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Optical Electronic Spectroscopy 2
Lecture Date: January 28th, 2008
Molecular UV-Visible Spectroscopy
Molecular UV-Visible spectroscopy can:
– Enable structural analysis
– Detect molecular chromophore
– Analyze light-absorbing properties (e.g. for photochemistry)
Figures from http://www.cem.msu.edu/~reusch/VirtualText/Spectrpy/UV-Vis/uvspec.htm#uv1
Basic UV-Vis spectrophotometers acquire data in the 190-800 nm range and can be designed as “flow” systems.
Molecular UV-Visible spectroscopy is driven by electronic absorption of UV-Vis radiation.
Molecular UV-Vis Spectroscopy: Terminology
UV-Vis Terminology
– Chromophore: a UV-Visible absorbing functional group
– Bathochromic shift (red shift): to longer wavelengths
– Auxochrome: a substituent on a chromophore that causes a red shift
– Hypsochromic shift (blue shift): to shorter wavelengths
– Hyperchromic shift: to greater absorbance
– Hypochromic shift: to lesser absorbance
Molecular UV-Vis Spectroscopy: Transitions
Classes of Electron transitions
– HOMO: highest occupied molecular orbital
– LUMO: lowest unoccupied molecular orbital
– Types of electron transitions:
(1) , and n electrons (mostly organics)
(2) d and f electrons (inorganics/organometallics)
(3) charge-transfer (CT) electrons
Molecular UV-Vis Spectroscopy: Theory Molecular energy levels and absorbance wavelength:
* and * transitions: high-energy, accessible in vacuum UV (max <150 nm). Not usually observed in molecular UV-Vis.
n * and * transitions: non-bonding electrons (lone pairs), wavelength (max) in the 150-250 nm region.
n * and * transitions: most common transitions observed in organic molecular UV-Vis, observed in compounds with lone pairs and multiple bonds with max = 200-600 nm.
Figure from http://www.cem.msu.edu/~reusch/VirtualText/Spectrpy/UV-Vis/spectrum.htm
Molecular UV-Vis Spectroscopy: Theory
d/f orbitals – transition metal complexes – UV-Vis spectra of lanthanides/actinides are particularly sharp, due
to screening of the 4f and 5f orbitals by lower shells.
– Can measure ligand field strength, and transitions between d-orbitals made non-equivalent by the formation of a complex
Charge transfer (CT) – occurs when electron-donor and electron-acceptor properties are in the same complex – electron transfer occurs as an “excitation step”
– MLCT (metal-to-ligand charge transfer)
– LMCT (ligand-to-metal charge transfer)
– Ex: tri(bipyridyl)iron(II), which is red – an electron is exicted from the d-orbital of the metal into a * orbital on the ligand
Molecular UV-Vis Spectroscopy: Absorption
max is the wavelength(s) of maximum absorption (i.e. the peak position)
The strength of a UV-Visible absorption is given by the molar absorptivity ():
= 8.7 x 1019 P a
where P is the transition probability (0 to 1) – governed by selection rules and orbital overlap,
and a is the chromophore area in cm2
Again, the Beer-Lambert Law:
A = bc
Molecular UV-Vis Spectroscopy: Quantum Theory UV-Visible spectra and the states involved in electronic transitions
can be calculated with theories ranging from Huckel to ab initio/DFT.
Example: * transitions responsible for ethylene UV absorption at ~170 nm calculated with ZINDO semi-empirical excited-states methods (Gaussian 03W):
HOMO u bonding molecular orbital LUMO g antibonding molecular orbital
Molecular UV-Visible Spectrophotometers
Continuum UV-Vis sources – the 2H lamp:
Tungsten lamps used for longer wavelengths.
The traditional UV-Vis design – double-beam grating systems
Figure from http://www.cem.msu.edu/~reusch/VirtualText/Spectrpy/UV-Vis/uvspec.htm#uv1
Hamamatsu L2D2 lamps
Molecular UV-Visible Spectrophotometers
Diode array detectors can acquire all UV-Visible wavelengths at once.
Advantages:– Sensitivity
(multiplex)
– Speed
Disadvantages:– Resolution
Figure from Skoog, et al., Chapter 13
Interpretation of Molecular UV-Visible Spectra
UV-Visible spectra can be interpreted to help determine molecular structure, but this is presently confined to the analysis of electron behavior in known compounds.
Information from other techniques (NMR, MS, IR) is usually far more useful for structural analysis
However, UV-Vis evidence should not be ignored!
Figure from Skoog, et al., Chapter 14
Calculation of Molar Absorption Coefficient
The molar absorption coefficient for each absorbance in a UV spectrum is calculated as follows:
– Molar Abs Coeff (AU mol-1 cm-1) = A x mwt / mass x pathlength
Solvent “cutoffs” for UV-visible work:
Solvent UV Cutoff (nm)
Acetonitrile (UV grade) 190
Acetone 330
Dimethylsulfoxide 268
Chloroform (1% ethanol) 245
Heptane 200
Hexane (UV grade) 195
Methanol 205
2-Propanol 205
Tetrahydrofuran (UV grade) 212
Water 190
Burdick and Jackson High Purity Solvent Guide, 1990
Interpretation of UV-Visible Spectra
Although UV-Visible spectra are no longer frequently used for structural analysis, it is helpful to be aware of well-developed interpretive rules.
Examples: – Woodward-Fieser rules for max dienes and polyenes
– Extended Woodward rules for a,b-unsaturated ketones
– Substituted benzenes (max base value = 203.5 nm)
See E. Pretsch, et al., Structure Determination of Organic Compounds, Springer, 2000. (Chapter 8).
XSubstituent (X) Increment (nm)
-CH3 3.0
-Cl 6.0
-OH 7.0
-NH2 26.5
-CHO 46.0
-NO2 65.0
Interpretation of UV-Visible Spectra
Other examples:– The conjugation of a lone pair on a
enamine shifts the max from 190 nm (isolated alkene) to 230 nm. The nitrogen has an auxochromic effect.
See E. Pretsch, et al., Structure Determination of Organic Compounds, Springer, 2000. (Chapter 8).Figures from http://www.cem.msu.edu/~reusch/VirtualText/Spectrpy/UV-Vis/spectrum.htm
Why does increasing conjugation cause bathochromic shifts (to longer wavelengths)?
CH2 HC CH2vs.
~230 nm ~180 nm
H2N H3C
Interpretation of UV-Visible Spectra
Transition metal complexes
Lanthanide complexes – sharp lines caused by “screening” of the f electrons by other orbitals
See Shriver et al. Inorganic Chemistry, 2nd Ed. Ch. 14
More Complex Electronic Processes
Fluorescence: absorption of radiation to an excited state, followed by emission of radiation to a lower state of the same multiplicity
Phosphorescence: absorption of radiation to an excited state, followed by emission of radiation to a lower state of different multiplicity
Singlet state: spins are paired, no net angular momentum (and no net magnetic field)
Triplet state: spins are unpaired, net angular momentum (and net magnetic field)
Molecular Fluorescence
Non-resonance fluorescence is a phenomenon in which absorption of light of a given wavelength by a fluorescent molecule is followed by the emission of light at longer wavelengths (applies to molecules)
Why use fluorescence? Its not a difference method!
Method Mass detection limit (moles)
Concentration detection limit
(M)
Advantage
UV-Vis 10-13 to 10-16 10-5 to 10-8 Universal
fluorescence 10-15 to 10-17 10-7 to 10-9 Sensitive
Molecular Fluorescence: Terminology
Notation: S2, S1 = singlet states, T1 = triplet state
Excitation directly to a triplet state is forbidden by selection rules.
See Skoog Figure 15-1
Jablonski energy diagram:
Molecular Fluorescence: Terminology
Quantum yield (): the ratio of molecules that luminescence to the total # of molecules
Resonance fluorescence: fluorescence in which the emitted radiation has the same wavelength as the excitation radiation
Intersystem crossing: a transition in which the spin of the electron is reversed (change in multiplicity in molecule occurs, singlet to triplet).
– Enhanced if vibrational levels overlap or if molecule contains heavy atoms (halogens), or if paramagnetic species (O2) are present.
Dissociation: excitation to vibrational state with sufficient energy to break a chemical bond
Pre-dissociation: relaxation to vibrational state with sufficient energy to break a chemical bond
Stokes shift: a shift (usually seen in fluorescence) to longer wavelengths between excitation and emitted radiation
Predicting the Fluorescence of Molecules
Some things that improve fluorescence:– Low energy * transitions
– Rigid molecules
– Transitions that don’t have competition! Example: fluorescence does not often occur after absorption of UV wavelengths (< 250 nm) because the radiation has too much energy (>100 kcal/mol) – dissociation occurs instead (but see MPE!!!)
– Chelation to metals
Intersystem crossings reduce fluorescence (competing process is phosphorescence).
biphenylfluorescence QE = 0.2
fluorenefluorescence QE = 1.0
Predicting the Fluorescence of Molecules
More things that affect fluoroescence:– decrease temperature = increase fluorescence
– increase viscosity = increase fluorescence
– pH dependence for acid/base compounds (titrations)
Time-resolved fluorescence spectroscopy– Study of fluorescence spectra as a function of time (ps to ns)
Fluorescence probes for microscopy: will be covered in the Surface Analysis and Microscopy lectures (in conjunction with e.g. confocal scanning microscopy)
Applications of Fluorescence
Applications in forensics: trace level analysis of specific small molecules
Example: LSD (lysergic acid diethylamide) spectrum obtained with a Fourier-transform instrument and a microscope, but with no derivitization
M. Fisher, V. Bulatov, I. Schechter, “Fast analysis of narcotic drugs by optical chemical imaging”, Journal of Luminescence 102–103 (2003) 194–200
Applications of Fluorescence Applications in biochemistry:
analysis of proteins, enyzmes, anything that can be tagged with a fluorophore
In some cases, an externally-introduced label can be avoided.
In proteins, the stryptophan (Trp), tyrosine (Tyr), and phenylalanine (Phe) residues are naturally UV-fluorescent
– Example: single -galactosidase molecules from Escherichia coli (Ec Gal)
– 1-photon excitation at 266 nm
Q. Li and S. Seeger, “Label-Free Detection of Single Protein Molecules Using Deep UV Fluorescence Lifetime Microscopy”. Anal. Chem. 2006, 78, 2732-2737
Another Application of Fluorescence: FRAP
Fluorescence Recovery After Photo-bleaching (FRAP), developed in 1974, is a technique for measuring motion and diffusion.
– FRAP can be applied at a microscopic level.
– FRAP is commonly applied to microscopically heterogeneous systems.
A high power laser first bleaches an area of the sample, after which the recovery of fluorescence is monitored with the low power laser.
– Recent studies have used a single laser that is attenuated with a Pockel’s cell.
Applications of FRAP have included:– Biological systems
– Diffusion in polymers
– Solvation in adsorbed layers on chromatographic surfaces
– Curing of epoxy resins
J. M. Kovaleski and M. J. Wirth, Anal. Chem. 69, 600A (1997).
Fluorescence Recovery After Photo-bleaching
Spot photobleaching:– A spot is bleached, and its subsequent recovery is predicted by:
J. M. Kovaleski and M. J. Wirth, Anal. Chem. 69, 600A (1997).D. E. Koppel, D. Axelrod, J. Schlessinger, E. Elson, and W. W. Webb, Biophys. J. 16, 1315 (1976).
1 2
2
4/
D 1/2 is the time for the fluorescence to recover 1/2 of its intensity
is the diameter of the spot
– D is the diffusion coefficient depends on the initial amount of fluorophor bleached
Periodic pattern photobleaching– Eliminates dependence
– Currently the most flexible and accurate FRAP measurement method
Fluorophores: organic fluorescent molecules that are excited by the laser
– Example: rhodopsin
D
d2
2
2/1 4
Fluorescence Recovery After Photo-bleaching
J. M. Kovaleski and M. J. Wirth, Anal. Chem. 69, 600A (1997).B. A. Smith and H. M. McConnell, Proc. Natl. Acad. Sci. USA. 75, 2759 (1978).
A periodic pattern is first photobleached with a high power laser
The recovery of the fluorescence is monitored via a low power laser
Fluorescence Recovery After Photo-bleaching
J. M. Kovaleski and M. J. Wirth, Anal. Chem. 69, 600A (1997).B. A. Smith and H. M. McConnell, Proc. Natl. Acad. Sci. USA. 75, 2759 (1978).
Diffusion coefficients can be calculated from periodic pattern experiments via:
is the time constant of the simple exponential fluorescence recovery
– d is the spacing of the lines of the grid
– D is the diffusion coefficient
Methods of generating the periodic pattern:– Ronchi ruling
– Holographic imaging
d
D
2
24
Multiphoton-Excited Fluorescence
Known as MPE (as opposed to the usual 1PE)
Lots of energy required – femtosecond pulsed lasers
Multiple low energy photons can be absorbed, via short-lived “virtual states” (lifetime ~ 1 fs). Can get to far-UV wavelengths without “waste”
Spatial localization is excellent (because of the high energy needed, it can be confined to < 1 m3.)
Applications: primarily bioanalytical
J. B. Shear, “Multiphoton Excited Fluoroescence in Bioanalytical Chemistry”, Anal. Chem., 71, 598A-605A (1999).
groundstate
excitedstate
virtualstate
Molecular Phosphorescence
Phosphorescence – often used as a complementary technique to fluorescence.
– If a molecule won’t fluorescence, sometimes it will phosphoresce
– Phosphorescence is generally longer wavelength that fluorescence
Some phosphorimeters are “pulsed-source”, which allows for time-resolution of excited states (which have lifetimes covering a few orders of magnitude).
– Pulsed sources also help avoid the interference of Rayleigh scattering or fluorescence.
Instrumentation similar to fluorescence, but with cooling dewars and acquisition delays
wavelength
excitation fluorescence phosphorescence
Note that the wavelength difference between F and P can be used to measure the energy difference between singlet and triplet states
Phosphorescence Studies
Room-temperature Phosphorescence (RTP)– Phosphorescence is performed at low temperatures (77K) to avoid
“collisional deactivation” (molecules hitting each other), which causes quenching of phosphorescence signal
By absorbing molecules onto a substrate, and evaporating the solvent, the phosphorescence of the molecules can be studied without the need for low temperatures
By trapping molecules within micelles (and staying in solution), the same effect can be achieved
Applications: – nucleic acids, amino acids, enzymes, pesticides, petroleum products, and
many more
For more details, see: R. J. Hurtubise, Phosphorimetry: Theory, Instrumentation, and Applications, Chap. 3, New York, VCH 1990.
Chemi-luminescence
A chemical reaction that yields an electronically excited species that emits light as it returns to ground state.
In its simplest form:
A + B C* C + h
The radiant intensity (ICL) depends on the rate of the chemical reaction and the quantum yield:
ICL = CL (dC/dt) = EX EM (dC/dt)
excited states per molecule reacted
photons per excited states
Chemi-luminescence and Gas Analysis Gas analysis – see examples in Skoog pg. 375-376.
Example: Determination of nitrogen monoxide to 1 ppb levels (for pollution analysis in atmospheric gases):
Figure from: http://www.shu.ac.uk/schools/sci/chem/tutorials/molspec/lumin1.htm
nitric oxide+ O
O+
-O
ozone nitrogen dioxideO2+NO NO2*
NO2* NO2
hv
Chemi-luminescence: Luminol Reactions Luminol, a molecule that when oxidized can do many
things…
Representative uses of luminol:– Detecting hydrogen peroxide in seawater1 (indicator of
photoactivity)1
– Visualizing bloodstains – reaction catalyzed by haemoglobin2
– Detecting nitric oxide3
1. D. Price, P. J. Worsfold, and R. F. C. Mantoura, Anal. Chim. Acta, 1994, 298, 121.2. R. Saferstein, Criminalistics: An Introduction to Forensic Science, Prentice Hall, 1998.
3. J. K Robinson, M. J. Bollinger and J. W. Birks, Anal. Chem., 1999, 71, 5131.See also http://www.deakin.edu.au/~swlewis/2000_CL_demo.PDF
NH
NH
O
O
NH2
+oxidizing
agent
O
O
NH2
O-
O-
+ hv
Applications of Chemi-luminescence Detection of arsenic in water:
– Convert As(III) and As(V) to AsH3 via borohydride reduction
– pH < 1 converts both As(III) and As(V), pH 4-5 converts only As(III)
– Reacts with O3 (generated from air), CL results at 460 nm
– CL detected via photomultiplier tube down to 0.05 g/L for 3 mL
– Portable, automated analyzer, 6 min per analysis– See: A. D. Idowu et al., Anal. Chem., 2006, 78, 7088-7097.
Electrochemiluminescence: species formed at electrodes undergo electron-transfer reactions and produce light
– ECL converts electrical energy into radiation– See: M. M. Richter, Chem. Rev. 2004, 104, 3003-3036.
Chemi-luminescence can be applied to fabricated microarrays on a flow chip (biosensor applications)
– See: Cheek et al., Anal. Chem., 2001, 73, 5777.
Homework ProblemsOptical Electronic Spectroscopy
Chapter 13:
Problem 13-6Problem 13-13
Further Reading
Review Skoog et al. Chapters 13-15Review Cazes Chapters 5-6
UV-Visible SpectroscopyD. H. Williams and I. Fleming, “Spectroscopic Methods in
Organic Chemistry”, McGraw-Hill (1966).
Fluorescence, Phosphorescence, and Chemiluminescence Spectroscopy
K. A. Flectcher et al., Anal. Chem. 2006, 78, 4047-4068.