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^Resolving power of optical instruments

^Resolving power of optical instruments

Suppose a convex lens is used to form the image of an object. Consider a parallel beam of light falling on it. If the lens is well corrected for aberrations, then geometrical optics tells us that the beam will get focused to a point, producing a sharp image point. However, because of diffraction, the beam instead of getting focused to a point gets focused to a spot of finite area in the form of alternate bright & dark concentric circles around a central bright disc as shown in figure. This spot is called the diffraction pattern.

A detailed analysis shows that the radius of the central bright region is approximately given by,

Thus the conclusion is a parallel beam of light incident on a convex lens gets focused to a spot of radius,   because of diffraction effects.  Where f is the focal length of the lens and 2 a (= d) is the diameter of the circular aperture or the diameter of the lens.

^Resnel’s distance (DF)

^Resnel’s distance (DF)

The distance of the screen from the slit at which the diffraction spread of a beam is equal to the size of the aperture of the slit is called Fresnel’s distance. i.e., when y = d, D = DF, thus  

For a given value of d the quantity  is called the size of Fresnel zone and is denoted by dF.

Geometrical optics or ray optics is based upon the rectilinear propagation of light. If D < DF, then there will not be too much broadening by diffraction i.e., the light will travel along straight lines and the concepts of ray optics will be valid.

^Diffraction spread

^Diffraction spread

From the above discussion it is clear that a parallel beam of light of wavelength λ on passing through an aperture of size d gets diffracted into a beam of angular width,

If a screen is placed at distance D, this beam spreads over a linear width,

If the diffraction spread y is small, only then the concept of ray optics will be valid.

^Intensity of fringes

^Intensity of fringes

Intensity of fringes at point P is

Here I0 is the intensity of central maxima. For nth secondary maxima,

From above points we have the following plot.

Also using the relation of intensity we can say

  • Maximum intensity is central maxima.
  • Most of the light is diffracted between the two first order minima.
  • The intensities of secondary maxima relating to the intensity of central maximum are in ratio,
  • The intensity of the first secondary maximum is just 36 % of that of the central maximum.
  • As the width of a secondary maximum thus as the slit width is increased, the secondary maxima get narrower. If the slit is sufficiently wide, the secondary maxima disappear and only the central maximum is obtained which is the sharp image of the slit and not a diffraction, thus a distinct diffraction pattern is possible only if the slit is very narrow.

^Position of maxima

^Position of maxima

Also it is found that at P for nth maxima

In a similar way the angular position of nth bright fringe is

i.e. angular positions of 1st, 2nd, 3rd maxima are

From above relation we can say that each secondary maxima occupies an angular width of , thus linear width of each secondary maxima is . As the central maxima is a spread between the angular positions to , thus its angular width is i.e. central maxima is twice wider than secondary maxima. Linear width of central maxi. is 

^Position of minima

^Position of minima

Path difference between the wavefronts reaching P from the end of the slits B & A is, x or p = BP – AP = AN Also p = d sinθ =

A detailed mathematical analysis shows that at P for nth minima p = d sinθ = nl, n = ± 1, ± 2, ± 3, _ _ _

For small θ, sinθ » θ

Thus angular position of nth dark fringe is

i.e. angular positions of 1st, 2nd, 3rd minima are

^Diffraction & Huygens’ theory

^Diffraction & Huygens’ theory

Diffraction can be explained using Huygens’ theory. According to this theory all parts of the slit AB will become source of secondary wavelets, which all start in the same phase at that position. The wavefronts from any two corresponding points such as (1, 13), (2, 12), (3, 11) etc. from the two halves of the slit travel identical distances to reach O thus have zero path difference, hence they add constructively to produce a bright fringe at point O, centre called central maxima or central bright fringe.

 

^Diffraction of light

^Diffraction of light

When a wave (light or sound) strikes an obstacle it doesn’t go straight, rather it bends round the obstacle.

Also when a light wave passing from a narrow slit of width AB = d reaches screen placed at a distance D (>>d) from the slit, (Fig. A) then a bright spot on screen at a point just opposite to slit is expected & all other points on the screen are expected to be dark (called regions of geometrical shadow), but in actual practice light spreads into the region of geometrical shadow and alternate patterns of bright & dark bands (Fig. B) of varying intensity are formed.

This phenomena of spreading or bending is called diffraction of wave.

a) Diffraction dominates for longer wavelengths.

b) If the wavelength of the wave is smaller than the dimensions of obstacle diffraction is negligible & the wave behaves like a ray & travels along straight line (called, rectilinear propagation).

c) Diffraction in case of radio waves & sound waves is generally observed, because their wave length is not so small & obstacles/ apertures of theses sizes are readily available.

d) Diffraction with light is generally not observed, because light has very small wavelength (»mm) & obstacles of such small size are readily not available.

^Young’s double slit experiment

^Young’s double slit experiment

A common experiment to study interference of two light waves is YDSE. In this experiment overlapping of wave fronts of light waves coming from two slits S1 & S2 is studied by placing a screen at some distance from the slits. Let slits are separated by a distance ‘d’ & screen is situated ‘D >>d’ distance away from slits. Wavefronts reaching O from S1 & S2 are of equal path length produce no phase difference & thus we get maximum intensity at O (called central maxima, CM).

If the overlapping of waves is studied at a point P situated ‘y’ distance above or below the central maxima, then the intensity of the resultant wave depends on the phase difference between the waves S2P & S1P. If point P is situated ‘y’ distance above point ‘O’, then the path S2P is longer than S1P by an amount d sinθ. As here d << D, thus

thus path difference (p or Δx or simply x) can be expressed as

Phase & path difference for a sinusoidal wave are related as

Using above relation for conditions of maximum intensity we can say that maximum intensity is achieved at following positions from  central maxima

Using above relation for conditions of minimum intensity we can say that minimum intensity is achieved at following positions from  central maxima

For two waves of equal intensities the intensity of the resultant wave varies as square of the cos of Φ/2 i.e.

Here 4a2 is the maximum intensity of the resultant wave at central maxima.

Facts

1. Fringe width of any dark or bright fringe is same & is

2. When interference is studied with white light, each of the seven colours produces its own fringe pattern, having different fringe width & due to overlapping blurred fringes are observed. However central fringe is white, on either side the nearest fringe is blue and farthest fringe is red & then uniform illumination.

3. If a transparent sheet of thickness ‘t’ & refractive index ‘m’ is introduced in one of paths of interfering waves, the entire fringe pattern displaces towards the side in which the sheet is inserted by a distance   without any change in the fringe.

Also no. of fringes shifted is

^Geometrical optics

^Geometrical optics

Geometrical optics is also called ray optics. It treats propagation of light in terms of rays and is valid only if wavelength of light is much lesser than the size of obstacles. It deals with the following phenomena

  1. rectilinear propagation (i.e. light propagates in a straight line, due to its small wavelength)
  2. reflection (i.e. coming back in same medium on striking a shining surface)
  3. refraction (i.e. change of speed on changing transparent medium)
  4. dispersion (i.e. light splits up in to its constituent colours on changing transparent medium)
  5. image formation ( i.e. intersection of two or light rays after undergoing reflection or refraction).
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