Light Scattering - PowerPoint PPT Presentation

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Light Scattering

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Refractive index is a weak function of wavelength. How does light interact with objects? ... Shine light source though solutions in a dark room ... – PowerPoint PPT presentation

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Title: Light Scattering


1
Light Scattering
  • Rayleigh Scattering Mie Scattering

2
Theory
  • Characteristics of Polystyrene and Sulphur
    Nanoparticles.
  • -- Non absorbing
  • -- Refractive index is a weak function of
    wavelength.
  • How does light interact with objects?
  • -- Reflection (light deviated from its original
    path)
  • -- Refraction
  • -- Diffraction
  • -- Absorption (light absorbed and converted to
    heat)

3
Theory Cont
  • A collimated light source is the most basic tool
    for nanoparticle work. Often called a Tyndall
    beam.
  • The Tyndall effect is the scattered path of light
    observed in the suspension. Examples Milk,
    smoke, Lake Thunderbird.
  • Scattering Plane
  • -- The scattering plane is defined by the two
    rays involved, the source-particle ray and the
    particle-observer ray.
  • -- The scattering plane is determined by
    observation, it is not fixed in space. For
    example, if the observer moves, the scattering
    plane will move with the observer.

4
Theory Cont.
  • Theory of Rayleigh
  • -- Particles are treated as electric dipole.
  • Results
  • -- I ?1/ ?4 (only true if the refractive index
    is a weak function of ?, i.e. not a metal.)
  • -- I ?r6
  • -- scattered light at 90 is linearly polarized
    perpendicular to the scattering plane.

Horizontal Source Polarization
Verticle Source Polarization
5
Theory Cont
  • Mie Scattering
  • -- Absorption and Scattering by a Sphere.
  • -- Multipole expansion (EM modes of a sphere)
  • -- electric dipole.
  • -- magnetic dipole, electric quadrupole.
  • -- magnetic quadrupole, electric octupole.
  • If d lt ?/20 then only the first term (dipole) is
    needed. In this limiting case, Mies theory
    reduces to Rayleighs theory.
  • Efficiency factors Qsca, Qabs, Qext
  • Plot Qext vs ? for the extinction spectra
  • Qsca and Qabs vs ? show their contribution to
    Qext.
  • Intensity for perpendicular and parallel
    polarized light
  • Plot I vs ? for the angular intensity dependence
    for each polarization.

6
Objective
  • Learn about Scattering plane
  • The Polarization of Rayleigh Scattering
  • Mie Scattering
  • Angular Dependence

7
Procedure
  • Rayleigh scattering
  • Using a light source and polarization lens we
    observed the way light rays are polarized through
    rayleigh scattering in different solutions
    Silica SOL, Sulfur SOL and Fine Sulfur particles,
    by shining the light source through the solutions
  • Shine light source though solutions in a dark
    room
  • Place polarized lens in path of light source to
    observe polarization effects of scattered light
    in the scattering plane and outside of scattering
    plane, I.E. view from top (90 degrees) and other
    angles of observation

8
Higher Order Tyndall Spectra (HOTS)
  • Using the same procedure to observe the Rayleigh
    scattering effects, observe the different colors
    associated with the scattered light and observe
    angle dependency
  • Note the number of orders in each sample, one
    order is one color change from red to green

9
Scattering Angle
  • Using the Helium Neon laser apparatus (wavelength
    543.5 mm) the laser beam was shone through our
    samples of polystyrene latex
  • The samples were placed at an angle on the
    observation stage to avoid multiple reflection of
    the laser beam in the same area of the solution
  • Note the minimum intensity zones in the scattered
    light by observing in the horizontal plane and
    recording the angle these minima occur. This was
    done by observing from about 35 degrees to 145
    degrees from the laser beam in the scattering
    plane. See picture

Laser
Sample
Observation stage with angle measurement site
10
Optical Microscopy
  • Using an optical microscope in dark field
    observation mode, observe the nanoparticles in
    each of the three samples
  • Note their movement and size (each sample
    resembles a night sky filled with stars, the
    particles can be seen but not studied in detail)

11
(No Transcript)
12
Results Rayleigh Scattering
  • Silica SOL
  • With the vertical polarization lens in place we
    noticed there is no angular dependence in the
    scattering plane
  • By using a second polarization lens at a 90
    degree angle we verified that the light is
    polarized perpendicular to the scattering plane
  • Sulphur SOL
  • Using the same techniques we noted the HOTS
    followed slightly different result patterns,
    there was significantly more forward scattering
    which caused the scattered light to blend
    together and appear simply white toward larger
    scattering angles in the scattering plane
  • Polystyrene latex
  • By observing each of the three samples and noting
    their order using the HOTS phenomenon we ranked
    the sample by particle size from smallest to
    largest as follows Sample C, Sample B, Sample A
    (This initial ranking seemed to be correct
    according to our scattering angle experiment
    data)

13
Observation
Sample Gaurav Trevor Ye
A 50 49 85
74 73 98
98 100 105
124
B 54 54 50
96 96 98
C 141 141 141
14
Results Scattering Angle
  • Sample C
  • No minimum were found in this sample although the
    intensity significantly decreased as the viewing
    angle decreased, this result is consistant with
    the Mie plot data
  • Estimated particle size ?lt240 nm
  • Sample B
  • Minima recorded at scattering angles of 54 and 96
    degrees
  • Estimated particle size ? 600nm
  • Sample A
  • Minima recorded at 50, 74 and 98 degrees
  • Estimated particle size ? 1060 nm

15
Mie plot results
Sample C Particle size lt 240nm
Sample A Particle size 1060nm
50
Intensity decreases as angle increases
74
98
Sample B Particle size 600nm
54
96
16
Experiment discussion
  • Experimentally determined particle size
  • Sample A Particle size ? 1060 nm
  • Sample B Particle size ? 600 nm
  • Sample C Particle size ? lt 240 nm
  • Error and procedure improvement suggestions
  • Lab results were recorded by human observation of
    three different lab technicians, humans always
    make mistakes
  • These results could be improved my taking more
    measurements and averaging results
  • Mono-dispersed vs. Poly-dispersed HOTS
  • A more highly dispersed sample would appear more
    milky under observation, that is to say the
    light spectrum would be blended together and
    appear more like white light instead a showing
    distinct wavelengths
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