Atomic Absoption Spectroscopy. Electron excitation –The excitation can occur at different degrees low E tends to excite the outmost e - ’s first when.

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Presentation transcript:

Atomic Absoption Spectroscopy

Electron excitation –The excitation can occur at different degrees low E tends to excite the outmost e - ’s first when excited with a high E (photon of high v) an e - can jump more than one levels even higher E can tear inner e - ’s away from nuclei –An e - at its excited state is not stable and tends to return its ground state –If an e - jumped more than one energy levels because of absorption of a high E, the process of the e - returning to its ground state may take several steps, - i.e. to the nearest low energy level first then down to next … Atomic Spectra Energy n=1 n=2 n=3 n=4 1s 2s 2p 3s 3p 4s 3d 4p 4d 4f n = 1 n = 2 n = 3, etc. energy  E

Atomic spectra –The level and quantities of energy supplied to excite e - ’s can be measured & studied in terms of the frequency and the intensity of an e.m.r. - the absorption spectroscopy –The level and quantities of energy emitted by excited e - ’s, as they return to their ground state, can be measured & studied by means of the emission spectroscopy –The level & quantities of energy absorbed or emitted (v & intensity of e.m.r.) are specific for a substance –Atomic spectra are mostly in UV (sometime in visible) regions Atomic Spectra Energy n=1 n=2 n=3 n=4 1s 2s 2p 3s 3p 4s 3d 4p 4d 4f n = 1 n = 2 n = 3, etc. energy  E

Atomic spectroscopy Atomic emission –Zero background (noise) Atomic absorption –Bright background (noise) –Measure intensity change –More signal than emission –Trace detection

Argon HydrogenHelium Iodine Mercury Neon Nitrogen

Signal is proportional top number of atoms AES - low noise (background) AAS - high signal The energy gap for emission is exactly the same as for absorption. All systems are more stable at lower energy. Even in the flame, most of the atoms will be in their lowest energy state.

Boltzmann Distribution All systems are more stable at lower energy. Even in the flame, most of the atoms will be in their lowest energy state. At 3000K, for every 7 Cs atoms available for emission, there are 1000 Cs atoms available for absorption. At 3000 K, for each Zn available for emission, there are approximately Zn atoms available for absorption.

Source: R. Thomas, “Choosing the Right Trace Element Technique,” Today’s Chemist at Work, Oct. 1999, 42. Atomic Absorption/Emission Spectroscopy Atomic absorption/emission spectroscopes involve e - ’s changing energy states Most useful in quantitative analysis of elements, especially metals  These spectroscopes are usually carried out in optical means, involving  conversion of compounds/elements to gaseous atoms by atomisation. Atomization is the most critical step in flame spectroscopy. Often limits the precision of these methods.  excitation of electrons of atoms through heating or X-ray bombardment  UV/vis absorption, emission or fluorescence of atomic species in vapor is measured  Instrument easy to tune and operate  Sample preparation is simple (often involving only dissolution in an acid)

A. Walsh, "The application of atomic absorption spectra to chemical analysis", Spectrochimica Acta, 1955, 7,

The original 1954 AAS instrument

Atomic Absorption Spectrometer (AA) Source Sample P P0P0 Chopper Wavelengt h Selector Detector Signal Processor Readout TypeMethod of AtomizationRadiation Source atomic (flame) sample solution aspirated Hollow cathode into a flame lamp (HCL) atomic (nonflame) sample solution HCL evaporated & ignited x-ray absorptionnone required x-ray tube

Atomic Emission Spectrometer (AES) Source Sample P Wavelength Selector Detector Signal Processor Readout TypeMethod of Atomization Radiation Source arcsample heated in an electric arc sample sparksample excited in a high voltage spark sample argon plasma sample heated in an argon plasma sample flamesample solution aspirated into a flame sample x-ray emissionnone required; sample bombarded w/ e- sample

Atomic Fluorescence Spectrometer (AFS) Source Sample PP0P0 Chopper 90 o Wavelength Selector Detector Signal Processor Readout TypeMethod of Atomization Radiation atomic (flame) sample solution aspirated into a flame sample atomic (nonflame) sample solution sample evaporated & ignited x-ray fluorescencenone required sample

The hollow cathode lamp is an example of a metal vapour lamp at emits light at the characteristic wavelength(s) of the metal in the cathode. The lamp gas is under near-vacuum conditions. Electron flow ionises the gas. The cations bombard the cathode to vaporise the metal. Combination of ion-atom collisions, electron-atom collisions, and other processes excite the electrons inside the metal vapour atoms, which emit light.

Electron and ionic impact on cathode M(s)  M(g) M(g)    M*(g) M*(g)  M(g) + hn Hollow cathode lamp Thin lay of cathode material

A.Flame Atomization Nebulization -Conversion of the liquid sample to a fine spray. Desolvation -Solid atoms are mixed with the gaseous fuel. Volatilization -Solid atoms are converted to a vapor in the flame. There are three types of particles that exist in the flame:There are three types of particles that exist in the flame: 1)Atoms 2)Ions 3)Molecules

1.Types of Flames Fuel / OxidantTemperature H-C  C-Hacetylene / air2100 °C – 2400 °C (most common) acetylene / N 2 O2600 °C – 2800 °C acetylene / O °C – 3150 °C Selection of flame type depends on the volatilization temperature of the atom of interest.Selection of flame type depends on the volatilization temperature of the atom of interest. 2.Flame Structure Interzonal region is the hottest part of the flame and best for atomic absorption.Interzonal region is the hottest part of the flame and best for atomic absorption. Fuel rich flames are best for atoms because the likelihood of oxidation of the atoms is reduced.Fuel rich flames are best for atoms because the likelihood of oxidation of the atoms is reduced. Oxidation of the atoms occurs in the secondary combustion zone where the atoms will form molecular oxides and are dispersed into the surroundings.Oxidation of the atoms occurs in the secondary combustion zone where the atoms will form molecular oxides and are dispersed into the surroundings.

3.Temperature Profiles It is important to focus the entrance slit of the monochromator on the same part of the flame for all calibration and sample measurements.It is important to focus the entrance slit of the monochromator on the same part of the flame for all calibration and sample measurements. 4.Flame Absorption Profiles Mg -atomized by longer exposure to flame, but is eventually oxidized.Mg -atomized by longer exposure to flame, but is eventually oxidized. Ag -slow to oxidize, the number of atoms increases with flame height.Ag -slow to oxidize, the number of atoms increases with flame height. Cr -oxidizes readily, highest concentration of atoms at the base of the flame.Cr -oxidizes readily, highest concentration of atoms at the base of the flame.

5.Flame Atomizers Sample is “pulled” into the nebulization chamber by the flow of fuel and oxidant.Sample is “pulled” into the nebulization chamber by the flow of fuel and oxidant. Laminar Flow Burners Contains spoilers (baffles) to allow only the finest droplets to reach the burner head.Contains spoilers (baffles) to allow only the finest droplets to reach the burner head. Burner head has a long path length and is ideal for atomic absorption spectroscopy.Burner head has a long path length and is ideal for atomic absorption spectroscopy.

Flame Burner M n+ (aq) + anion(aq)  salt(s) salt(s)  salt(g) salt(g)  atoms (g) M*(g)  M(g) + h

Detection limits (ppm = ng mL-1) The detection limit is the smallest amount of an element that can be reliably measured. Smaller limits of detection (LODs) are better. Some common light metals have a lower LOD using flame atomic emission. Most transition elements have a significantly lower LOD using AAS.

Student determination of Fe Fe: 0.05 mg mL mL volumetric flasks 1.00 mL pipette 2 mL1 mL3 mL4 mL5 mL

Determination of Fe