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Delocalized Electrons

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p bonds move depending on the structure. The p electrons are delocalized ... Scissoring. Rocking. Wagging. Twisting. http://en.wikipedia.org/wiki/Infrared_spectroscopy ... – PowerPoint PPT presentation

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Title: Delocalized Electrons


1
Delocalized Electrons
  • Resonance Structures
  • always s bonds between nuclei, local electrons
  • p bonds move depending on the structure
  • The p electrons are delocalized
  • Use LE model for s, MO model for p electrons
  • Benzene

2
Sigma Bonds Hybrid Orbitals, Localized Electrons
Pi Bonds Molecular Orbitals, Delocalized
Electrons
3
Spectroscopy
  • Quantized energy levels of any sort
  • EM radiation is applied to system
  • Frequencies absorbed correspond to difference
    between energy levels

4
Electronic Spectroscopy (UV-VIS)
  • Energy levels electrons in different levels
    (atomic orbitals, molecular orbitals)
  • The frequencies are in the UV or Visible region

5
Uses of UV-Vis
  • Kinetics following a reaction
  • Finding concentration, if you have a standard or
    know absorption coefficient
  • Proteins concentration (abs of tyrosine)

6
Vibrational Spectroscopy (IR)
  • Energy levels molecular vibrations
  • Molecular identification
  • Some peaks can tell specific bonds
  • Other regions act like a fingerprint

http//en.wikipedia.org/wiki/Infrared_spectroscopy
7
Vibrational Spectroscopy (IR)
8
Rotational Spectroscopy (Microwave)
  • Energy levels molecular rotations
  • Only works in gases, where rotations are well
    quantized.
  • In liquids, rotations are quenched by collisions.
  • Uses
  • Physical Chemistry structure of gases
  • Astrophysics Composition of interstellar medium

9
http//www.sciencedaily.com/releases/2008/09/08091
9075007.htm
10
Nuclear Magnetic Resonance (NMR)
  • Energy Levels Nuclear alignment with and against
    a strong magnetic field
  • Energy corresponds to radio frequency
  • Uses
  • Small molecule structure determination
  • Protein structure and binding information
  • Magnetic Resonance Imaging (MRI)

11
1D spectrum of Ethanol (CH3CH2OH)
2D Spectra can give structures of large molecules
12
MRI
  • This same information in a spatial manner gives
    images

13
Intermolecular Forces
  • Attractions between molecules
  • If IMF are low relative to KE, substance is a gas
  • If comparable to KE, liquid
  • If high relative to KE, solid
  • Higher IMF higher melting point and boiling
    point

14
Dispersion Forces
  • The default (and weakest) IMF
  • Caused by fluctuations in electron distribution
    within molecules

15
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16
Dispersion Forces
  • Strength increases with size of molecule
  • Ex Which has a higher boiling point
  • He or Ar
  • CH4 or C10H22
  • The default (and weakest) IMF
  • Caused by fluctuations in electron distribution
    within molecules

17
Dipole-Dipole Forces
  • For molecules with a net dipole moment (polar)
  • end of one molecule attracts end of another
  • Stronger than dispersion

18
Hydrogen Bonding
  • A super dipole-dipole force, strongest IMF
  • Polar molecules with HF HO or HN bond
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