Presentation on theme: "Atomic UV-Visible Spectroscopy"— Presentation transcript:
1 Atomic UV-Visible Spectroscopy Important note on lecture design: X-ray methods are also a form of “electronic” spectroscopy, but typically involve higher energies (inner electrons), and are outside the UV-visible region. As such they require somewhat different instrumentation. This lecture focuses on the types of electronic spectrometry that can be accomplished with optical components and radiation.Lecture Date: January 28th, 2013
2 Electronic Spectroscopy Spectroscopy involving energy level transitions of the electrons surrounding an atom or a moleculeAtoms: electrons are in hydrogen-like orbitals (s, p, d, f)Molecules: electrons are in molecular orbitals (HOMO, LUMO, …)From(The Bohr model for nitrogen)(The LUMO of benzene)
3 UV-Visible Spectroscopy Definition: Spectroscopy in the optical (UV-Visible) range involving electronic energy levels excited by electromagnetic radiation (often valence electrons).Techniques discussed in this lecture are related to the “high-energy” (“non-optical”) methods covered in the X-ray spectroscopy lecture.Methods discussed in this lecture:Atomic absorptionAtomic emissionLaser induced breakdown spectroscopyAtomic fluorescenceImportant note on lecture design: X-ray methods are also obviously a form of “electronic” spectroscopy, but typically involve higher energies (inner electrons), and are outside the UV-visible region. As such they require somewhat different instrumentation. This lecture focuses on the types of electronic spectroscopy that can be accomplished with optical components and radiation.
4 The Electromagnetic Spectrum The visible region of an optical electronic spectrum generally comprises photon energies of 36 to 72 kcal/mole. The near UV region (to 200 nm) extends this energy range to 143 kcal/mole.UV-Visible
5 Elemental AnalysisElemental analysis – qualitative or quantitative determination of the elemental composition of a sampleAtomic UV-visible spectroscopic methods are heavily used in elemental analysisOther elemental analysis methods not discussed here:Mass spectrometry (MS), primarily ICP-MSX-ray methods (XRF, SEM/EDXA, Auger spectroscopy, XPS, etc…)Radiochemical or radioisotope methodsClassical methods (e.g. color tests, titrations)Note: there are many other methods for elemental analysis which are not based on optical electronic spectroscopy.
6 Definitions of Electronic Processes Absorption: radiation selectively absorbed by molecules, ions, or atoms, accompanied by their excitation (or promotion) to a more energetic state.Emission: radiation produced by excited molecules, ions, or atoms as they relax to lower energy levels.
7 The Absorption Process Electromagnetic radiation travels fastest in a vacuumWhen EM radiation travels through a substance, it can be slowed by propagation “interactions” that do not cause frequency (energy) changes:Absorption does involve frequency/energy changes, since the energy of EM radiation is transferred to a substance, usually at specific frequencies corresponding to natural atomic or molecular energiesAbsorption occurring at optical frequencies involves low to moderate energy electronic transitionsc = the speed of light (~3.00 x 108 m/s)i = the velocity of the radiation in the medium in m/sni = the refractive index at the frequency iFor more, see pg. 125 of Skoog et al.
8 Absorption and Transmission Transmittance:T = P/P0P0PAbsorbance:A = -log10 T = log10 P0/PbThe Beer-Lambert law commonly uses absorbance as a measure of the absorption rather than %transmittance, because of the linear relationship between concentration and absorbance.A is linear vs. b!(A preferred over T)Graphs from
9 The Beer-Lambert Law and Quantitative Analysis The Beer-Lambert Law (a.k.a. Beer’s Law):A = ebcWhere the absorbance A has no units, since A = log10 P0 / Pe is the molar absorbtivity with units of L mol-1 cm-1b is the path length of the sample in cmc is the concentration of the compound in solution, expressed in mol L-1 (or M, molarity)Beer’s law can be derived from a model that considers infinitesimal portions of a “block” absorbing photons in their cross-sections, and integration over the entire blockBeer’s law is derived under the assumption that the fraction of the light absorbed by each thin cross-section of solution is the sameSee pp of Skoog, et al. for detailsThe Beer-Lambert law commonly uses absorbance as a measure of the absorption rather than %transmittance, because of the linear relationship between concentration and absorbance.
10 Deviations From the Beer-Lambert Law Deviations from Beer’s law (i.e. deviations from the linearity of absorbance vs. concentration) occur from:Intermolecular interactions at higher concentrationsChemical reactions (species having different spectra)Peak width/polychromatic radiationBeer’s law is only strictly valid with single-frequency radiationNot significant if the bandwidth of the monochromator is less than 1/10 of the half-width of the absorption peak at half-height.Detailed discussion of Beer’s Law can be found in Skoog et al., Chapter 13.For an alternative view, see: Bare, William D. A More Pedagogically Sound Treatment of Beer's Law:A Derivation Based on a Corpuscular-Probability Model, J. Chem. Educ. 2000, 77, 929.
11 Deviations from the Beer-Lambert Law Intermolecular interactions at higher concentrations cause deviations, because the spectrum changesDimers,oligomersDetailed discussion of Beer’s Law can be found in Skoog et al., Chapter 13.Figure from Chapter 5 of Cazes, Analytical Instrumentation Handbook 3rd Ed. Marcel-Dekker 2005.
12 Deviations from the Beer-Lambert Law Deviations caused by use of polychromatic light on a spectrum in which e changes a lot over the bandwidth of the light.Consider two wavelengths a and b with a and b = 1000, 1000 = 1500, 500 = 1750, 250Absorbance (A)Detailed discussion of Beer’s Law can be found in Skoog et al., Chapter 13.Concentration (M)
13 Atomic Emission Two types of emission spectra: Examples: Continuum Line spectraExamples:ICP-OES (inductively-coupled plasma optical emission spectroscopy), also known as ICP-AES (atomic emission spectroscopy)LIBS (laser-induced breakdown spectroscopy)Note that emission here refers to spontaneous emission, not the stimulated emission used by lasers.
14 The Emission ProcessAtoms/molecules are driven to excited states (in this case electronic states), which can relax by emission of radiation.M + heat M*Higher energyE = hnLower energyOther process can happen instead of emission, such as “non-radiative” relaxation (e.g. transfer of energy by random collisions).M* M + heat
15 Atomization: The Dividing Line for Atomic and Molecular Optical Electronic Spectroscopy Samples used in optical atomic (elemental) spectroscopy are usually atomizedThis destroys molecules (if present) and leaves just atoms and atomic ionsThe UV-visible spectrum of the atoms is of interest, not the molecular spectrum.In the case of X-ray methods – the X-ray spectrum is not sensitive to molecular effects and atomization is not necessary! This is because core electrons are usually affected by the higher-energy X-ray radiation – physical and chemical state have only minute effects on these core electrons (i.e. gas vs solid, oxide vs. element).
16 Atomic Electronic Energy Levels Electronic energy level transitions in hydrogen – the simplest of all!Balmer series (visible)Transitions start (absorption) or end (emission) with the first excited state of hydrogenLyman series (UV)Transitions start (absorption) or end (emission) with the ground state of hydrogenIn 1885 Balmer derived a simple equation relating the emission lines for hydrogen. It is: 1/ = R(1/22 – 1/n2)R is the Rydberg constant x 107 m-1The equation can be generalized for theLyman series: 1/ = R(1/22 – 1/n2) Paschen series:Brackett series:Pfund series:Diagrams from
17 Atomic Electronic Energy Levels Term symbols and electronic states: used to precisely define the state of electronsspinmultiplicitys = total spin quantum numberj = total angular momentum quantum numberl = orbital quantum number (s,p,d,f…)mj = stateTerm:2Ps,p,d,f,g(l value)Level:2P3/22j+1State:2P3/2-1/2Used to denote energy levels, and label Grotrian (or term) diagrams for the hydrogen atomElectronic configuration (1s22s1 for Li, etc…) does not give all of the info about the arrangement of electrons in a atom.Ex. 2p2, where the two electrons could occupy orbitals with different angular momentum (when l=1, ml can be 1, 0, and –1). Also no spin is given by 2p2.Figure from the Sapphire Electronic Spectroscopy Software Package, Cavendish Instruments Limited.
18 Energy Levels for Different Atoms Atomic absorption and emission are generally selective and specific for different elements on the periodic table, allowing for qualitative identification of elementsIn 1885 Balmer derived a simple equation relating the emission lines for hydrogen. It is: 1/ = R(1/22 – 1/n2)R is the Rydberg constant x 107 m-1The equation can be generalized for theLyman series: 1/ = R(1/22 – 1/n2) Paschen series:Brackett series:Pfund series:Diagrams from
19 Atomic Electronic Energy Levels Term (Grotrian) diagram for the sodium atom: each transition on the diagram can be linked to a peak in the UV-visible spectrumThe number of lines can approach 5000 for transition-metal elements.Line broadening can be caused by:Doppler effectspressure broadening (collisions)Lifetime of state (uncertainty)Figure from H. A. Strobel and W. R Heineman, Chemical Instrumentation: A Systematic Approach, Wiley, 1989.
21 Intensity of Atomic Electronic Energy Levels The population of energy levels partly determines the intensity of an emission peakThe Boltzmann distribution relates the energy difference between the levels, temperature, and population:E = energy of stateP = number of states having equal energy at each levelN = number of atoms in stateKey point: to get more atoms into excited states, you need higher temperatures.Element/Line (nm)Ne/Ng at 2000 KNe/Ng at 3000 KNe/Ng at KNa 589.09.9 x 10-65.9 x 10-42.6 x 10-1Ca 422.71.2 x 10-73.7 x 10-51.0 x 10-2Zn 213.87.3 x 10-155.4 x 10-103.6 x 10-3(Values from Cazes pg 79, Table 1)
22 Basic Instrument Design for Atomic UV-Visible Spectrometers Atomic absorption:RadiationSource(Selectivespectral lines)Sample(in torch)WavelengthSelector(can be beforesample)Detector(photoelectric transducer)Atomic emissionSource(sample intorch)WavelengthSelectorDetector(photoelectric transducer)See Skoog et al. Figure 7-1.Wavelength selector is a mono- or polychromator
23 Sources for Atomic Emission History: Emission came first (study of sunlight by Fraunhofer in 1817, identification of spectral “lines”), studied throughout the 1800’s and early 1900’sBefore the use of the plasma for OES in 1964, the flame/gas torch (or arc/spark, etc…) had the following problems:Temperature instabilityNot hot enough to excite/decompose all materialsAtomizer/Emission SourceTemperature (°C)FlamePlasma (e.g. ICP)Electric arcElectric spark>10000Today: The plasma has become the almost universally-preferred methodHistory: atomic emission placed demands on monochromatorsToday: Technology has led to polychromators/detectors with sufficient resolutionDCP torches – not as hot, fewer emission lines, much more maintenance.
24 Plasma Torch SourcesPlasma: a low-density gas containing ions and electrons, controlled by EM forcesDCP torches – not as hot, fewer emission lines, much more maintenance.
25 Plasma Torch SourcesIn the inductively-coupled plasma (ICP) torch, the sample will reside for several milliseconds at K.Other designs: direct current plasma, microwave induced plasmaDCP torches – not as hot, fewer emission lines, much more maintenance.An argon ICP torch in action:Photo by Steve Kvech,
26 More on Plasma Torches Another view of an argon ICP torch: DCP torches – not as hot, fewer emission lines, much more maintenance.Diagram from Lagalante, Appl. Spect. Reviews. 34, 191 (1999)
27 Arc and Spark Sources for Atomic Emission Arc and spark sources – used for qualitative analysis of organic and geological samplesOnly semi-quantitative because of source instabilitySpark sources achieve higher energiesSeveral mg of solid sample is packed between electrodes, 1-30 A of current is passed achieving several hundred volts potential.Applications include metals analysis or cases where solids must be analyzed.
28 Designs for Monochromators and Polychromators Paschen-Runge design, shown as a polychromatorCzerny-Turner design, shown as a monochromatorPolychromatorsHigh sample throughput rateSpectral interference can be an issue if the interfering spectral line is not included on the detector arrayMonochromatorsFlexibility to access any wavelength within the dimensions of the monochromatorGood for applications requiring complex background correctionsLess sensitive – lower radiation throughput (because light blocked by slits)
29 Atomic Emission: Diffraction Gratings Diffraction gratings are used to select wavelengths (in combination with collimating lens, and slits)Echelle (ladder) gratings: high dispersion and high resolution (a two-step system with a cross-disperser standard grating or prism)~ grooves/mm typical for UV-Vis workRequire filters to isolate “orders” (i.e. n=1)Figure from T. Wang, in J. Cazes, ed, “Ewing’s Analytical Instrumentation Handbook”
30 Atomic Emission: Detectors At the end of the spectrometer, photons are detected.Commonly used detectors:Photomultiplier tubes (PMT) – dynamic range 109Solid-state detectors:Charge-coupled devices (CCD) – 1D or 2D arrays (charge readout or “transfer” devices)Silicon photodiodes with thousands of individual addressable elementsThese detectors are very sensitive, very well-suited to 2D echelle grating polychromators, very fast
31 Example Detector: Photomultiplier Tubes A PMT is a vacuum tube that contains a photosensitive material, called the photocathodeThe photocathode ejects electrons when it is struck by light. These ejected electrons are accelerated towards a dynode which ejects two to five secondary electrons for every electron that strikes its surface.The secondary electrons strike another dynode, ejecting more electrons which strike yet another dynode, and so on (electron multiplication).The electrical current measured at the anode is then used as a relative measure of the intensity of the radiation reaching the PMT.
32 Modern ICP-OES Spectrometers Example system:Varian Vista PROFeatures:1. Axial flame view2. Echelle grating polychromator (note the design is like a Czerny-Turner monochromator)3. CCD detectorCCD chips are made of sub-arrays matched to emission lines.This design features an axial view of the plasma, a echelle polychromator, a CCD chip detector, and no moving parts.It can measure wavelengths between nm simultaneously. Its advantages translate into the following benefits: less time and sample needed for multiple element scans, the ability to measure multiple wavelengths for a given element for confirmation in quantitative analyses, and reduced flicker noise because the line, background, and/or internal standard can be measured all at the same time.Typical cost: $110K USDFigure from Varian Vista PRO sales literature.
33 Detection Limits of ICP-OES Typical detection limits (for a Varian Vista MPX)Considerations include the number of emission lines, spectral overlapLinearity can span several orders of magnitude.Note – axial view maximizes sensitivity, radial view maximizes stability.Note limits in ppb assuming equal densities.
34 Atomic Absorption Spectroscopy (AAS) In the beginning – atomic emission was the only way to do elemental analysis via optical spectroscopyBunsen and Kirchhoff (1861) – invented a non-luminous flame to study emission. Showed that alkali elements in the flame removed lines from a continuous source.Walsh (1955) – notices that molecular spectra are often obtained in absorption (e.g. UV-Vis and IR), but atomic spectra are always obtained in emission. Proposes to use atomic absorption (AA or AAS) for elemental analysisAdvantages over emission – far less interference, avoids problems with flame temperatureElectrothermal vaporizers/atomizers also used, take advantage of conductive heating.
35 Atomic Absorption Spectroscopy: Instruments Atomic absorption spectrometry is one of the most widely used methods for elemental analysis.Basic principles of AA:The sample is atomized via:A flame (methane/H2/acetylene and air/oxygen)An electrothermal atomizer (an electrically-heated graphite tube or cup)UV-Visible light is projected through the flameThe atoms absorb light (electronic excitation), reducing the beamThe difference in intensity is measured by the spectrometerSourceP0Sample/FlamePMonochromatorDual flame/electrothermal atomizers are now available. Electrothermal vaporizers/atomizers are used for higher sensitivity applications, take advantage of conductive heating. See chapter 9 of Skoog et al.DetectorImages are of Aurora AI1200,
36 Atomic Absorption: Sources Hollow cathode lamps – sputtering of an element of interest, generating a line emission spectrum:EDL stands for electrode-less discharge lamp.Anode – the element in an electron tube, sometimes called the plate, that attracts the electrons emitted by the cathode.Cathode – the element of an electron tube that emits electrons.Typical linewidths of nm (0.02Å)Single and multi-element lamps are availableOther AA Sources: electrode-less discharge lamp (EDL) – see Skoog Ch 9B-1
37 Atomic Absorption: Monochromators The monochromator filters out undesired light in AA (typical bandwidths are 1 angstrom/0.1 nm)This differs from ICP-OES, where the monochromator actually analyzes the frequency.In other words – there is no need to scan the grating, just set (aimed through a slit) and runEchelle (ladder) gratings (combined with a cross-disperser) are popular:Figure from T. Wang, in J. Cazes, ed, “Ewing’s Analytical Instrumentation Handbook”
38 Other Features of Atomic Absorption Systems Sample nebulizers: Produces aerosols of samples to introduce into the flame (oxyacetylene is the hottest)Detectors: Common examples are photomultiplier tubes, CCD (charge-coupled devices), and many more.Monochromator: removes emissions from the flame (flame is often kept cool just to avoid emission)Modulated source (chopper): also removes the remaining emissions from the flame. The signal of interest is given an AC modulation and passed through a high-pass filter.Spectral interferences:Absorption from other things (besides the element of interest) – other flame components, particulates, etc… Scattering can cause similar problemsBackground correction can help
39 Graphite Furnace and Hydride AAS Graphite furnace and electrothermal AASAnalyze solutions, solids, slurries, by placing a small amount (uL) of sample on a support for evaporation and them atomizationMore efficient atomization (entire sample atomized at once) – leads to smaller sample quantity requirements or better sensitivity, but reproducibility can be an issueHydride generation AASEfficiently volatilizes hydride forming elements (As, Se, Tl, Pb, Bi, Sb, Te) by making their hydrides via pre-reaction with sodium borohydride and HClInexpensive method of increasing sensitivity of an AAS to ppt levels for these elementsMercury cold-vapor AAS (Hg only)
40 Detection Limits of Atomic Absorption Systems Detection limits in ppb (µg/L) for a selection of elementsIndividual results can vary depending on system, matrix, etc…AAS(Flame)(Electrothermal)ICP-OESAl300.0052As1000.0240Cd10.0001Hg5000.1Mg0.05Pb100.002Sn20ZnValues from D. A. Skoog, et al., “Principles of Instrumental Analysis,” 5th Ed., Orlando, Harcourt Brace and Co. 1998, pg. 225.
41 How Are Elements Actually Analyzed? For AA and ICP-OES, samples are dissolved or digested into solution, flowed into the flame/plasma and analyzed.Two methods for quantitative analysis calibration:Standard calibration: the unknown sample’s absorbance/emission is compared with several references which “bracket” the expected concentration assuming a linear relationship.Standard addition: the unknown sample is divided into several portions. One portion is directly analyzed, the others have the reference material added in varying amounts. The linear relationship is determined, and the intercept is used to calculate the real concentration of the unknown.Speciated analysis may be needed. The analysis of atomic “species”, elements in chemically distinguishable environments, usually by hyphenation (e.g. ICP-OES coupled to a HPLC, AA coupled to a GC) or offline extraction.At the end: the results yield elements in ppm, ppb, mg/mL, or below LOQ or LOD
42 Laser-Induced Breakdown Spectroscopy (LIBS) A focused laser can be used to create a plasma (usually a pulsed Q-switched Nd:YAG laser)Portable systems capable of standoff analysis are now available – applications in the detection of explosives, chemical warfare agents, environmental analysis, etc…Figure from D. A. Cremers, R. C. Chinni, “Laser-induced breakdown spectroscopy - Capabilities and limitations,” Appl. Spectrosc. Rev., 2009, 44, ,
43 A Typical LIBS Spectrum The LIBS spectrum of ibuprofen drug substanceFrom the paper’s experimental section: “The instrumentation used consisted of a Nd:YAG laser, an xyz stage carrying thesample (Standa ), a spectrograph, and an intensified charge-coupled device (ICCD) detector. A Nd:YAG laser (Brilliant Quantel, Q-Switched) with a 115 mJ laser pulse energy at the second harmonic of 532 nm, a 4.4 ns pulse duration, and 0.7 Hz repetition frequency was used. The crater diameter was 0.4 mm. The plasma light was collected and transported to the spectrograph by a light collector and optical fiber. The collector position was adjusted by a diode laser (Andor, HE-OPI-0009). An Echelle spectrograph (Andor Mechelle ME5000, focal length 195 mm, F/7, k/Dk 5,000, spectral range 200–975 nm) was coupled to an ICCD detector (Andor iStarDH734, 1, ,024 pixels, lm2/pixel, 18 mm intensifier diameter). This system was calibrated by a Hg:Ar lamp (Ocean Optics, HG-1, Hg–Ar lines 253–922 nm). A measurement gate delay time of 1 us and an integration time of 500 ns were optimized.”Emission lines used for C, H, O, and N analysis were 247.9, 656.3, (triplet), and nm, along with the molecular band of C2 at 516 nm.Figure from J. Anzano et al., “Rapid characterization of analgesic pills by laser-induced breakdown spectroscopy (LIBS),” Med. Chem. Res. 2009, 18, 656–664.
44 Atomic FluorescenceDeveloped as an alternative to AA and ICP-OES, with potentially greater sensitivity.Has not yet achieved widespread use but cheaper tunable lasers may change this.Laser – stimulated emission (coherent emission from an excited state induced by a second photon)Processes that emit a fluorescent photon:hvNon-radiativeThermalhvhvNon-radiativehvResonanceDirect LineStepwiseThermally-assisted
45 (photoelectric transducer) Atomic FluorescenceBasic AF instrument design:SampleWavelengthSelectorDetector(photoelectric transducer)Radiationsource(90° angle)AF sources include hollow-cathode lamps, electrodeless discharge tubes (brighter), and lasers (brightest)EDLs produce atomic line spectra that is brighter than HCTs. Ionized argon in a sealed quartz tube is used to excite a small quantity of a metal (or salt). The argon is excited and ionized by strong RF at ~20-40 MHz.Picture of HCT lamps from Perkin-Elmer
46 A Comparison of Atomic Fluorescence with Other Techniques Plasma Emission (ICP-OES)AA (Flame)Atomic FluorescenceDynamic RangeWideLimitedQualitative AnalysisGoodPoorMultielement Scan?Trace AnalysisSmall samplesMatrix interferencesLowHighSpectral interferencesCostModerate ($100K USD)Low ($50K USD)Moderate
47 Further Reading Required: Optional: A. F. Lagalante, “Atomic absorption spectroscopy: A tutorial review.” Appl. Spectrosc. Rev. 1999, 34,A. F. Lagalante, “Atomic emission spectroscopy: A tutorial review.” Appl. Spectrosc. Rev. 1999, 34,Optional:J. Cazes, Ed. Ewing’s Analytical Instrumentation Handbook, 3rd Edition, 2005, Marcel Dekker, Chapters 3 and 4.D. A. Skoog, F. J. Holler and S. R. Crouch, Principles of Instrumental Analysis, 6th Edition, 2006, Brooks-Cole, Chapters 8, 9, and 10.N. Lewen, “The use of atomic spectroscopy in the pharmaceutical industry for the determination of trace elements in pharmaceuticals,” J. Pharm. Biomed. Anal. 2011, 55, ,H. A. Strobel and W. R. Heineman, “Chemical Instrumentation: A Systematic Approach”, 3rd Ed., Wiley (1989).D. A. Cremers, R. C. Chinni, “Laser-induced breakdown spectroscopy - Capabilities and limitations,” Appl. Spectrosc. Rev., 2009, 44, ,