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Ultraviolet-Visible (uv-vis) Spectroscopy

Basics
Ultraviolet-visible spectropscopy (uv = 200-400 nm, visible = 400-800 nm) corresponds to electronic excitations between the energy levels that correspond to the molecular orbitals of the systems.  In particular, transitions involving π orbitals and lone pairs (n = non-bonding) are important and so uv-vis spectroscopy is of most use for identifying conjugated systems which tend to have stronger absorptions.
The lowest energy transition is that between the highest occupied molecular orbital (HOMO) and the lowest unoccupied molecular orbital (LUMO) in the ground state.  The absorption of the EM radiation excites an electron to the LUMO and creates an excited state. The more highly conjugated the system, the smaller the HOMO-LUMO gap, DE, and therefore the lower the frequency and longer the wavelength, l.  The colours we see in inks, dyes, flowers etc. are typically due to highly conjugated organic molecules. The unit of the molecule that is responsible for the absorption is called the chromophore, of which the most common are C=C (π to π*) and C=O (n to π*) systems. The basis of electronic excitation in uv-vis spectroscopy
The following table contains some data for polyenes and demonstrates how the wavelength of the absorbance increases as the conjugated system becomes more extended.
 
H(CH=CH)nH
  λmax / nm 
    εmax 
1
170
15,000
2
217
21,000
3
258
35,000

Terminology
 

Absorbance A, a measure of the amount of radiation that is absorbed
Band Term to describe a uv-vis absorption which are typically broad.
Chromophore Structural unit responsible for the absorption.
Molar absorptivity ε, absorbance of a sample of molar concentration in 1 cm cell.
Extinction coefficicent An alternative term for the molar absorptivity.
Path length l, the length of the sample cell in cm.
Beer-Lambert Law A = ε.c.l    (c = concentration in moles / litre)
λmax The wavelength at maximum absorbance
εmax The molar absorbance at λmax
HOMO Highest Occupied Molecular Orbital
LUMO Lowest Unoccupied Molecular Orbital


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organic chemistry © Dr. Ian Hunt, Department of Chemistry University of Calgary