Download presentation
1
Microwave Rotational Spectroscopy
CHE 6416 Michael Evans
2
How does Microwave relate to other spectroscopies
Different types of motion Translational Vibrational Rotational.
3
What is Microwave Spectroscopy?
Microwave stimulates Rotational translations Measures the rotational states of molecules Gas Phase Must have a dipole. Tjb – Fix bullets throughout, The use of photons in the Microwave region to cause measureable translations in the Quantum Rotational Levels of a gas phase molecule
4
Applications of MW Measurement of bond lengths
Observation by radio telescopes for life precursors in interstellar clouds Precise observation of translating stereochemistries and confirmation verification Tjb- fix bullets, needs to be earlier in talk
5
Microwave Spectroscopy
RADAR was impetus for its invention 1948, Walter Gordy, first published review Tjb- fix bullets Microwave Spectroscopy, Reviews of Modern Physics, Volume 20, Number 4, October 1948, Gordy, Walter. Gordy, W., Microwave Spectroscopy, Reviews of Modern Physics, Volume 20, Number 4, October 1948,
6
Microwaves
7
TJB this needs to be shown early
TJB this needs to be shown early!!! The theory and data makes more sense if shown earlier, references In the conventional Stark-modulated spectrometer, the sample is contained in a long (1- to 3-metre, or 3.3- to 9.8-foot) section of a rectangular waveguide, sealed at each end with a microwave transmitting window (e.g., mica or Mylar), and connected to a vacuum line for evacuation and sample introduction. The radiation from the source passes through a gaseous sample and is detected by a crystal diode detector that is followed by an amplifier and display system (chart recorder). In order to increase the sensitivity of the instrument, signal modulation by application of a high-voltage square wave across the sample is used. (Note the above is a cut and paste, there are some references to flight tubes up to 20M)
8
Rotational vs. Vibrational
Where J = rotational V= vibrational Observed from lowest vibration state 𝐸 𝐽 =𝐵 𝐽(𝐽+1) Where does e(j) come from?
9
Motion of Rotation 3 Possible moments of inertia 𝐼 𝑎 , 𝐼 𝑏 , 𝐼 𝑐
𝐼 𝑎 , 𝐼 𝑏 , 𝐼 𝑐 Graph…needs one.
10
Diatomic molecule Rotation E from Schrodinger. 𝐼 𝑎 = 𝐼 𝑏 , 𝐼 𝑐 =0
𝐼 𝑎 = 𝐼 𝑏 , 𝐼 𝑐 =0 𝐵= ℎ 8𝐼 𝑐𝜋 2 𝐼= 𝑅 2 𝑢= ( 𝑀 1 𝑀 2 ) ( 𝑀 1 + 𝑀 2 ) 𝑅 2 Line spacing is 2B.
11
Theory of Microwave Spectroscopy
Microwave wavelength photon Highest probability of transition Molecules with dipoles Tjb- fix bullets
12
How do we measure if it will translate?
Probability of Transition=∫ψrot(F)μ^ ψrot(I) dτ Where: ψrot(F) is the complex conjugate of the final rotational state ψrot(I) is the wave function of the initial rotational state μ is the dipole moment operator with X, y, z coordinates. The function is positive. Only tells if is allowed. might need graph of probability Per Dr Burkey, a comparison of the sin and antisine waves may be appropriate
13
But there are limits. Photons limited ΔJ±1 Only one transition per
Each photon has one unit of momentum ΔJ±1 Only one transition per
14
Is it available to translate?
Boltzmann distribution Where nJ=number of molecules excited n0=number of molecules in ground state R=gas constant T=temperature ErotJ=molar energy of the rotational state
15
Plot of Probability Probability of Population Similar to spectra
16
Types of Molecules that are MW-Active
Linear Tjb- line structure are ineffective - show structures here not later!!! Break up into two slides if needed, don’t make audience interpret line formula because they will be distracted and stop listening to you, get ChemDraw from the University if you don’t have it already.
17
Types of Molecules that are MW-Active
Symmetric Tops
18
Types of Molecules that are MW-Active
Antisymmetric tops
19
Types of Molecules that are MW-Active
Spherical tops-Not active
20
Linear Molecules. Linear molecules(Rigid rotors)
Bond length directly calculated 𝐼 𝑎 = 𝐼 𝑏 , 𝐼 𝑐 =0 𝐼= 𝑅 2 𝑢= ( 𝑀 1 𝑀 2 ) ( 𝑀 1 + 𝑀 2 ) 𝑅 2 Tjb- fix bullets
21
http:// en.wikipedia.org/wiki/Rotational_spectroscopy#Asymmetric_top
Linear Molecules. Linear molecules(Rigid rotors) ∆𝐽= 𝐽 ′ − 𝐽 ′′ =±1 𝑣 𝐽 ′ ↔ 𝐽 ′′ =𝐸 𝐽 ′ −𝐸 𝐽 ′′ =2𝐵 𝐽 " +1 Where 𝐽 ′′ =𝐿𝑜𝑤𝑒𝑟 𝑙𝑒𝑣𝑒𝑙 𝐽 ′ =𝑈𝑝𝑝𝑒𝑟 𝐿𝑒𝑣𝑒𝑙 en.wikipedia.org/wiki/Rotational_spectroscopy#Asymmetric_top
22
Symmetric Tops (Rotors)
Two rotational axes same, one different Oblate 𝐼 𝑎 ≠ 𝐼 𝑏 = 𝐼 𝑐 Oblate. Benzene, XeF4 Prolate 𝐼 𝑎 = 𝐼 𝑏 ≠ 𝐼 𝑐 Prolate. CH3Cl, NH3 Tjb- fix bullets
23
Symmetric Top Spectra On the Cl⋅⋅⋅N Halogen Bond: A Rotational Study of CF3Cl⋅⋅⋅NH3 Gang Feng, Dr. Luca Evangelisti, Nicola Gasparini and Prof. Dr. Walther Caminati* Chemistry - A European Journal Volume 18, Issue 5, pages 1364–1368, January 27, 2012 Fengm G., Evangelisti, L, Gaspartini, N., Caminati, W., On the Cl⋅⋅⋅N Halogen Bond: A Rotational Study of CF3Cl⋅⋅⋅NH3, Chemistry-A European Journal, Vol 18, #5 pg
24
Why more complicated? With more axis, more complicated
Symmetrical molecules gain 2 terms K = vector about the symmetry axis Must be between –J and +J M = rotational momentum about a external field Also between –J and +J 0 if no external field
25
Why more complicated? With more axis, more complicated
𝐸 𝐽, 𝐾 =𝐵𝐽 𝐽+1 + 𝐴−𝐵 𝐾 2 Where B= ℎ 8 𝜋 2 𝑐 𝐼 𝑏 A= ℎ 8 𝜋 2 𝑐 𝐼 𝑎 , Prolate A= ℎ 8 𝜋 2 𝑐 𝐼 𝑐 , Oblate
26
Why more complicated? Which leads to Lines at:
𝑣 𝐽 ′ ↔ 𝐽 ′′ , 𝐾 =𝐸 𝐽 ′ , 𝐾 −𝐸 𝐽 ′′ , 𝐾 =2𝐵 𝐽 " +1
27
Why more complicated? With more axis, more complicated Stark Effect
- Hyperfine splitting
28
Stark Effect Similar to Zeeman effect Lifts level degeneracy
Due to external electric field 1rst Order-Linear 2nd Order-Quadratic
29
Stark Effect 𝐸 𝑆𝑡𝑎𝑟𝑘 𝐽, 𝐾, 𝑀 =− 𝑢𝐸𝐾𝑀 𝐽(𝐽+1) M = 0, no stark
𝐸 𝑆𝑡𝑎𝑟𝑘 𝐽, 𝐾, 𝑀 =− 𝑢𝐸𝐾𝑀 𝐽(𝐽+1) M = 0, no stark K, M ≠0 splitting occurs -M inc, + M dec Post note, uE is the energy of the level, with K and M quantum numbers
30
Hyperfine Splitting Coupling of Nuclear spin and molecular rotation.
If J > l, 2l+1 levels If J < l, 2J+1 levels.
31
Hyperfine splitting CF3I, Splitting due to 127I
32
Asymmetrical Tops Three different axes, 3 different inertias
Most molecules. Very complex spectra.
33
Effect of Isotope Substitution
12C16O13C16O, mass ↑, B ↓ (~1/I), E ↓.
34
Isotope splitting c-C3HD
35
Isotopic Substitution
As Isotopic Mass ↑, Energy ↓ Example (CO) 12CO J=0->J=1 @ cm-1 13CO @ cm-1 Tjb- fix bullets
36
Instrumentation Most homemade. Two types spectrometers.
Stark Modulated Fortier Transform Microwave Spectroscopy Similar in concept to FTIR Tjb- fix bullets
37
Stark Modulated MW Spectrometer
Samples introduced as a gas. Can be heated. Generally high vacuum.
38
TJB this needs to be shown early
TJB this needs to be shown early!!! The theory and data makes more sense if shown earlier, references In the conventional Stark-modulated spectrometer, the sample is contained in a long (1- to 3-metre, or 3.3- to 9.8-foot) section of a rectangular waveguide, sealed at each end with a microwave transmitting window (e.g., mica or Mylar), and connected to a vacuum line for evacuation and sample introduction. The radiation from the source passes through a gaseous sample and is detected by a crystal diode detector that is followed by an amplifier and display system (chart recorder). In order to increase the sensitivity of the instrument, signal modulation by application of a high-voltage square wave across the sample is used.
39
FTMW Spectrometer Similar in principle to FTIR
Broader Frequency, Greater Precision
40
Chipped Pulse FTMW Add waveform generators
Widens Bandwidth several 1000x Decreases spectral search time Tjb- fix bullets
41
Chipped Pulse FTMW This is not needed, spend more time on spectra and interpretation
42
FTMW Spectrometer Typical setup
43
Sample Preparation/Introduction
Gas samples As is As a diluted analyte in a non-MW reactive gas such as Neon Solids Laser abatement Vaporization Liquids Supersonic Expansion
44
Supersonic Expansion/Laser Ablatement
I don’t think this is important for your audience,
45
Applications of MW Measurement of bond lengths
Observation by radio telescopes for life precursors in interstellar clouds Precise observation of translating stereochemistries and confirmation verification
46
Measuring Bond Length. For example, we will use the easiest case, a diatomic molecule, HCL. cm-1 J->J+1 R(nm) 83.03 3-4 .1288 103.73 4-5 124.3 5-6 .1289 145.03 6-7 165.51 7-8 .1290 185.86 8-9 .1291 206.38 9-10 .1292 226.5 10-11 .1293
47
Calculation example (HCL)
𝐵= ℎ 8𝐼 𝑐𝜋 2 R= ℎ 8 𝜋 2 𝑐𝐵𝑢 R= 6.626𝑒−34 𝐽.𝑆 8 (3.14) 2 ( 𝑒10 𝑐𝑚.𝑠)( ∗1.661𝑥10−27 𝑘𝑔)(10.3 𝑐𝑚−1) R=1.29x10-10 M or nm
48
Problem Calculate bond length for CO Given= 2B = 3.8626 cm-1
h = x J.S c = x 1010 cm.s Amu to kg = 1.661x kg
49
Calculation example (CO)
𝐵= ℎ 8𝐼 𝑐𝜋 2 R= ℎ 8 𝜋 2 𝑐𝐵𝑢 R= 6.626𝑒−34 𝐽.𝑆 8 (3.14) 2 ( 𝑒10 𝑐𝑚.𝑠)( 48 7 )∗1.661𝑥10−27 𝑘𝑔)( 𝑐𝑚−1) R=1.13x10-10 M or nm Reference value is nm for CO
50
Identification of Organics in Interstellar Space
Gas phase molecules and radicals Observed using a radio telescope. Linear molecule Simple spectra
51
Identification of Organics in Interstellar Space
Symmetric Molecule Complicated due to symmetric top Many more possible states
52
Glycine? in interstellar clouds
Other more complicated molecules may be observed Data too complicated
53
Molecular Confirmation
Resolve rapidly interchanging conformers. 17000 scans/52 hrs. 27 yrs on standard unit. B C Dian et al, Science, 2008, 320, 924 (DOI: /science B C Dian et al, Science, 2008, 320, 924 (DOI: /science
54
Conformers Cyclopropane carboxaldehyde
55
Conclusion Useful for Gas Molecules Can determine bond length.
Diverse usages for the technique. Tjb- fix bullets, never ever write out sentences like this, Ughh!!!
Similar presentations
© 2024 SlidePlayer.com Inc.
All rights reserved.