FAQs)

Q1: Why is phosphorescence emission slower and longer-lived than fluorescence?

Fluorescence is a spin-allowed transition (S1 → S0, ΔS = 0) with a very short lifetime (τ ≈ 10−9 s). Phosphorescence is a spin-forbidden transition (T1 → S0, ΔS ≠ 0), requiring an electron spin flip, which significantly lowers the transition probability and results in a long lifetime (τ ≈ 10−3 s to minutes).

Q2: How does temperature affect dynamic vs. static quenching?

In dynamic (collisional) quenching, increasing temperature increases diffusion rates and collision frequency, thereby increasing KSV. In static quenching (ground-state complex formation), increasing temperature dissociates the complex, thereby decreasing KSV.

Q3: Are these notes sufficient for both CSIR NET and GATE Chemistry?

Yes. These notes thoroughly cover both Physical Photochemistry (quantum yields, actinometry, decay kinetics) and Organic Photochemistry (rearrangements, photocycloadditions, biradical mechanisms), perfectly aligning with CSIR NET Part B & C and GATE CY syllabus requirements.

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