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Interaction of radiation & matter
 Electromagnetic
radiation in
different regions of
spectrum can be
used for qualitative
and quantitative
information
 Different types of
chemical
information
Energy transfer from photon to
molecule or atom
At room temperature most molecules
are at lowest electronic & vibrational
state
IR radiation can excite vibrational levels that
then lose energy quickly in collisions with
surroundings
UV Visible Spectrometry
absorption - specific energy
emission - excited molecule
emits
fluorescence
phosphorescence
What happens to molecule after
excitation
collisions deactivate
vibrational levels (heat)
emission of photon
(fluorescence)
intersystem crossover
(phosphorescence)
General optical spectrometer
Wavelength
separation
Photodetectors
Light source - hot
objects produce “black
body radiation
Black body radiation
 Tungsten lamp, Globar, Nernst glower
 Intensity and peak emission wavelength are
a function of Temperature
 As T increases the total intensity increases
and there is shift to higher energies (toward
visible and UV)
Temp
(K)
 max.
int.
Rel. int
1000 3000 nm 0.0003
2000 1600 nm 0.01
3000 1100 nm 0.1
4000 700 nm 0.4
UV sources
 Arc discharge lamps with electrical
discharge maintained in appropriate gases
 Low pressure hydrogen and deuterium
lamps
 Lasers - narrow spectral widths, very high
intensity, spatial beam, time resolution,
problem with range of wavelengths
 Discrete spectroscopic- metal vapor &
hollow cathode lamps
Why separate wavelengths?
Each compound absorbs different
colors (energies) with different
probabilities (absorbtivity)
Selectivity
Quantitative adherence to Beer’s
Law A = abc
Improves sensitivity
Why are UV-Vis bands broad?
Electronic energy states give band
with no vibrational structure
Solvent interactions
(microenvironments) averaged
Low temperature gas phase
molecules give structure if
instrumental resolution is adequate
Wavelength Dispersion
 prisms (nonlinear, range
depends on refractive
index)
 gratings (linear, Bragg’s
Law, depends on spacing
of scratches, overlapping
orders interfere)
 interference filters
(inexpensive)
Monochromator
Entrance slit - provides narrow
optical image
Collimator - makes light hit
dispersive element at same angle
Dispersing element - directional
Focusing element - image on slit
Exit slit - isolates desired color to
exit
Resolution
 The ability to distinguish different
wavelengths of light - R=/D
 Linear dispersion - range of wavelengths
spread over unit distance at exit slit
 Spectral bandwidth - range of wavelengths
included in output of exit slit (FWHM)
 Resolution depends on how widely light is
dispersed & how narrow a slice chosen
Filters - inexpensive alternative
 Adsorption type - glass with dyes to
adsorb chosen colors
 Interference filters - multiple
reflections between 2 parallel reflective
surfaces - only certain wavelengths
have positive interferences -
temperature effects spacing between
surfaces
Wavelength dependence in
spectrometer
Source
Monochromator
Detector
Sample - We hope so!
Photodetectors - photoelectric
effect E(e)=hn - w
 For sensitive detector we need a small
work function - alkali metals are best
 Phototube - electrons attracted to
anode giving a current flow
proportional to light intensity
 Photomultiplier - amplification to
improve sensitivity (10 million)
Spectral sensitivity is a function
of photocathode material
 Ag-O-Cs mixture
gives broader range
but less efficiency
 Na2KSb(trace of
Cs)has better response
over narrow range
 Max. response is 10%
of one per photon
(quantum efficiency)
300nm 500 700 900
Na2KSb
AgOCs
Photomultiplier - dynodes of
CuO.BeO.Cs or GaP.Cs
Cooled Photomultiplier
Tube
Dynode array
Photodiodes - semiconductor that
conducts in one direction only
when light is present
Rugged and small
Photodiode arrays - allows
observation of a number of
different locations (wavelengths)
simultaneously
Somewhat less sensitive than PMT
T=I/Io
A= - log T = -log (I/Io)
Calibration curve
One million photons impinge on
a sample in a UV-vis
spectrometer and
800,000 of the photons pass
through to the detector, the
remaining photons
having been absorbed.
How many photons will pass
through the sample if
the concentration is doubled?
Beer’s Law •
• A=
A=abc
abc
•
• A=
A=absorbance
absorbance
•
• a=
a=absorbtivity
absorbtivity
(depends on species
(depends on species
and wavelength)
and wavelength)
•
• b=
b=pathlength
pathlength in
in
sample
sample
•
• c=concentration of
c=concentration of
absorbing species
absorbing species
Deviations from Beer’s Law
High concentrations (0.01M)
distort each molecules electronic
structure & spectra
Chemical equilibrium
Stray light
Polychromatic light
Interferences
Interpretation - quantitative
Broad adsorption bands -
considerable overlap
Specral dependence upon solvents
Resolving mixtures as linear
combinations - need to measure as
many wavelengths as components
Beer’s Law .html
Resolving mixtures
 Measure at different wavelengths and
solve mathematically
 Use standard additions (measure A and
then add known amounts of standard)
 Chemical methods to separate or shift
spectrum
 Use time resolution (fluorescence and
phosphorescence)
Improving resolution in mixtures
 Instrumental (resolution)
 Mathematical (derivatives)
 Use second parameter (fluorescence)
 Use third parameter (time for
phosphorescence)
 Chemical separations
(chromatography)
Fluorescence
 Emission at lower energy than
absorption
 Greater selectivity but fluorescent
yields vary for different molecules
 Detection at right angles to excitation
 S/N is improved so sensitivity is better
 Fluorescent tags
Spectrofluorometer
Light source
Monochromator to select excitation
Sample compartment
Monochromator to
select fluorescence
Photoacoustic spectroscopy
Edison’s observations
If light is pulsed then as gas is
excited it can expand (sound)
Principles of IR
 Absorption of energy at various frequencies
is detected by IR
 plots the amount of radiation transmitted
through the sample as a function of
frequency
 compounds have “fingerprint” region of
identity
Infrared Spectrometry
 Is especially useful for qualitative analysis
 functional groups
 other structural features
 establishing purity
 monitoring rates
 measuring concentrations
 theoretical studies
How does it work?
 Continuous beam of radiation
 Frequencies display different absorbances
 Beam comes to focus at entrance slit
 molecule absorbs radiation of the energy to
excite it to the vibrational state
How Does It Work?
 Monochromator disperses radiation into
spectrum
 one frequency appears at exit slit
 radiation passed to detector
 detector converts energy to signal
 signal amplified and recorded
Instrumentation II
 Optical-null double-beam instruments
 Radiation is directed through both cells by
mirrors
 sample beam and reference beam
 chopper
 diffraction grating
Double beam/ null detection
Instrumentation III
 Exit slit
 detector
 servo motor
 Resulting spectrum is a plot of the intensity
of the transmitted radiation versus the
wavelength
Detection of IR radiation
 Insufficient energy to excite
electrons & hence photodetectors
won’t work
 Sense heat - not very sensitive and
must be protected from sources of heat
 Thermocouple - dissimilar metals
characterized by voltage across gap
proportional to temperature
IR detectors
 Golay detector - gas expanded by heat
causes flexible mirror to move - measure
photocurrent of visible light source
Detector
IR beam Vis
source
GAS
Flexible mirror
Carbon analyzer - simple IR
Sample flushed of carbon
dioxide (inorganic)
Organic carbon oxidized by
persulfate & UV
Carbon dioxide measured in gas
cell (water interferences)
IR Source
IR Source IR Source
IR Source
Chopper
SAMP
REF
Detector cell
Filter
CO2 CO2
Beam trimmer
Press. sens. det.
NDIR detector - no
monochromator
Limitations
Mechanical coupling
Slow scanning / detectors slow
Limitations of Dispersive IR
 Mechanically complex
 Sensitivity limited
 Requires external
calibration
 Tracking errors limit
resolution (scanning fast
broadens peak,
decreases absorbance,
shifts peak
Problems with IR
 c no quantitative
 H limited resolution
 D not reproducible
 A limited dynamic range
 I limited sensitivity
 E long analysis time
 B functional groups
Limitations
 Most equipment can
measure one
wavelength at a time
 Potentially time-
consuming
 A solution?
Fourier-Transform Infrared
Spectroscopy (FTIR)
A Solution!
FTIR
 Analyze all wavelengths simultaneously
 signal decoded to generate complete
spectrum
 can be done quickly
 better resolution
 more resolution
 However, . . .
FTIR
 A solution, yet an
expensive one!
 FTIR uses
sophisticated
machinery more
complex than generic
GCIR
Fourier Transform IR
 Mechanically
simple
 Fast, sensitive,
accurate
 Internal
calibration
 No tracking
errors or stray
light
IR Spectroscopy - qualitative
Double beam required to correct
for blank at each wavelength
Scan time (sensitivity)
Vs resolution
Michelson
interferometer & FTIR
Advantages of FTIR
 Multiplex--speed, sensitivity (Felgett)
 Throughput--greater energy, S/N
(Jacquinot)
 Laser reference--accurate wavelength,
reproducible (Connes)
 No stray light--quantitative accuracy
 No tracking errors--wavelength and
photometric accuracy
New FTIR Applications
Quality control--speed, accuracy
Micro, trace analysis--nanogram
levels, small samples
Kinetic studies--milliseconds
Internal reflection
Telescopic
Attenuated Internal Reflection
 Surface analysis
 Limited by 75%
energy loss
New FTIR Applications
Quality control--speed, accuracy
Micro, trace analysis--nanogram
levels, small samples
Kinetic studies--milliseconds
Internal reflection
Telescopic
62700523-Uv-Ir-Spectroscopy.ppt
62700523-Uv-Ir-Spectroscopy.ppt

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62700523-Uv-Ir-Spectroscopy.ppt

  • 1. Interaction of radiation & matter  Electromagnetic radiation in different regions of spectrum can be used for qualitative and quantitative information  Different types of chemical information
  • 2. Energy transfer from photon to molecule or atom At room temperature most molecules are at lowest electronic & vibrational state IR radiation can excite vibrational levels that then lose energy quickly in collisions with surroundings
  • 3. UV Visible Spectrometry absorption - specific energy emission - excited molecule emits fluorescence phosphorescence
  • 4. What happens to molecule after excitation collisions deactivate vibrational levels (heat) emission of photon (fluorescence) intersystem crossover (phosphorescence)
  • 5. General optical spectrometer Wavelength separation Photodetectors Light source - hot objects produce “black body radiation
  • 6. Black body radiation  Tungsten lamp, Globar, Nernst glower  Intensity and peak emission wavelength are a function of Temperature  As T increases the total intensity increases and there is shift to higher energies (toward visible and UV) Temp (K)  max. int. Rel. int 1000 3000 nm 0.0003 2000 1600 nm 0.01 3000 1100 nm 0.1 4000 700 nm 0.4
  • 7. UV sources  Arc discharge lamps with electrical discharge maintained in appropriate gases  Low pressure hydrogen and deuterium lamps  Lasers - narrow spectral widths, very high intensity, spatial beam, time resolution, problem with range of wavelengths  Discrete spectroscopic- metal vapor & hollow cathode lamps
  • 8. Why separate wavelengths? Each compound absorbs different colors (energies) with different probabilities (absorbtivity) Selectivity Quantitative adherence to Beer’s Law A = abc Improves sensitivity
  • 9. Why are UV-Vis bands broad? Electronic energy states give band with no vibrational structure Solvent interactions (microenvironments) averaged Low temperature gas phase molecules give structure if instrumental resolution is adequate
  • 10. Wavelength Dispersion  prisms (nonlinear, range depends on refractive index)  gratings (linear, Bragg’s Law, depends on spacing of scratches, overlapping orders interfere)  interference filters (inexpensive)
  • 11. Monochromator Entrance slit - provides narrow optical image Collimator - makes light hit dispersive element at same angle Dispersing element - directional Focusing element - image on slit Exit slit - isolates desired color to exit
  • 12. Resolution  The ability to distinguish different wavelengths of light - R=/D  Linear dispersion - range of wavelengths spread over unit distance at exit slit  Spectral bandwidth - range of wavelengths included in output of exit slit (FWHM)  Resolution depends on how widely light is dispersed & how narrow a slice chosen
  • 13. Filters - inexpensive alternative  Adsorption type - glass with dyes to adsorb chosen colors  Interference filters - multiple reflections between 2 parallel reflective surfaces - only certain wavelengths have positive interferences - temperature effects spacing between surfaces
  • 15. Photodetectors - photoelectric effect E(e)=hn - w  For sensitive detector we need a small work function - alkali metals are best  Phototube - electrons attracted to anode giving a current flow proportional to light intensity  Photomultiplier - amplification to improve sensitivity (10 million)
  • 16. Spectral sensitivity is a function of photocathode material  Ag-O-Cs mixture gives broader range but less efficiency  Na2KSb(trace of Cs)has better response over narrow range  Max. response is 10% of one per photon (quantum efficiency) 300nm 500 700 900 Na2KSb AgOCs
  • 17. Photomultiplier - dynodes of CuO.BeO.Cs or GaP.Cs
  • 20. Photodiodes - semiconductor that conducts in one direction only when light is present Rugged and small Photodiode arrays - allows observation of a number of different locations (wavelengths) simultaneously Somewhat less sensitive than PMT
  • 21.
  • 22. T=I/Io A= - log T = -log (I/Io) Calibration curve
  • 23. One million photons impinge on a sample in a UV-vis spectrometer and 800,000 of the photons pass through to the detector, the remaining photons having been absorbed. How many photons will pass through the sample if the concentration is doubled? Beer’s Law • • A= A=abc abc • • A= A=absorbance absorbance • • a= a=absorbtivity absorbtivity (depends on species (depends on species and wavelength) and wavelength) • • b= b=pathlength pathlength in in sample sample • • c=concentration of c=concentration of absorbing species absorbing species
  • 24. Deviations from Beer’s Law High concentrations (0.01M) distort each molecules electronic structure & spectra Chemical equilibrium Stray light Polychromatic light Interferences
  • 25. Interpretation - quantitative Broad adsorption bands - considerable overlap Specral dependence upon solvents Resolving mixtures as linear combinations - need to measure as many wavelengths as components Beer’s Law .html
  • 26. Resolving mixtures  Measure at different wavelengths and solve mathematically  Use standard additions (measure A and then add known amounts of standard)  Chemical methods to separate or shift spectrum  Use time resolution (fluorescence and phosphorescence)
  • 27. Improving resolution in mixtures  Instrumental (resolution)  Mathematical (derivatives)  Use second parameter (fluorescence)  Use third parameter (time for phosphorescence)  Chemical separations (chromatography)
  • 28. Fluorescence  Emission at lower energy than absorption  Greater selectivity but fluorescent yields vary for different molecules  Detection at right angles to excitation  S/N is improved so sensitivity is better  Fluorescent tags
  • 29. Spectrofluorometer Light source Monochromator to select excitation Sample compartment Monochromator to select fluorescence
  • 30. Photoacoustic spectroscopy Edison’s observations If light is pulsed then as gas is excited it can expand (sound)
  • 31.
  • 32. Principles of IR  Absorption of energy at various frequencies is detected by IR  plots the amount of radiation transmitted through the sample as a function of frequency  compounds have “fingerprint” region of identity
  • 33. Infrared Spectrometry  Is especially useful for qualitative analysis  functional groups  other structural features  establishing purity  monitoring rates  measuring concentrations  theoretical studies
  • 34. How does it work?  Continuous beam of radiation  Frequencies display different absorbances  Beam comes to focus at entrance slit  molecule absorbs radiation of the energy to excite it to the vibrational state
  • 35. How Does It Work?  Monochromator disperses radiation into spectrum  one frequency appears at exit slit  radiation passed to detector  detector converts energy to signal  signal amplified and recorded
  • 36. Instrumentation II  Optical-null double-beam instruments  Radiation is directed through both cells by mirrors  sample beam and reference beam  chopper  diffraction grating
  • 37. Double beam/ null detection
  • 38. Instrumentation III  Exit slit  detector  servo motor  Resulting spectrum is a plot of the intensity of the transmitted radiation versus the wavelength
  • 39. Detection of IR radiation  Insufficient energy to excite electrons & hence photodetectors won’t work  Sense heat - not very sensitive and must be protected from sources of heat  Thermocouple - dissimilar metals characterized by voltage across gap proportional to temperature
  • 40. IR detectors  Golay detector - gas expanded by heat causes flexible mirror to move - measure photocurrent of visible light source Detector IR beam Vis source GAS Flexible mirror
  • 41. Carbon analyzer - simple IR Sample flushed of carbon dioxide (inorganic) Organic carbon oxidized by persulfate & UV Carbon dioxide measured in gas cell (water interferences)
  • 42. IR Source IR Source IR Source IR Source Chopper SAMP REF Detector cell Filter CO2 CO2 Beam trimmer Press. sens. det. NDIR detector - no monochromator
  • 44. Limitations of Dispersive IR  Mechanically complex  Sensitivity limited  Requires external calibration  Tracking errors limit resolution (scanning fast broadens peak, decreases absorbance, shifts peak
  • 45. Problems with IR  c no quantitative  H limited resolution  D not reproducible  A limited dynamic range  I limited sensitivity  E long analysis time  B functional groups
  • 46. Limitations  Most equipment can measure one wavelength at a time  Potentially time- consuming  A solution?
  • 48. FTIR  Analyze all wavelengths simultaneously  signal decoded to generate complete spectrum  can be done quickly  better resolution  more resolution  However, . . .
  • 49. FTIR  A solution, yet an expensive one!  FTIR uses sophisticated machinery more complex than generic GCIR
  • 50. Fourier Transform IR  Mechanically simple  Fast, sensitive, accurate  Internal calibration  No tracking errors or stray light
  • 51. IR Spectroscopy - qualitative Double beam required to correct for blank at each wavelength Scan time (sensitivity) Vs resolution Michelson interferometer & FTIR
  • 52. Advantages of FTIR  Multiplex--speed, sensitivity (Felgett)  Throughput--greater energy, S/N (Jacquinot)  Laser reference--accurate wavelength, reproducible (Connes)  No stray light--quantitative accuracy  No tracking errors--wavelength and photometric accuracy
  • 53. New FTIR Applications Quality control--speed, accuracy Micro, trace analysis--nanogram levels, small samples Kinetic studies--milliseconds Internal reflection Telescopic
  • 54. Attenuated Internal Reflection  Surface analysis  Limited by 75% energy loss
  • 55. New FTIR Applications Quality control--speed, accuracy Micro, trace analysis--nanogram levels, small samples Kinetic studies--milliseconds Internal reflection Telescopic