Light Absorption + Emission Flashcards

1
Q

Light scattering (Rayleigh and ​Mie).

A
  • Lights scattering happens when EM waves encounter particles in air, Light waves cause a dipole moment, so electrons in atom vibrate, Cause them to emit light
  • Rayleigh: Depends on wavelength (blue scattered more), When spacing is larger than wavelength there is no interference. Intensity of incident light = intensity of scattered light
  • Mie: All wavelengths scatter equally, producing white light, when size of particle is on order of wavelength.
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2
Q

The Beer-Lambert law.

A

In dilute solution, if solvent doesn’t absorb in applied wavelength, absorption coefficient is proportional to concentration of solute. (Formula)

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3
Q

Properties of the absorption spectrum.

A
  • Absorbance or transmittance (photon goes through something) as a function of wavelength
  • Can be used to identify an element
  • Absorption requires excitation of electron
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4
Q

Turbidimetry and nephelometry.

A
  • Turbidemitry: Involved with measuring the amount of transmitted light, and calculating absorbed light by particles in suspension to determine conc. Of a substance.
  • Nephelometry: At low intensity, measures scattered light. Proportional to conc. Amount of scattered light is much greater than transmitted, this method offers a higher sensitivity than turbidimetry.
  • Both Dependent on: Number of particles, Size of particles.
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5
Q

Dynamic light scattering

A
  • Method of analyzing solutions where hydrostatic diameter of particle can be measured.
  • Light directed through sample —> Scattering occurs —> light intensity detected on other side —> intensity changes when particles in solution diffuse (brownian motion) —> speed of change depends on size of molecules —> information about intensity used to calculate diffusion coefficient.
    Formula: D= k*t/6pinr
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6
Q

Measurement of the absorption spectrum.

A
  • Absorbance vs wavelength of incident light.
  • Absorption maxima
  • Incident light must be at certain frequency
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7
Q

Energy levels of atoms and molecules: the Jablonski diagram

A

(Diagram)
Kasha’s rule when electron goes to closest energy level (internal conversion)
And intersystem crossing when going to Triplet or “Forbidden state”

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8
Q

Thermal radiation

A
  • Transfer of heat using EM radiation
  • Possible even in Vacuum
  • Everything over 0K radiates thermal radiation
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9
Q

Planck’s radiation law

A
  • Studied emission spectrum of black bodies
  • Energy emitted resulted from vibration of atoms within the material
  • Vibrational energies have discrete values, 1, 2, 3 , never in between.
  • E2 - E1 = e = hf
  • 6.626 x 10^-34
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10
Q

Light sources based on thermal radiation

A
  • Sun, lightbulbs, heated metal.
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11
Q

Absolute black body

A
  • Ideal, theoretical body which absorbs all radiation incident on it and reemits it.
  • Model can be created from closed metal cavity with hole drilled so radiation entering can not easily escape, so absorbed completely.
  • Stefan-Boltzmann law describes that emittance of a black body is proportional to the fourth power of the temperature. M black = o T4
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12
Q

Emission spectrum of the absolute black body.

A
  • Emission is in all wavelength spectrum
  • Wien’s law: Maximum radiation is in wavelength that is inversely proportional to temperature.
  • At low temp, black body is dark, most energy radiated is infra-red
  • When temp increases it glows red first, then yellow, then white/blue.
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13
Q

Medical applications of thermal radiation

A
  • Thermography: Test using infrared camera to detect heat patterns and blood flow in body tissues. DITI is the type of thermography used to diagnose breast cancer. (Thermotropic crystals used)
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14
Q

Kirchhoff’s law

A
  • A body which radiates more thermal energy also absorbs thermal energy to a higher extent.
  • Ratio between radiant emittance and absorption coefficient is constant with a narrow wavelength range.
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15
Q

The Stefan-Boltzmann law.

A

Describes that the emittance of a black body is proportional to the 4th power of the temperature.
M black = o T^4

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16
Q

Wien’s displacement law

A
  • The black body radiation curve for different temp peaks at a wavelength inversely proportional to the temperature.
17
Q

Luminescence: excitation and relaxation.

A
  • Emission of excess energy from excited electrons in form of light.
  • Types of excitation: Thermo, bio, photo electro.
  • Process: Absorption of external energy causes excitation and emission of energy in the form of light.
  • Types of relaxation: Fluorescence, Phosphorescence
18
Q

Kasha’s rule

A
  • The excited molecule first reaches the lowest vibrational level S1
  • Internal conversion
  • Photon emission occurs going to ground state.
19
Q

Fluorescence

A
  • If the luminescence stops as excitation stops
20
Q

Phosphorescence

A
  • During transition from triplet state to ground state
  • Slower luminescence than fluorescence.
21
Q

Luminescence spectra

A
  • Atoms: Line spectra (Medium pressure Hg lamp)
  • Molecules: Band spectrum, (High pressure Hg lamp)
22
Q

Stokes-shift

A

Shift difference between peak absorption and peak emission due to loss of energy in the form of heat.

23
Q

The fluorescence spectrometer

A

Device which shines light through a sample, measuring excitation spectrum and resulting emission spectrum.
- Parts: Xe lamps, Excitation monochromator, sample cell, emission monochromator, photon detector.

24
Q

(FRET) Fluorescence Resonance Energy transfer

A

Energy transfers from donor molecules without emission, to acceptor molecules when they form dipole-dipole interactions.
1) They have to be in the right orientation
2) They have to be really close
3) Spectral overlap between donor and acceptor
Applied to protein-protein interactions

25
Q

Fl​uorescence ​Re​covery after ​photobleaching (FRAP)

A
  • Used to study diffusion of molecules on the lipid membrane.
  • Limited cycles of excitation and emission for fluorescent molecules, so they can be bleached.
  • When previously bleached area of membrane recovers, this is proof of lateral diffusion.
26
Q

Notable transitions of luminescence: vibrational relaxation, intersystem crossing.

A
  • Vibrational relaxation: Internal conversion. Kasha’s rule states an excited molecule will first reach lowest vibrational level of S1 by vibration and rotation losing energy as heat.
  • Intersystem crossing: Occurs in phosphorescence, a process in which electron transition occurs between the singlet (S1) and the triplet state (T1)
27
Q

Quantum yield of luminescence.

A

Measure of the efficiency of photon emission through fluorescence, which is the loss of energy by a substance that has absorbed light via emission of a photon.
Quantum yield = N. Of photons emitted / N. Of photons absorbed

28
Q

Luminescence lifetime.

A

Inverse of rates of all transitions
N = No e^t/lifetime

29
Q

Laser: induced emission.

A
  • Process where emission is stimulated by incoming photon (incoming photon is amplified)
  • Laser materials, there are 3 energy levels, and one should be long lifetime.
  • Emission from level is achieved only by induced emission.
30
Q

Laser: the optical resonator.

A
  • Tube with 2 mirrors on both sides to reflect light emitted by laser material to amplify it.
  • One mirror allows 1% of light through, this will be utilized.
  • Condition for resonator is that wavelength must return in same wavelength.
  • 2L = m*wavelength
31
Q

Laser: population inversion.

A
  • Process where exerting energy on system the electrons are pumped from their ground state, and most molecules are excited (Until induced emission is formed)
32
Q

Types of lasers.

A
  • CO2 Laser: Surgery
  • Krypton Laser: Opthalmology
  • Ruby laser: Dermatology
  • Solid state, Gas, Dye lasers
33
Q

Properties of laser light

A
  • Monochromatic
  • Coherent (Due to induced emission)
  • Small divergence (near to parallel)
  • High intensity (beam focusing)
  • Often polarized
34
Q

Applications of lasers.

A
  • Surgery (CO2)
  • Photodynamic diagnosis and therapy: fluorophores inserted into body, causing tumor cells to fluoresce. Laser beams directed at that area cause free radicals which kill tumor cells.