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Wavelength
Distance between 2 peaks, variable
Electromagnetic spectrum
Continuum of waves at different wavelengths,
Absorption
Interaction of electromagnetic field with mater, transfer of energy carried by photons to molecules that absorb a
Photon
Elementary particle, carries electromagnetic radiation
Energy of photons (E)
E=hc/lambda, h=planks constant, c=speed of light, lambda=wavelength of light carrying it, inversely proportional to wavelength
Absorption
Photon strikes molecule and is absorbed (energy photon=energy difference between energy levels), electron in ground state is excited into higher energy state, very quick (10^-15), remains for short time before return to ground (release energy)
Consider when detection of absorption
light source, select wavelength, direct and control shining, measuring the light, quantifying
Spectrophotometers key elements
Light source, Monochromator and slits, Cuvettes and cuvette holders, Dectectors
Light source depends
wavelength, consistency of intensity, durability and cost
Light source examples
Halogen (350-2500), Deuterium (<200-400), Xenon arc (<200-1100)
Monochromator
Separate light into different distinct wavelengths, primarily prisms or grating
Coloured filter
Mostly in fluorescence, selected for light using colorimetry
Slits
Select for particular wavelength, allows selective passage of light in wavelength
Cuvettes
1 or 3mL, path length typically 1cm, different materials for different wavelengths,
Cuvettes material
Polystyrene (325-750), PMMA (245-750), Quartz (170-2500)
Micro volume spectrophotometer
Small volumes (1-2.5 uL), use fiber optical cable to detect
Plate reader
Multiple samples, hold <150uL
Detectors
Gather and quantify intensity or wavelength reaching it
Blanks
Reference solution, same component as sample minus analyte
Dual beam spectrophotometer
Measure amount of light through blank and analyte simultaneously, split light into 2 beams, more expensive
Single beam spectrophotometer
Do not split light beam
Incident light (Io)
Intensity of light reaching detector during blank
I
Intensity of light reaching detector with analyte
Absorbance equation
A= log (Io/I)
Absorbance
Quantification of absorption process
Beer Lamber law considerations(3)
Wavelength used, thickness absorbing material, concentration absorbing material
Beer lambert law
A=Elc, A=absorbance, E=molar absorption coefficient(1/M*cm), l=path length(cm), c= concentration analyte(M)
Molar absorption coefficient
Constant of substance at particular wavelength, units 1/M*cm
Calibration curve
Graph that depicts response to some analyte under known conditions, relationship between [] and signal for instrument (absorbance proportional to concentration)
Absorption spectra
Graph, Absorption of light for molecules over broad range of wavelengths, peaks=elevated absorption
Lambda max
Wavelength at which highest absorption occurs
Chromophores
Structure in molecules that absorb light, tend to have conjugated double bonds,
Protein chromophores
Peptide bonds(lambda at 190), only aromatic side chains absorb (Trp/Tyr at 280), some have prose this groups or coenzymes (hemes)
Intrinsic absorption
Efficient absorption of Trp and Tyr for quantification
Hemes
In FAD and NADH, found oxygen transporting molecules or redox reactions
Nucleotides and nucleic acids
Aromatic rings absorbs at 260, quantitation of in solution, monitor change in secondary and tertiary structure
Light absorbing molecules
Proteins, nucleic acids, plants pigments (beta carotene)
Factors affecting absorption (4)
Solvents, Protonation, Redox state, Interaction effects
Solvents affects on absorption
Influence stability electronic states
Protonation affect on Absorbance
Affect absorption in certain regions (2nd peaks)
Redox states affect on Absorbance
Absorbance spectrum change depending redox state, increase sensitivity spectrophotometer to redox states
Interaction effects affect of Absorbance
Absorbance can change when interacting with other molecules (ex: dsDNA vs ssDNA), hyperchromicity
Fluorescence
Only when molecule is excited, measure photon release when falls back to ground state (less energy)
Fluorescence steps
Excitation- absorption of photons, internal relation in excited states (lose some energy), Emission-excited electron falls back to ground releasing photon
Stokes shift
Shift to higher wavelength when photon realized (less energy)
Sensitivity of fluorescence
Detect individual photons
Limitations of fluorescence
Scarcity of fluorescent. Molecules, Artefacts (probes attached), Photobleaching (lose fluorescence after continuous excitation), Toxic effects (kills cells), cost (more expensive)