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Introduction to Infrared Spectrometry Chap 16. Quantum Mechanical Treatment of Vibrations Required to include quantized nature of E From solving the wave.

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Presentation on theme: "Introduction to Infrared Spectrometry Chap 16. Quantum Mechanical Treatment of Vibrations Required to include quantized nature of E From solving the wave."— Presentation transcript:

1 Introduction to Infrared Spectrometry Chap 16

2 Quantum Mechanical Treatment of Vibrations Required to include quantized nature of E From solving the wave equations of QM: Selection rule for vib. transitions

3 Quantum Mechanical Treatment of Vibrations Interatomic distance, r → hv res Plot of potential energy: where level spacings: All vib levels spaced equally for HO only

4 Anharmonic Oscillator (AHO) Problems with Harmonic Oscillator (HO) Model Real vib levels coalesce as v levels increase Real vib levels coalesce as v levels increase Does not allow for dissociation of bond Repulsion is steeper at small r Appears as if atoms can pass through each other during vibrational amplitude Solution:

5 Anharmonic Oscillator (AHO) Fig. 16-3

6 Anharmonic Oscillator (AHO) Three consequences: (1) Harmonic at low v levels (2) ΔE becomes smaller at high v levels (3) Selections rule fails: Δv = ±1 and ± 2... referred to as overtones

7 Vibrational Modes Approach: Each atom in a molecule can be located with three coordinates (degrees of freedom) A molecule with N atoms then has 3N DOF Translational motion defined by center-of- mass coordinates (COM)

8 Linear Molecules 3 DOF to define translation 2 DOF to define rotation 3N – 5 ≡ number of vibrational modes Nonlinear Molecules 3 DOF to define translation 3 DOF to define rotation 3N – 6 ≡ number of vibrational modes

9 Examples N2N2 CO 2 H2OH2O CH 3 -C(O)-CH 3

10 Vibrations of CO 2 No dipole changeDipole change } 667 cm -1 2350 cm -1 1388 cm -1 Fig 16-10 Doubly degenerate

11 Vibrations of H 2 O 1595 cm -1 3657 cm -1 3766 cm -1

12 IR Sources and Transducers Sources (1200 – 2200 K)

13 Spectral emission from a Nernst glower at ~ 2200 K Fig 16-16

14 IR Sources and Transducers Sources (1200 – 2200 K)

15 Transducers IR beam 10 -7 - 10 -9 W, ΔT at transducer mK-µK

16 IR Instrumentation Dispersive Grating IR Instruments: Fig 16-11

17 IR Instrumentation Dispersive Grating IR Instruments:   Similar to UV-Vis spectrophotometer   BUT sample after source and before monochromator in IR   Sample after monochromator in UV- Vis - less incident light   Grating 10-500 blazes per mm   Single beam and double beam (DB in time and space)   DB eliminates atmospheric gas interference

18 Fig. 16-9 Single- and Double-Beam Spectra of the Atmosphere

19 Fourier Transform IR Instruments: FTIR has largely displaced dispersive IRs A multiplex instrument (e.g., diode array) Beam is split and pathlength is varied to produce interference patterns Signal converted from frequency domain to time domain Fourier transform then converts “clean” signal back to frequency domain

20 Fourier Transform Instruments (Section 7-I) have two advantages: (1) (1) Throughput (or Jaquinot) advantage Few optics, no slits, high intensity Usually, to improve resolution, decrease slit width but less light makes spectrum "noisier" i.e., signal-to-noise ratio (S/N) decreases (p. 110-111):

21 S/N improves with more scans (noise is random, signal is not!) Fig. 5-10

22 (2) Multiplex (or Fellget) advantage Simultaneously measure entire spectrum Components of Fourier Transform Instruments Based on Michelson Interferometer frequencytime Converts frequency signal to time signal

23 Fig. 7-41 (p 207) Frequency domain Time domain

24 Fig. 7-42 (p 207) Time Domain Signal of a Source Made Up of Many Wavelengths

25 Frequencies of IR photons ~ 100 THz No detector can respond on 10 -14 s time scale Need to modulate high freq signal → lower freq without loss of P(t) relationships Interferometer: Splits beam equally in power Recombines them such that variations in power can be measured as P(δ) δ ≡ retardation, difference in pathlengths of the two beams

26 Single Frequency Source Michelson Interferometer Fig. 7-43 (p 208)

27 Computer needed to turn complex interferogram into spectrum: Single Frequency: Fig. 7-43 (p 188)

28 Two Frequencies: Many Frequencies:

29 High S/N ratios - high throughput Rapid (<10 s) Reproducible High resolution (<0.1 cm -1 ) Inexpensive (relatively!) Advantages to FT Instruments


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