Q16Engineering Chemistry
Question
Q.6 Explain the various types of electronic transitions in UV-Vis spectroscopy.
Answer
In Ultraviolet-Visible (UV-Vis) spectroscopy, absorbing high-energy electromagnetic radiation physically causes valence electrons to systematically undergo four primary electronic transitions between distinct molecular orbitals: , , , and .
UV-Visible spectroscopy rigorously analyzes exactly how organic molecules physically absorb high-energy electromagnetic radiation strictly in the ultraviolet () and visible () regions. The absorption of this massive energy mathematically forces the excitation of loosely held valence electrons directly from their stable, low-energy Ground State molecular orbitals strictly up to unstable, high-energy Excited State (anti-bonding) molecular orbitals.
Types of Participating Molecular Orbitals
Before understanding the transitions, the three fundamental ground-state orbitals must be rigorously defined:
- Sigma () Bonding Orbitals: The extremely strong, tightly held electron pairs explicitly forming single covalent bonds (e.g., C-C, C-H).
- Pi () Bonding Orbitals: The relatively weaker, loosely held electron pairs explicitly forming the second and third bonds in double or triple unsaturated bonds (e.g., C=C, C=O).
- Non-bonding () Orbitals: Completely unshared, lone pairs of electrons physically residing exclusively on heteroatoms (e.g., Oxygen, Nitrogen, Halogens).
The Four Primary Electronic Transitions
- (Sigma to Sigma Star): This transition systematically requires the absolute highest amount of massive thermal energy because bonds are phenomenally stable. It mathematically absorbs strictly in the Far/Vacuum UV region (). Because atmospheric oxygen totally absorbs radiation in this region, standard UV spectrophotometers cannot detect it. Occurrence: Saturated alkanes like Methane ().
- (n to Sigma Star): Requires moderately high energy, typically absorbing strictly between and . Occurrence: Saturated compounds containing a heteroatom with unshared lone pairs, such as alcohols (e.g., Methanol, ) and alkyl halides.
- (Pi to Pi Star): Requires highly moderate energy, actively absorbing strongly directly in the standard near-UV region (). This specific transition mathematically possesses a very high molar absorptivity (strong intensity peak). Occurrence: All unsaturated organic compounds containing distinct double or triple bonds, specifically isolated or heavily conjugated alkenes, alkynes, and aromatic benzene rings.
- (n to Pi Star): Systematically requires the absolute lowest amount of transition energy, mathematically absorbing at the longest possible wavelengths (), frequently extending completely into the visible spectrum. However, quantum mechanical selection rules strictly label this transition as "forbidden," resulting in extremely weak intensity peaks. Occurrence: Unsaturated compounds containing a heteroatom with lone pairs directly bonded to a system, specifically Carbonyl groups (C=O), Nitro groups (-NO2), and Cyano groups (-CN).