Refraction, Diffraction and Interference

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Cards (20)

  • all waves diffract
  • the amount of diffraction depends on the wavelength of the wave compared to the size of the gap
    • when the gap is bigger than the wavelength, diffraction is unnoticeable
    • when the gap is several wavelengths wide, you get noticeable diffraction
    • you get the most diffraction when the gap is the same size as the wavelength
    • if the gap is smaller than the wavelength then the waves are mostly reflected back
  • to observe a diffraction pattern
    • monochromatic, coherent light source (such as a laser)
    • if the wavelength is around the same size as the aperture then you get a diffraction pattern
    • fringes are caused by destructive and constructive interference of light waves
  • diffracted white light creates a spectra of colours
    since white light is a mix of different wavelengths of light
    • the different wavelengths are diffracted by different amounts
    • this gives you a spectra of colours
  • increasing the slit width decreases the amount of diffraction
    • the central maximum is narrower
    • its intensity is higher
  • increasing the wavelength increases the amount of diffraction
    • the central maximum is wider
    • its intensity is lower
  • interference patterns become sharper with more slits
    diffracted light intensity is more intense
    because there are lots of different beams reinforcing the pattern, making for more accurate measurements
  • for monochromatic light, all the maxima are sharp lines
    • there is a line of maximum brightness in the centre called the zero order line
    • for a grating with slits a distance of d apart (d=1/ the number of slits per metre), the angle between the incident beam and the nth order maximum is dsinθ=d\sin\theta=nλn\lambda
  • diffraction gratings help to identify elements and calculate atomic spacing by using X-ray crystallography
    • the wavelength of X-rays are of a similar wavelength to the atom spacings in crystalline solids
    • the crystal acts as a diffraction grating, causing the X-rays to form a diffraction pattern
  • light is fastest in a vacuum. it slows down in other materials because it interacts with the particles in them. the more optically dense a material is, the more light slows down when it passes through
  • absolute refractive index of a material
    n=n=c÷csc\div c_{s}
    the absolute refractive index is a property of THAT MATERIAL ONLY
    the relative refractive index is a property of the interface BETWEEN TWO MATERIALS
  • optical fibres use total internal reflection
    • thin flexible tube of glass or plastic fibre that can carry light signals over long distances and around corners
    • step-index optical fibres have a high refractive index but are surrounded by cladding with a lower refractive index to allow total internal reflection (also protects from scratches which could cause light to escape)
    • all of the light is totally internally reflected from boundary to boundary until it reaches the other end
  • a signal travelling down an optical fibre can be degraded by absorption or dispersion. signal degradation can cause information to be lost
  • absorption causes loss in amplitude
    • as the signal travels, some of its energy is lost through absorption by the material that the fibre is made from
    • this energy loss results in the amplitude of the signal being reduced
  • there are two types of dispersion
    • modal dispersion is when the light rays enter at different angles and so take different paths. a single-mode fibre only allows for one path and stop this
    • material dispersion - some wavelengths of the light will reach the end faster. using monochromatic light can stop this.
    • dispersion causes pulse broadening which can overlap and confuse the signal
  • an optical fibre repeater can be used to boost and regenerate the signal every once in a while which can reduce signal degradation caused by both absorption and dispersion
  • the angle of incidence is between the normal to the boundary and the ray of light arriving at the boundary