1. SPECTROSCOPY Light interacting with matter as an analytical tool

2. X-ray: core electron excitation UV: valance electronic excitation IR: molecular vibrations Radio waves: Nuclear spin states (in a magnetic field) Electronic Excitation by UV/Vis Spectroscopy :

3. Spectroscopic Techniques and Chemistry they Probe UV-visUV-vis regionbonding electrons Atomic AbsorptionUV-vis regionatomic transitions (val. e-) FT-IRIR/Microwavevibrations, rotations RamanIR/UVvibrations FT-NMRRadio wavesnuclear spin states X-Ray SpectroscopyX-raysinner electrons, elemental X-ray CrystallographyX-rays3-D structure

4. Spectroscopic Techniques and Common Uses UV-visUV-vis region Quantitative analysis/Beer’s Law Atomic AbsorptionUV-vis region Quantitative analysis Beer’s Law FT-IRIR/MicrowaveFunctional Group Analysis RamanIR/UV Functional Group Analysis/quant FT-NMRRadio wavesStructure determination X-Ray SpectroscopyX-raysElemental Analysis X-ray CrystallographyX-rays3-D structure Anaylysis

5. Different Spectroscopies UV-vis – electronic states of valence e/d- orbital transitions for solvated transition metals Fluorescence – emission of UV/vis by certain molecules FT-IR – vibrational transitions of molecules FT-NMR – nuclear spin transitions X-Ray Spectroscopy – electronic transitions of core electrons

6. Quantitative Spectroscopy Beer’s Law A l1 = e l1 bc e is molar absorptivity (unique for a given compound at l 1 ) b is path length c concentration

7. Beer’s Law A = -logT = log(P 0 /P) = ebc T = P solution /P solvent = P/P 0 Works for monochromatic light Compound x has a unique e at different wavelengths cuvette source slit detector

8. Characteristics of Beer’s Law Plots One wavelength Good plots have a range of absorbances from 0.010 to 1.000 Absorbances over 1.000 are not that valid and should be avoided 2 orders of magnitude

9. Standard Practice Prepare standards of known concentration Measure absorbance at max Plot A vs. concentration Obtain slope Use slope (and intercept) to determine the concentration of the analyte in the unknown

10. Typical Beer’s Law Plot

11. UV-Vis Spectroscopy UV- organic molecules –Outer electron bonding transitions –conjugation Visible – metal/ligands in solution –d-orbital transitions Instrumentation

12. Characteristics of UV-Vis spectra of Organic Molecules Absorb mostly in UV unless highly conjugated Spectra are broad, usually to broad for qualitative identification purposes Excellent for quantitative Beer’s Law- type analyses The most common detector for an HPLC

13. Molecules have quantized energy levels: ex. electronic energy levels. energy hv energy }  = hv Q: Where do these quantized energy levels come from? A: The electronic configurations associated with bonding. Each electronic energy level (configuration) has associated with it the many vibrational energy levels we examined with IR.

14. Broad spectra Overlapping vibrational and rotational peaks Solvent effects

15. Molecular Orbital Theory Fig 18-10

16. 2s       2p n

17. max = 135 nm (a high energy transition) Absorptions having max < 200 nm are difficult to observe because everything (including quartz glass and air) absorbs in this spectral region. Ethane

18. Example: ethylene absorbs at longer wavelengths: max = 165 nm  = 10,000  = hv =hc/

19. The n to pi* transition is at even lower wavelengths but is not as strong as pi to pi* transitions. It is said to be “forbidden.” Example: Acetone: n  max = 188 nm ;  = 1860 n  max = 279 nm ;  = 15

20.  135 nm  165 nm n  183 nmweak  150 nm n  188 nm n  279 nmweak A 180 nm 279 nm

21. Conjugated systems: Preferred transition is between Highest Occupied Molecular Orbital (HOMO) and Lowest Unoccupied Molecular Orbital (LUMO). Note: Additional conjugation (double bonds) lowers the HOMO- LUMO energy gap: Example: 1,3 butadiene: max = 217 nm ;  = 21,000 1,3,5-hexatriene max = 258 nm ;  = 35,000

22. Similar structures have similar UV spectra: max = 238, 305 nm max = 240, 311 nm max = 173, 192 nm

23. max = 114 + 5(8) + 11*(48.0-1.7*11) = 476 nm max (Actual) = 474.

24. Metal ion transitions Degenerate D-orbitals of naked Co D-orbitals of hydrated Co 2+ Octahedral Configuration EE

25. Co 2+ H2OH2O H2OH2O H2OH2O H2OH2O H2OH2O H2OH2O Octahedral Geometry

26. Instrumentation Fixed wavelength instruments Scanning instruments Diode Array Instruments

27. Fixed Wavelength Instrument LED serve as source Pseudo-monochromatic light source No monochrometer necessary/ wavelength selection occurs by turning on the appropriate LED 4 LEDs to choose from photodyode sample beam of light LEDs

28. Scanning Instrument cuvette Tungsten Filament (vis) slit Photomultiplier tube monochromator Deuterium lamp Filament (UV) slit Scanning Instrument

29. sources Tungten lamp (350-2500 nm) Deuterium (200-400 nm) Xenon Arc lamps (200-1000 nm)

30. Monochromator Braggs law, nl = d(sin i + sin r) Angular dispersion, d r/ d = n / d(cos r) Resolution, R = /  nN, resolution is extended by concave mirrors to refocus the divergent beam at the exit slit

31. Sample holder Visible; can be plastic or glass UV; you must use quartz

32. Single beam vs. double beam Source flicker

33. Diode array Instrument cuvette Tungsten Filament (vis) slit Diode array detector 328 individual detectors monochromator Deuterium lamp Filament (UV) slit mirror

34. Advantages/disadvantages Scanning instrument –High spectral resolution (63000), /  –Long data acquisition time (several minutes) –Low throughput Diode array –Fast acquisition time (a couple of seconds), compatible with on-line separations –High throughput (no slits) –Low resolution (2 nm)

35. HPLC-UV Mobile phase HPLC Pump syringe 6-port valve Sample loop HPLC column UV detector Solvent waste