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Organic Photochemistry Introduction to Photochemistry Classifications of Photochemical Reactions Application of Photochemistry in Organic Synthesis
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Page 1: Photochemistry

Organic Photochemistry

Introduction to PhotochemistryClassifications of Photochemical ReactionsApplication of Photochemistry in Organic Synthesis

Page 2: Photochemistry
Page 3: Photochemistry

Energies100 kcal/mol= 4.3 eV= 286 nm= 35000 /cm (near UV)nano= 10-9286 kcal/mol= 12.4 eV= 100 nm= 100000 /cm (far UV)Typical Bond Energies

C-H = 110 kcal/molC-C = 80C=C = 150C=O = 170Uv light 150 -40 nm wavelength, so this is sufficient energy to break bonds –knock electrons out of bonding orbitals (electronic excitation).

Page 4: Photochemistry
Page 5: Photochemistry

Chemically useful light is generally in the range of 200-400 nm

Often employ filters to regulate the wavelength of the radiation

n

*

n

*

n

*

n

*

n

*

ground state (S0) n-* (S1) n-* (T1) -* (S1) -* (T1)

Page 6: Photochemistry

A Jablonski diagram, named after the Polish physicist AleksanderJabłoński, is a diagram that illustrates the electronic states of a molecule and the transitions between them. The states are arranged vertically by energy and grouped horizontally by spin multiplicity. Radiative transitions are indicated by straight arrows and nonradiative transitions by squiggly arrows.The vibrational ground states of each electronic state are indicated with thick lines, the higher rotational states with thinner lines.

Page 7: Photochemistry
Page 8: Photochemistry

Physical Processes Undergone by Excited Molecules

• So + hv --- S1 Excitation

• S1v -- S1 + heat Vibrational Relaxation

• S1 ----- So + hv Fluorescence

• S1 ---- So + heat Internal Conversion

• S1 --- T1 Intersystem Crossing

• T1v -- T1 + heat Vibrational Relaxation

• T1v -- So + hv Phosphorescence

• T1 --- So + heat Intersystem Crossing

• S1 + A (So) --- So + A (S1) Singlet-Singlet Energy Transfer

• T1 + A (So) -- So + A (T1) Triplet-Triplet Energy Transfer

Page 9: Photochemistry

Why Use Photochemistry

• Overcome large kinetic barriers in a short amount of time• Produce immense molecular complexity in a single step• Form thermodynamically disfavored products• Allows reactivity that would otherwise be inaccessible by almost

any other synthetic method• The reagent (light) is cheap, easily accessible, and renewable

• Drawback• Reactivity is often unpredictable• Many substrates are not compatible• Selectivity and conversion are sometimes low

Page 10: Photochemistry

Chemical Processes undergone by Excited Molecules

(A-B-C) A-B. + C. Simple Cleavage

(A-B-C) E + F Decomposition

(A-B-C) A-C-B Intramolecular Rearrangement

(A-B-C) A-B-C' Photoisomerization

(A-B-C) A-B-C-H + R. Hydrogen Atom AbstractionRH

(A-B-C) (ABC)2 Photodimerization

(A-B-C) ABC + A* PhotosensitizationA

Page 11: Photochemistry

• 1) α-Cleavage (Norrish type I reaction). In solution the radicals undergo further reactions to give products.

Page 12: Photochemistry

• 2) Hydrogen Abstraction followed by cleavage = Norrishtype II cleavage.The radicals can abstract a Hydrogen atom from a donor. The resulting radicals can then undergo further reactions.

Page 13: Photochemistry

• An intramolecular example:

Page 14: Photochemistry
Page 15: Photochemistry
Page 16: Photochemistry
Page 17: Photochemistry

O

R1

R2

R2 R2R1

R1O

OR1

R2+

h, (300 nm)

solvent

1a–f

3f 4f2a–f

a b c d

R1

R2 CO2EtH

CO2Me

CO2Me

Ph H Ph

Ph

CO2EtH

HH

e f

+

Page 18: Photochemistry

O

R1 R2

R2

R2 R1

O

O

R2

25a–f

28a–f

1a–f

3a–f

17a–f

20a–f

22a–f

DPMODPM

R1O

O

R2

R1

R1

R2

R1

O

5

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