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An Introduction to Spectrometric Methods 1 Bivek Timalsina [email protected]

Introduction to spectroscopic methods

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Page 1: Introduction to spectroscopic methods

1

An Introduction to

Spectrometric Methods

Bivek [email protected]

Page 2: Introduction to spectroscopic methods

2

Quantum Mechanical Properties of Electromagnetic Radiation (EMR)

The amount of energy involved in transitions from its ground state to exited state (following absorption of energy) and from excited to ground state (by emission of radiation) is given by the following equation;

ΔE = E1 – E2 = hV

where, ΔE = change in energy state of the electron or the energy of electromagnetic radiation absorbed or emitted by an atom or molecule.

E1 = energy of electron in original state,E2 = energy of electron in the final state,h = the Plank’s constant

V= frequency of the electromagnetic radiation in hertz (C/ λ), where, C= speed of electromagnetic radiation (3x108 m/s)

λ = wavelength of electromagnetic radiation

(= 6.63 x 10-34 JS)The greater the energy, the higher the frequency and wavenumber and the shorter the wavelength

Page 3: Introduction to spectroscopic methods

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Energy level and transition in atom and molecule

E0

E1

E2

E3

E4

Atomic energy level Molecular energy level

Page 4: Introduction to spectroscopic methods

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Emission of Radiation

Page 5: Introduction to spectroscopic methods

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Absorption of Radiation

Page 6: Introduction to spectroscopic methods

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The Beer-Lambert Law

I0

Sample

I Detector

Source

Cuvette

Transmittance, T, is simply defined as “the fraction of light that reaches a detector after passing through a sample”

T = I/I0 …………… (i)

Where, I0 = intensity of Incident radiationI= intensity of transmitted radiation

Percentage Transmission (%T) = % T = I/I0 x 1000 < %T < 100

Page 7: Introduction to spectroscopic methods

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The Beer-Lambert Law

Absorbance (A): A = -log T = log (1/T) = log (I o / I)

Absorbance is also called as Optical Density (O.D.)range from 0 (= 100% T) to infinity (=0%T).

The Beer-Lambert law states Absorbance is directly proportional to:1. concentration, c, of absorbing species in the sample (A c)2. path length of light, L, through the sample (A L)

A = € C L ……………… (iii)Where, € = Molar absorbance coefficient of the absorber

C = Concentration of absorbing solution, andb = Path length through the solution (or thickness)

Page 8: Introduction to spectroscopic methods

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The Beer-Lambert Law

Absorbance (A):

A = € C L ……………… (iii) Concentration of the analyte is given in unit mol/L (M) The path length, L, in cm , is called the molar absorptivity or molar absorption coefficient “Absorbance of 1 M solution measured in a cell of 1 cm pathlength”

, is characteristic for each substance at a particular wavelength, .

11111 cmMcmmolLcm

Lmolcl

A

Page 9: Introduction to spectroscopic methods

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Concentration

Abs

orba

nce,

A

0

0.5

1

Concentration

Tran

smitt

ance

, TA=cLcertain constant LOne analyte

T=10-A =10- bc

Beer’s law is a relation between absorbance and concentration which is a straight line passes by origin at constant pathlength, b, and at certain wavelength, .

Transmittance decreases exponentially as concentration

increases

Beer’s law is obeyed for monochromatic light

Slope = L

The Beer-Lambert Law

Page 10: Introduction to spectroscopic methods

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Beer’s Law and Multicomponent samples

For sample containing several absorbing components (say X and Y) given that there are no interactions between the components, the total absorbance is,

Atotal = Ax+ By = €x Cx L + €y Cy L

Page 11: Introduction to spectroscopic methods

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The Beer-Lambert Law

Blank

Detector

Source

I0

Use of Blank

I0

Sample

I Detector

Source

Cuvette

Page 12: Introduction to spectroscopic methods

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The Beer-Lambert LawA = € C L

Use of Curve

Page 13: Introduction to spectroscopic methods

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This relationship is a linear for the most part. However, under certain

circumstances the Beer relationship gives a non-linear relationship.

These deviations from the Beer Lambert law can be classified into three

categories:

Real Deviations - These are fundamental deviations due to the limitations

of the law itself.

Chemical Deviations- These are deviations observed due to specific

chemical species of the sample which is being analyzed.

Instrument Deviations - These are deviations which occur due to how the

absorbance measurements are made.

Derivation of Beer Lambert Law

Page 14: Introduction to spectroscopic methods

ReadoutAbsorbance

0.00

Source

Detector

The Beer-Lambert LawA = € C L

14

Path Length Dependence, L

Page 15: Introduction to spectroscopic methods

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Path Length Dependence, L ReadoutAbsorbance

0.22

Source

Detector

b

Sample

The Beer-Lambert LawA = € C L

Page 16: Introduction to spectroscopic methods

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Path Length Dependence, L

ReadoutAbsorbance

0.44

Source

Detector Samples

Of course, we are not introducing two cells in the light pathway, but let us assume that we doubled the path length of light through the absorbing medium

The Beer-Lambert LawA = € C L

Page 17: Introduction to spectroscopic methods

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ReadoutAbsorbance

0.66

Source

Detector Samples

The Beer-Lambert LawA = € C L

Path Length Dependence, L

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Concentration Dependence, c ReadoutAbsorbance

0.00

Source

Detector

The Beer-Lambert LawA = € C L

Page 19: Introduction to spectroscopic methods

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Concentration Dependence, c

ReadoutAbsorbance

0.42

Source

Detector

b

Sample

The Beer-Lambert LawA = € C L

Page 20: Introduction to spectroscopic methods

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Concentration Dependence, c ReadoutAbsorbance

0.63

Source

Detector

b

Sample

The Beer-Lambert LawA = € C L

Page 21: Introduction to spectroscopic methods

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Wavelength Dependence,

ReadoutAbsorbance

0.30

Source

Detector

b

The blue solution do absorb the red radiation

The Beer-Lambert LawA = € C L

Page 22: Introduction to spectroscopic methods

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Wavelength Dependence,

ReadoutAbsorbance

0.00

Source

Detector

b

The red solution can not absorb the red radiation but it can absorb radiation that is complimentary to red.

The Beer-Lambert LawA = € C L

Page 23: Introduction to spectroscopic methods

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Any Questions ?