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Diffraction of Light Waves

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Title: Diffraction of Light Waves


1
Chapter 4
  • Diffraction of Light Waves

2
Diffraction
  • Huygens principle requires that the waves spread
    out after they pass through slits
  • This spreading out of light from its initial line
    of travel is called diffraction
  • In general, diffraction occurs when waves pass
    through small openings, around obstacles or by
    sharp edges

3
  • A single slit placed between a distant light
    source and a screen produces a diffraction
    pattern
  • It will have a broad, intense central band
  • The central band will be flanked by a series of
    narrower, less intense secondary bands
  • Called secondary maxima
  • The central band will also be flanked by a series
    of dark bands
  • Called minima

4
  • The results of the single slit cannot be
    explained by geometric optics
  • Geometric optics would say that light rays
    traveling in straight lines should cast a sharp
    image of the slit on the screen

5
Fraunhofer Diffraction
  • Fraunhofer Diffraction occurs when the rays leave
    the diffracting object in parallel directions
  • Screen very far from the slit
  • Converging lens (shown)
  • A bright fringe is seen along the axis (? 0)
    with alternating bright and dark fringes on each
    side

6
Single Slit Diffraction
  • According to Huygens principle, each portion of
    the slit acts as a source of waves
  • The light from one portion of the slit can
    interfere with light from another portion
  • The resultant intensity on the screen depends on
    the direction ?

7
  • All the waves that originate at the slit are in
    phase
  • Wave 1 travels farther than wave 3 by an amount
    equal to the path difference (a/2) sin ?
  • If this path difference is exactly half of a
    wavelength, the two waves cancel each other and
    destructive interference results

8
  • In general, destructive interference occurs for a
    single slit of width a when
  • sin ?dark m? / a
  • m ?1, ?2, ?3,
  • Doesnt give any information about the variations
    in intensity along the screen

9
  • The general features of the intensity
    distribution are shown
  • A broad central bright fringe is flanked by much
    weaker bright fringes alternating with dark
    fringes
  • The points of constructive interference lie
    approximately halfway between the dark fringes

10
Resolution of Single-Slitand Circular Apertures
  • The resolution is the ability of optical systems
    to distinguish between closely spaced objects,
    which are limited because of the wave nature of
    light
  • If no diffraction occurred, two distinct bright
    spots would be observed on the viewing screen.
    However, because of diffraction, each source is
    imaged as a bright central region flanked by
    weaker bright and dark bands.

11
  • If the two sources are separated enough to keep
    their central maxima from overlapping, their
    images can be distinguished and are said to be
    resolved.
  • If the sources are close together, however, the
    two central maxima overlap and the images are not
    resolved.

12
  • Rayleigh's criterion
  • To decide when two images are resolved, the
    following criterion is used
  • When the central maximum of one image falls on
    the first minimum another image, the images are
    said to be just resolved.
  • This limiting condition of resolution is known as
    Rayleigh's criterion.

13
The diffraction patterns of two point sources
(solid curves) and the resultant pattern (dashed
curves) for various angular separations of the
sources
14
  • From Rayleigh's criterion, we can determine the
    minimum angular separation, ?min , subtended by
    the sources at the slit so that their images are
    just resolved.
  • the first minimum in a single-slit diffraction
    pattern occurs at the angle for which
  • sin ? ? / a
  • where a is the width of the slit. According to
    Rayleigh's criterion, this expression gives the
    smallest angular separation for which the two
    images are resolved.

15
  • Because ? a in most situations,
  • sin ? is small and we can use the approximation
  • sin ? ? . Therefore, the limiting angle of
    resolution for a slit of width a is
  • ?min ? / a
  • where ?min is expressed in radians. Hence, the
    angle subtended by the two sources at the slit
    must be greater than ? / a if the images are to
    be resolved.

16
  • The diffraction pattern of a circular aperture
    consists of a central circular bright disk
    surrounded by progressively fainter rings. The
    limiting angle of resolution of the circular
    aperture is
  • Where D is the diameter of the aperture.

17
Diffraction Grating
  • The diffracting grating consists of many equally
    spaced parallel slits
  • A typical grating contains several thousand lines
    per centimeter
  • The intensity of the pattern on the screen is the
    result of the combined effects of interference
    and diffraction

18
Diffraction Grating
  • The condition for maxima is
  • d sin ?bright m ?
  • m 0, 1, 2,
  • The integer m is the order number of the
    diffraction pattern
  • If the incident radiation contains several
    wavelengths, each wavelength deviates through a
    specific angle

19
  • All the wavelengths are focused at m 0
  • This is called the zeroth order maximum
  • The first order maximum corresponds to m 1
  • Note the sharpness of the principle maxima and
    the broad range of the dark area
  • This is in contrast to the broad, bright fringes
    characteristic of the two-slit interference
    pattern

20
diffraction grating spectrometer.
  • The collimated
  • beam incident
  • on the grating is
  • spread into its
  • various wavelength
  • components with
  • constructive interference for a particular
    wavelength occurring at the angles that satisfy
    the equation

21
Resolving power of the diffraction grating
  • The diffraction grating is useful for measuring
    wavelengths accurately.
  • Like the prism, the diffraction grating can be
    used to disperse a spectrum into its components.
  • Of the two devices, the grating may be more
    precise if one wants to distinguish between two
    closely spaced wavelengths.

22
  • If ?1 and ?2 are the two nearly equal
    wavelengths between which the spectrometer can
    barely distinguish, the resolving power R is
    defined as
  • where ? ( ?1 ?2 ) / 2 , and
  • ? ? ?2 - ?1
  • a grating that has a high resolving power can
    distinguish small differences in wavelength.

23
  • if N lines of the grating are illuminated, it can
    be shown that the resolving power in the mth
    order diffraction equals the product N m
  • R N m
  • Thus, resolving power increases with increasing
    order number.
  • R is large for a grating that has a large number
    of illuminated slits.

24
  • Consider the second-order diffraction pattern (m
    2) of a grating that has 5000 rulings
    illuminated by the light source.
  • The resolving power of such a grating in second
    order is R 5000 x 2 10,000.
  • The minimum wavelength separation between two
    spectral lines that can be just resolved,
    assuming a mean wavelength of 600 nm, is
  • ?? ? / R 6.00 X 10-2 nm.
  • For the third-order principal maximum,
  • R 15 000 and ?? 4.00 x 2 nm, and so on.
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