Lecture 6 Atomic Spectroscopy

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    Lecture 6 ATOMIC SPECTR

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    Sample is atomized (atoms/ions)

    absorption or emission measured

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    ENERGY LEVEL DIAGRAMS

    Every elements has unique set of atomic orbital

    p,d,f... levels split by spin-orbit coupling

    Spin (s) and orbital (l) motion create magnetic

    that perturbeach other (couple) if fields parallel - slightly higher energy if fields antiparallel - slightly lower energy

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    ELECTRONIC TERM SYMBOLS

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    Similar pattern between atoms but different s Spectrum of ion different to atom Separations measured in electronvolts (eV)

    As # of electrons increases, # of levels increaseEmission spectra become more complexLi 30 lines, Cs 645 lines, Cr 2277 lines

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    As # of electrons increases, # of levels increase

    Emission spectra become more complex

    Li 30 lines, Cs 645 lines, Cr 2277 lines

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    Desire narrow lines for accurate identification

    Broadened by

    (i) uncertainty principle(ii) pressure broadening(iii) Doppler effect(iv) (electric and magnetic fields)

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    (i) Uncertainty Principle:

    Quantum mechanical idea states must measure

    some minimum time to tell two frequencies apa

    ATOMIC LINE WIDTHS

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    Shows up in lifetime of excited state

    if lifetime infinitely long, E infinitely narrow

    if lifetime short, E is broadened

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    Example

    Lifetime of Hg*=2x10-8 s. What is uncertainty

    broadening for 254 nm line?

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    Differentiating with respect to frequency:

    sometimes called natural linewidth.

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    (ii) Pressure broadening:Collisions with atoms/molecules transfers smallquantities of vibrational energy (heat) - ill-defin

    ground state energy

    Effect worse at high pressures For low pressure hollow cathode lamps (1-10 1-10-2 For high pressure Xe lamps (>10,000 torr) 10 (turns lines into continua!)

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    (iii) Doppler broadening:Change in frequency produced by motion relatdetector

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    Other Effects of T on Atomic Spectrometry

    T changes # of atoms in ground and excited sta

    Boltzmann equation

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    Important in emission measurements relying onexcitation

    Na atoms at 2500 K, only 0.02 % atoms in firststate!

    Less important in absorption measurements - 9atoms in ground state!

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    Methods for Atomizingand Introducing Sample

    Sample must be convertedto atoms first

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    Must transfer sampleto atomizer - easy forgases /solutions but

    difficult for solids

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    Lecture 7 ATOMIC EMMISION SPECTR

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    Excitation and Atomization:

    Traditionally based on flame but

    arc and spark plasma

    excitation offers(i) increased atomization/excitation

    (ii) wider range of elements(iii) emission from multiple speciessimultaneously

    (iv) wide dynamic range

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    Flame Excitation Sources:

    Primary Combustion Zone

    Interzonal RegionSecondary Combustion Zone

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    ATOMIC EMISSION SPECTR

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    Arc and Spark Excitation Sources:

    Limited to semiquantitative/qualitative analys

    flicker) Usually performed on solids Largely displaced by plasma-AES

    Electric current flowing between two C electrode

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    Electric current flowing between two C electrode

    ATOMIC EMISSION SPECTR

    Sample pressed into

    electrode or mixed withCu powder and pressed

    briquetting

    Cyanogen bands (CN)

    350-420 nm occur with

    C electrodes in air -

    He, Ar atmosphere

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    Arc/spark unstable - each line measured >20 s multichannel detection)

    photographic film: Cheap Long integration times Difficult to develop/analyze Non-linearity of line "darkness"

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    Plasma Excitation Sources:

    gas containing high proportion of cations and el(1) Inductively Coupled Plasma (ICP)

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    Plasma Structure: Brilliant white core - Arcontinuum and lines Flame-like tail up to 2 cm Transparent region -measurements made Hotter than flame (10,000K) - more completeatomization/excitation

    Atomized in "inert"atmosphere Little ionization - too manyelectrons in plasma

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    (2) Direct Current (DC)Plasma DC current (10-15 A)flows between C anodesand W cathode

    Plasma core at 10,000 K,viewing region at ~5,000K

    Simpler, less Ar than ICP- less expensive

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    Three instrument types:

    sequential (scanning and slew-scanning)

    Multichannel

    (Fourier transform FT-AES)

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    S i l i PMT d b hi d

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    Sequential instrument - PMT moved behind apeplate, or grating+prism moved to focus new oslit

    Cheaper Slower Pre-configured exit slits to detect up to 20 line

    scanMultichannel instrument - multiple PMT'sExpensiveFaster

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    S l ti S l I t d ti

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    Solution Sample Introduction:(1) Electrothermal vaporizer* (ETV) electric current rapidly heats crucible containin

    sample sample carried to atomizer by gas (Ar, He) only for introduction, not atomization

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    (2) N b li t l ti t fi

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    (2) Nebulizer - convert solution to fine spray or

    a) Ultrasonic nebulizer uses ultrasound waves t

    solution flowing across disc

    b) Pneumatic nebulizer uses high pressure gas entrain solution

    ATOMIC EMISSION SPECTR

    Cross flow Nebulizer

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    Cross-flow Nebulizer

    ATOMIC EMISSION SPECTROSCOPY

    Solid Sample Introduction:

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    Solid Sample Introduction:

    (1) Electrothermal vaporizer*(2) Direct Insertion(*) uses powder placed insid

    plasma, arc or spark atomizer (atomizer acts asvaporizer)Coating on electrode in atomizer(3) Ablation uses coating of electrodes in dischaand sample entrained in Ar or He gas

    Laser ablation uses laser to vaporize sample

    ATOMIC EMISSION SPECTR

    APPLICATION OF AES

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    APPLICATION OF AES

    AES relatively insensitive (small excited state poat moderate temperature)

    AAS still used more than AES(i) less expensive/complex instrumentation(ii) lower operating costs(iii) greater precision

    ATOMIC EMISSION SPECTR

    In practice ~60 elements detectable

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    In practice ~60 elements detectable 10 ppb range most metals Li, K, Rb, Cs strongest lines in IR

    Large # of lines, increase chance of overlap

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    ATOMIC EMISSION SPECTR

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    Lecture 8 ATOMIC ABSOSPECTR

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    ATOMIC ABSORPTION SPECTROSCO

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    ATOMIC ABSORPTION SPECTROSCO

    AAS intrinsically more sensitive than AES

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    similar atomization techniques to AES

    addition ofradiation source

    high temperature for atomization necessaryflame and electrothermal atomization

    very high temperature for excitation not necessary/ gno plasma/arc/spark AAS

    ATOMIC ABSORPTION SPECTROSCO

    FLAME AAS:i l t t i ti f / l ti / lid

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    simplest atomization of gas/solution/solid

    laminar flow burner - stable "sheet" of flame

    flame atomization best for reproducibility (pre(

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    most sensitive part of flame for AAS varies with

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    ATOMIC ABSORPTION SPECTR

    Consequences?

    sensitivity varies with ele

    must maximize burner po

    makes multielement dete

    difficult

    Electrothermal Atomizers:

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    entire sample atomized short time (2000-3000

    sample spends up to 1 s in analysis volume

    superior sensitivity (10-10-10-13 g analyte)

    less reproducible (5-10 %)

    ATOMIC EMISSION SPECTR

    Graphite furnace ETA

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    external Ar gas prevents tube destructioninternal Ar gas circulates gaseous analyte

    ATOMIC ABSORPTION SPECTR

    Three step sample preparation for graphite furn1) Dry - evaporation of solvents (10->100 s)

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    1) Dry - evaporation of solvents (10->100 s)2) Ash - removal of volatile hydroxides, sulfates

    carbonates (10-100 s)3) Fire/Atomize - atomization of remaining anal

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    ATOMIC ABS

    SPECTR

    Atomic Absorption Instrumentation:

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    AAS should be very selective - each element hdifferent set of energy levels and lines very na

    BUT for linear calibration curve (Beers' Law) nbandwidth of absorbing species to be broader that of light source difficult with ordinary

    monochromator

    ATOMIC ABSORPTION SPECTR

    Solved by using very narrow line radiation sour

    i i i l b d i

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    minimize Doppler broadening

    pressure broadening

    lower P and T than atomizerand using resonanabsorption

    Na emission 3p2s at 589.6 nm used to probe

    analyte

    ATOMIC ABSORPTION SPECTR

    Hollow Cathode Lamp:

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    ATOMIC ABSORPTION SPECTR

    300 V applied between anode (+) and metal cathode

    Ar ions bombard cathode and sputter cathode atoms

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    Ar ions bombard cathode and sputter cathode atoms

    Fraction of sputtered atoms excited, then fluoresce

    Cathode made of metal of interest (Na, Ca, K, Fe...)different lamp for each element

    restricts multielement detection

    Hollow cathode to

    maximize probability of redeposition on cathoderestricts light direction

    ATOMIC ABSORPTION SPECTR

    ELECTRODELESS DISCHARGE LAMP

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    Signal at one wavelength often contains luminescence finterferents in flame

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    Chemical interference:

    (i) reverses atomization equilibria(ii) reacts with analyte to form low volatility compoundreleasing agent- cations that react preferentially interferent - Sr acts as releasing agent for Ca withphosphate

    protecting agent- form stable but volatile compoanalyte (metal-EDTA formation constants)

    ATOMIC ABSORPTION SPECTR

    IONIZATION

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    ATOMIC ABSORPTION SPECTR

    hotter atomization means:

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    more ionization

    emission from interferents

    ATOMIC ABSORPTION SPECTR

    Spectral interference - emission or absorption interferent overlaps analyte

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    ATOMIC ABSORPTION SPECTR

    Beam usuall

    ormodulated

    frequency

    Signal then c

    constant (ba

    and dynamic

    varying) sign

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    ATOMIC ABSORPTION SPECTR

    DETECTION LIMITS for AAS/AES?

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    AA/AE comparable (ppb in flame)

    AAS less suitable forweak absorbers (forbidden transitions)

    metalloids and non-metals (absorb in UV)

    metals with low IP (alkali metals)

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    ATOMIC EMISSION SPECTR

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    INTRODUCTION TO ATOMIC SPECTROMETR

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