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Electronic
Spectroscopy
Ultraviolet andUltraviolet and
visible
Beckman DU640 UV/Vis
Spectrophotometer
Scattering & Absorption
• When light impinges on solutions
and crystals two distinct processes
occur:occur:
1. Light scattering and
2. Light absorption
Based on these developed fundamental techniques for
characterization and analysis of molecules
Absorption & Fluorescence
• Absorption in UV regions is specially valuable
for molecular structure elucidation.
• In some molecules process of absorption is
followed by emission of light of a differentfollowed by emission of light of a different
wavelength called FLUORESCENCE.
• Fluorescence assists in characterization and
analysis of biologically significant molecules.
• Other techniques used: NMR (sec, ter structure)
and MS (mol. Wt.).
• Composed of a continuum of waves with
different properties.
• Several regions are of importance in
biochemical studies:
Electromagnetic Spectrum
biochemical studies:
1. X-ray- For x-ray crystallography up to 7nm.
2. Ultraviolet: 180-340nm.
3. Visible: 340-800nm.
4. InfraRed:1000 to 100000nm and
5. Radio waves: NMR 106 to 1010 nm.
• Ultraviolet: 190~400nm
• Violet: 400 - 420 nm• Violet: 400 - 420 nm
• Indigo: 420 - 440 nm
• Blue: 440 - 490 nm
• Green: 490 - 570 nm
• Yellow: 570 - 585 nm
• Orange: 585 - 620 nm
• Red: 620 - 780 nm
VISIBLE
Light wave or Particle?
Wavelength
λ=λ=λ=λ= C////ννννC νννν
As particle
Light also behaves as though it were
composed of energetic particles. The
amount of energy associated with these
particles or photons is given by
Where h is Plank’s constant
E=hνννν
Rayleigh Scattering
• Photon of specified energy interacts with a
molecule either
1. Gets scattered
2. Transfers energy producing excited state.
Rayleigh scattering occurs when a photon
collides with a molecule and is diffracted
or scattered with unchanged frequency.
• Used in techniques like x-ray diffraction,
Electron microscopy, laser/neutron
scattering etc.
Absorption
• Transfer of energy from a photon to a
molecule.
• Electrons promoted from ground state to
excited state.—electronic transition.excited state.—electronic transition.
• UV and visible energy sufficient for
electronic transition basis for
spectroscopy.
Electronic Spectroscopy
• Ultraviolet (UV) and visible (VIS)
spectroscopy.
• Earliest method of molecular
spectroscopy.spectroscopy.
• A phenomenon of interaction of
molecules with ultraviolet and
visible lights.
UV & VIS Spectroscopy
• In structure determination : UV-VIS
spectroscopy is used to detect the
presence of chromophores like
1. Dienes,
2. Aromatics,
3. Polyenes, and
4. Conjugated ketones, etc.
Terms: UV absorptions
1. Chromophores: functional groups that
cause electronic transitions.
2. Auxochromes: substituents with unshared pair
e's like OH, NH, SH ..., when attached to π-
chromophore they generally move the absorptionchromophore they generally move the absorption
max. to longer λ.
3. Bathochromic shift/ red shift. shift to longer λ.
4. Hysochromic shift/ blue shift.: shift to shorter λ.
5. Hyperchromism: increase in ε of a band.
6. Hypochromism: decrease in ε of a band.
Why should we learn?
Organic molecules have chromophores that
absorb UV.
UV absorbance is 1000 x easier to detect per
mole than NMR.mole than NMR.
Still used in following reactions where the
chromophore changes.
Useful because timescale is so fast, and
sensitivity so high.
Uses for UV
Knowing UV can help you know when to
be skeptical of quantitative results.
Assessing purity of a major peak in
HPLC. Sensitivity makes HPLC sensitive.HPLC. Sensitivity makes HPLC sensitive.
One of the best ways for identifying the
presence of acidic/basic groups, due to big
shifts in λ for a chromophore containing a
phenol, carboxylic acid, etc.
Instrumentation
Components
1. Light source
2. Monochromator
3. Sample Chamber3. Sample Chamber
4. Detector: Photo multiplier tube
5. Printers & Recorders : mostly
is a computer now a days.
1) Light Source
• Hydrogen/Deuterium Lamps-a truly
continuous spectrum in the ultraviolet
region is produced by electrical
excitation of deuterium at lowexcitation of deuterium at low
pressure. (160nm~375nm).
• Tungsten Filament Lamps-the most
common source of visible and near
infrared radiation (340nm~800nm)..
2) Monochromator
• Prism or Diffraction grating used.
• Used as a filter: the monochromator
will select a narrow portion of the
spectrum (the bandpass) of a given
sourcesource
• Used in analysis: the monochromator
will sequentially select for the
detector to record the different
components (spectrum) of any source
or sample emitting light.
Monochromator
Czerny-Turner design
Grating
3) Sample Chamber
Cuvette
Chamber varieties
Two types:
1. Single beam: hold one cuvette
2. Double beam: hold two: 1 for
reference (solvent) and one forreference (solvent) and one for
sample.
In double beam instruments the sample
spectrum is continuously corrected by
substraction of the reference spectrum
4) Detector: Photovoltaic
Detector
• Measures the intensity of photons by means
of the voltage developed across the
semiconductor layer.semiconductor layer.
• Electrons, ejected by photons from the
semiconductor, are collected by silver layer.
• The potential depends on the number of
photons hitting the detector.
Detector
Barrier Layer/Photovoltaic
Detector Phototube
Vacuum tube with
Cesium coated
photocathode.
Principle of Phototube
Detector
• This detector is a vacuum tube with a
cesium-coated photocathode.
• Photons of sufficiently high energy
hitting the cathode can dislodge electrons,
which are collected at the anode.
• Photon flux is measured by the current
flow in the system.
Detector Photomultiplier
Principle of
Photomultiplier Detector
• The detector consists of a photo-emissive
cathode coupled with a series of electron-
multiplying dynode stages, and usuallymultiplying dynode stages, and usually
called a photomultiplier.
• The primary electrons ejected from the
photo-cathode are accelerated by an
electric field so as to strike a small area
on the first dynode.
• The impinging electrons strike with
enough energy to eject 2-5 secondary
electrons, which are accelerated to the
Principle of
Photomultiplier Detector
electrons, which are accelerated to the
second dynode to eject still more electrons.
• A photomultiplier may have 9 to 16 stages,
and overall gain of 106~109 electrons per
incident photon.
5) Printers and recorders
Single and Double
Beam Spectrometer
• Single-Beam: There is only one light
beam or optical path from the source
through to the detector.through to the detector.
• Double-Beam: The light from the source,
after passing through the
monochromator, is split into two
separate beams-one for the sample and
the other for the reference.
Rotates, to achieve scan
Two photomultiplier inputs,
differential voltage drives amplifier.
Double beam in space configuration
Double beam in time configurationDouble beam in time configuration
Quantitative Analysis
Beer-Lambert Law
Quantitative measurements in spectrophotometry
are evaluated using this law. Absorbance
A = -log I/I = εεεεLCA = -log I/Io= εεεεLC
ε = molar absorptivity (L mol-1 cm-1)
L= Path length of the sample
C=Concentration of the compound in
solution, expressed in mol L-1
The visible absorbance
spectrum of haemoglobin
Limits to Beer’s Law
• Chemical Deviations
-absorbing undergo association,
dissociation or reaction with the
solventsolvent
• Instrumental Deviations
-non-monochromatic radiation
-stray light
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Uv spec

  • 3. Scattering & Absorption • When light impinges on solutions and crystals two distinct processes occur:occur: 1. Light scattering and 2. Light absorption Based on these developed fundamental techniques for characterization and analysis of molecules
  • 4. Absorption & Fluorescence • Absorption in UV regions is specially valuable for molecular structure elucidation. • In some molecules process of absorption is followed by emission of light of a differentfollowed by emission of light of a different wavelength called FLUORESCENCE. • Fluorescence assists in characterization and analysis of biologically significant molecules. • Other techniques used: NMR (sec, ter structure) and MS (mol. Wt.).
  • 5. • Composed of a continuum of waves with different properties. • Several regions are of importance in biochemical studies: Electromagnetic Spectrum biochemical studies: 1. X-ray- For x-ray crystallography up to 7nm. 2. Ultraviolet: 180-340nm. 3. Visible: 340-800nm. 4. InfraRed:1000 to 100000nm and 5. Radio waves: NMR 106 to 1010 nm.
  • 6.
  • 7. • Ultraviolet: 190~400nm • Violet: 400 - 420 nm• Violet: 400 - 420 nm • Indigo: 420 - 440 nm • Blue: 440 - 490 nm • Green: 490 - 570 nm • Yellow: 570 - 585 nm • Orange: 585 - 620 nm • Red: 620 - 780 nm VISIBLE
  • 8. Light wave or Particle? Wavelength λ=λ=λ=λ= C////ννννC νννν
  • 9. As particle Light also behaves as though it were composed of energetic particles. The amount of energy associated with these particles or photons is given by Where h is Plank’s constant E=hνννν
  • 10. Rayleigh Scattering • Photon of specified energy interacts with a molecule either 1. Gets scattered 2. Transfers energy producing excited state. Rayleigh scattering occurs when a photon collides with a molecule and is diffracted or scattered with unchanged frequency. • Used in techniques like x-ray diffraction, Electron microscopy, laser/neutron scattering etc.
  • 11. Absorption • Transfer of energy from a photon to a molecule. • Electrons promoted from ground state to excited state.—electronic transition.excited state.—electronic transition. • UV and visible energy sufficient for electronic transition basis for spectroscopy.
  • 12.
  • 13. Electronic Spectroscopy • Ultraviolet (UV) and visible (VIS) spectroscopy. • Earliest method of molecular spectroscopy.spectroscopy. • A phenomenon of interaction of molecules with ultraviolet and visible lights.
  • 14. UV & VIS Spectroscopy • In structure determination : UV-VIS spectroscopy is used to detect the presence of chromophores like 1. Dienes, 2. Aromatics, 3. Polyenes, and 4. Conjugated ketones, etc.
  • 15. Terms: UV absorptions 1. Chromophores: functional groups that cause electronic transitions. 2. Auxochromes: substituents with unshared pair e's like OH, NH, SH ..., when attached to π- chromophore they generally move the absorptionchromophore they generally move the absorption max. to longer λ. 3. Bathochromic shift/ red shift. shift to longer λ. 4. Hysochromic shift/ blue shift.: shift to shorter λ. 5. Hyperchromism: increase in ε of a band. 6. Hypochromism: decrease in ε of a band.
  • 16.
  • 17. Why should we learn? Organic molecules have chromophores that absorb UV. UV absorbance is 1000 x easier to detect per mole than NMR.mole than NMR. Still used in following reactions where the chromophore changes. Useful because timescale is so fast, and sensitivity so high.
  • 18. Uses for UV Knowing UV can help you know when to be skeptical of quantitative results. Assessing purity of a major peak in HPLC. Sensitivity makes HPLC sensitive.HPLC. Sensitivity makes HPLC sensitive. One of the best ways for identifying the presence of acidic/basic groups, due to big shifts in λ for a chromophore containing a phenol, carboxylic acid, etc.
  • 20. Components 1. Light source 2. Monochromator 3. Sample Chamber3. Sample Chamber 4. Detector: Photo multiplier tube 5. Printers & Recorders : mostly is a computer now a days.
  • 21. 1) Light Source • Hydrogen/Deuterium Lamps-a truly continuous spectrum in the ultraviolet region is produced by electrical excitation of deuterium at lowexcitation of deuterium at low pressure. (160nm~375nm). • Tungsten Filament Lamps-the most common source of visible and near infrared radiation (340nm~800nm)..
  • 22. 2) Monochromator • Prism or Diffraction grating used. • Used as a filter: the monochromator will select a narrow portion of the spectrum (the bandpass) of a given sourcesource • Used in analysis: the monochromator will sequentially select for the detector to record the different components (spectrum) of any source or sample emitting light.
  • 25.
  • 26.
  • 29. Chamber varieties Two types: 1. Single beam: hold one cuvette 2. Double beam: hold two: 1 for reference (solvent) and one forreference (solvent) and one for sample. In double beam instruments the sample spectrum is continuously corrected by substraction of the reference spectrum
  • 30. 4) Detector: Photovoltaic Detector • Measures the intensity of photons by means of the voltage developed across the semiconductor layer.semiconductor layer. • Electrons, ejected by photons from the semiconductor, are collected by silver layer. • The potential depends on the number of photons hitting the detector.
  • 32.
  • 33. Detector Phototube Vacuum tube with Cesium coated photocathode.
  • 34. Principle of Phototube Detector • This detector is a vacuum tube with a cesium-coated photocathode. • Photons of sufficiently high energy hitting the cathode can dislodge electrons, which are collected at the anode. • Photon flux is measured by the current flow in the system.
  • 36. Principle of Photomultiplier Detector • The detector consists of a photo-emissive cathode coupled with a series of electron- multiplying dynode stages, and usuallymultiplying dynode stages, and usually called a photomultiplier. • The primary electrons ejected from the photo-cathode are accelerated by an electric field so as to strike a small area on the first dynode.
  • 37. • The impinging electrons strike with enough energy to eject 2-5 secondary electrons, which are accelerated to the Principle of Photomultiplier Detector electrons, which are accelerated to the second dynode to eject still more electrons. • A photomultiplier may have 9 to 16 stages, and overall gain of 106~109 electrons per incident photon.
  • 38. 5) Printers and recorders
  • 39. Single and Double Beam Spectrometer • Single-Beam: There is only one light beam or optical path from the source through to the detector.through to the detector. • Double-Beam: The light from the source, after passing through the monochromator, is split into two separate beams-one for the sample and the other for the reference.
  • 40. Rotates, to achieve scan Two photomultiplier inputs, differential voltage drives amplifier.
  • 41. Double beam in space configuration Double beam in time configurationDouble beam in time configuration
  • 42. Quantitative Analysis Beer-Lambert Law Quantitative measurements in spectrophotometry are evaluated using this law. Absorbance A = -log I/I = εεεεLCA = -log I/Io= εεεεLC ε = molar absorptivity (L mol-1 cm-1) L= Path length of the sample C=Concentration of the compound in solution, expressed in mol L-1
  • 44.
  • 45. Limits to Beer’s Law • Chemical Deviations -absorbing undergo association, dissociation or reaction with the solventsolvent • Instrumental Deviations -non-monochromatic radiation -stray light