Spectrophotometry Flashcards

1
Q

What is electromagnetic radiation?

A
  • Electromagnetic radiation comprises radiant energy extending from cosmic rays (λ 10-9 nm) to radio waves (λ km).
  • ‘Visible Light’ – describes radiant energy in the visible portion of spectrum where our eyes work.
  • All forms of electromagnetic radiation travel at the speed of light.

speed of light in a vacuum (c): 299,792,458 metres per second.

186,000 miles per second.

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2
Q

What is the equation of wavelegnth?

A

Wavelength is inversely proportional to a given frequency:

v = c / λ

v = frequency of light (cycles per second)

c = speed of light in a vacuum (3 x 1010 cm/s)

λ = wavelength in cm

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3
Q

What is energy proportional to?

A

Energy is proportional to frequency

  • The relationship between the energy of photons and their frequency is proportional.
  • It makes sense that the more times a wave wobbles in a second, then the more energy required to make that happen:

E = hv

E = energy (ergs)

h = Plank’s constant (6.62 x 1027 erg s)

v = frequency of light (cycles per second [Hz])

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4
Q

What is energy inversely proprotional to?

A

Therefore, it stands that wavelength (λ) is inversely proportional to E

E = hc / λ

For example: UV radiation at 200 nm possesses greater energy than IR radiation at 750 nm.

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5
Q

What happens when light interacts with matter?

A
  • Be absorbed
  • Be transmitted
  • Be scattered
  • Be reflected
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6
Q

What happens when absorbed light interacts with electrons?

A
  • Electrons in the “ground state” promoted to higher energy orbitals
  • Energy absorbed corresponds to difference between orbitals
  • Energy is then lost either vibrationally (non-radiative) or radiatively e.g. fluorescence
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7
Q

Why are organic molecules useful in spectrophotemetry?

A
  • Organic molecules often have conjugated double bond systems, so easy for electrons to move around (delocalise).
  • Conjugated double bond systems have fairly low energies for absorption.
  • Since colour occurs with absorption, many organic conjugatedcompounds are coloured
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8
Q

Why are some chemical coloured?

A
  • lThe wavelength of light absorbed will depend on the chemical structure of the compound in solution.
  • Since “white” light is a spectrum, only certain parts of the spectrum will be absorbed. The remainder produces the colour observed.
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9
Q

What is absorbance and how is it calculated?

A
  • Absorbance is calculated from intensity
  • Incident light with intensity (I0). Light reaching the detector with intensity (I)
  • Transmittance (the fraction of incident light reaching the detector):

T = I /I0

%T = I x 100 / I0

  • Relationship between concentration and transmittance is non-linear:
  • From the transmittance, one can calculate the absorbance (A)
  • Convert to absorbance which is the logarithm of the reciprocal

A = log10 1/T

A = 2 – log10 %T

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10
Q

What is the Beer-Lambert Law?

A
  • Light is absorbed when a photon collides with a molecule.
  • Therefore, it is not surprising that the amount of light absorbed depends on the concentration of the compound in solution.
  • Beer-Lambert Law: Concentration of a substance is directly proportional to the amount of light absorbed.
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11
Q

What is the equation for Beer-Lambert Law?

A

A = εcl

Where:

  • ε = molar absorptivity (molar extinction coefficient)
  • c = concentration (mol/L)
  • l = path length (cm).
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12
Q

How can molar absoptivity be used to calculate concentration?

A
  • A proportionality constant for any given compound at any given wavelength of light.

ε = A / cl

  • Since most cuvettes have a path length of 1 cm, the above equation can be simplified to:

ε = A / c

  • We can then rearrange to calculate concentration:

c = A / ε

Where:

ε = molar absorptivity (molar extinction coefficient)

c = concentration (mol/L)

  • So that concentration can be calculated from a absorbance reading if the molar absorptivity is known.
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13
Q

Why is absorbance an ideal analysis?

A
  • Measurement is quick and easy
  • (relatively) cheap
  • Readily integrated into automation
  • Reproducible
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14
Q

What is Spectrophotometry?

A
  • The quantitative measurement of the reflection or transmission properties of a material as a function of wavelength.
  • The light passing through the solution is detected by the photo-detector, generating an electrical current proportional to the intensity of the light, which is then converted into a reading.
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15
Q

What are the main types light sources of spectroscopy?

A

Need to produce light at wavelength where absorbance is measured

Tungsten

  • Covers the visible spectral range reasonably well
  • Tends to have higher intensity in the red region of the spectrum
  • Cheap

Deuterium

  • Deuterium: isotopic hydrogen (abundance ~ 1 in 6000 H atoms)
  • Deuterium arc light produces mainly UV light (so invisible to the eye)
  • Expensive
  • Relatively short lifetime
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16
Q

What is needed for optimal analytical performance in Spectrophotometry?

A
  • Incident light beam is parallel and of a constant wavelength (monochromatic)
  • Incident light beam is of the wavelength which gives the maximum absorption (minimum transmission) of the light.
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17
Q

How does spectrophotometry achieve optimal analytical performance?

A

Spectrophotometers use a prism or diffraction grating to isolate a portion of spectrum of white light from the bulb.

18
Q

What is Collimator and Monochromator?

A

Collimator

  • A lens to produce a near parallel beam of light
  • Monochromators only work if beam is collimated

Monochromator

  • Coloured filters
  • Prism
  • Diffraction grating
19
Q

What is the role of a Prism?

A
  • Light separated by refraction (bending by passing through transparent medium)
  • Target wavelength selected by rotating the prism
20
Q

What is Diffraction Grating?

A
  • Light separated by diffraction (bending of light at the edge of an opaque surface)
21
Q

What is Holmium Oxide?

A
  • Holmium (atomic mass 165) is a rare earth lanthanide element
  • It forms an oxide Ho2O3
  • This has a complex absorption spectra with sharp, well defined peaks across the UV/visible range
22
Q

What are properties of Cuvettes?

A
  • Known path length
  • Optically inert
  • No absorption in the region of interest
  • No internal reflection or scatter
  • Smooth, plain walls in optical path
23
Q

What are are types of Cuvette?

A
  • Polystyrene
  • Glass
  • Quartz
24
Q

What are the advantages and disadvantages of Polystyrene Cuvettes?

A

Advantages

  • Cheap
  • Disposable

Disadvantages

  • Strong absorbance in UV region
  • Sensitive to some organic solvents
25
Q

What are the advantages and disadvantages of Glass Cuvettes?

A

Advantages

  • Intermediate cost
  • Scratch resistant
  • Chemically resistant

Disadvantages

  • Doesn’t have full UV transparency
26
Q

What are the advantages and disadvantages of Quartz Cuvettes?

A

Advantages

  • Transparent to UV and visible wavelengths
  • Chemically resistant

Diasadvantages

  • Expensive
  • Not disposable
27
Q

What are types of detectors?

A
  • Photomultiplier tube (very high sensitivity)
  • Diode array
28
Q

What is the use of photomultiplier tube?

A

(very high sensitivity)

  • Exponentially amplify light signal
  • Cascade system of “dynodes”
  • Convert light to electron beams then to electric current
  • Relatively expensive
29
Q

What is a Diode array’s use?

A
  • Slightly different way to conventional spectrophotometers
  • The array contains several light detectors
  • Several wavelengths of light can be measured simultaneously
30
Q

What is Blanking and how is it done?

A

All components of the cuvette and contents can affect absorbance. Only the absorbance due to the substance being measured is required. Instrument must be “blanked”

How?

  • Measure the absorbance before adding the analyte
  • Measure absorbance prior to addition of reagents (if producing a coloured product)
  • Use a dual beam spectrophotometer
31
Q

What is aDual-beam spectrophotometer?

A
  • The incident beam is split by a mirror
  • Allows correction for drift and power variations in the light source
32
Q

What are different forms of spectrophotometry?

A
  • Reflectance
  • Scatter
  • Fluorescence
  • Luminometry
33
Q

What is Reflectance Spectrphotometry?

A
  • Reflectance spectrophotometry is a technique for non-invasive analysis which illuminates the surface to be analyzed with a light of a known spectrum and recording the spectral response of the surfaceof the diffuse light
  • A comparison is made with a reference surface.
  • Used in dry-reagent chemistry systems (e.g. Vitros), and in some POCT applications (e.g. bilirubinometer).
34
Q

What is immunoturbidimetry?

A
  • Antibodies bind to the analyte (usually a protein)
  • Form aggregates which scatter light
  • The amount of scatter is proportional to the amount of analyte (antigen)
  • Sensitivity is of the order of 100mg/L
  • Attaching antibodies to latex or polystyrene particles can increase analytical sensitivity.
35
Q

What are features of nephelometry?

A
  • Nephelometric assays are more sensitive (1 - 10mg/L)
  • Nephelometry needs more specialist equipment
  • Measuring light scattered at 90°
36
Q

What is Fluorescence spectrophometry?

A
  • Occurs when a molecule absorbs light at one wavelength and re-emits light at a longer wavelength.
  • Emitted light is always lost at a longer wavelength (lower energy) than the excitation light
  • Stokes shift: difference between λmax of excitation light and emitted fluorescence light.
37
Q

Where is fluorescence used in the clinical lab?

A
  • lmmunoassay detection systems: e.g. DELFIA, etc.
  • In some polarisation methods (FPIA: e.g. for TDMs)
  • FISH
  • PCR
38
Q

What are the features of using luminescence?

A
  • This is the generation of light from a chemical reaction (chemiluminescence)
  • Extremely sensitive

Siemens Centaur: acridinium ester.

Siemens Immulite platform: adamantyl dioxetane phosphate

39
Q

What are applications of luminescence?

A
  • Enzymatic reactions (e.g. glucose) – see enzymology lecture.
  • Chemical reactions (e.g. creatinine)
  • Dye binding (e.g. magnesium, calcium)
  • Transition metal complexes (e.g. phosphate)
40
Q

What are examples of luminescence molecules?

A
  • Glucose – hexokinase coupled with G6PDH with reduction of NADP
  • Creatinine – alkaline picrate (Jaffe)
  • Magnesium – xylidyl blue
  • Calcium – CPC, arsenazo
  • Phosphate – Molybdenum.