1. 1 Coherence: Spatial, Temporal Interference: Young’s Double Slit Experiment Fringes of Equal Inclination Fringes of Equal Thickness 1

2. 22 Coherence

3. 3 Concept of coherence is related to stability or predictability of phase Spatial coherence describes the correlation between signals at different points in space. Temporal coherence describes the correlation between signals at different moments of time.

4. 44 Electric field distribution around the focus of a laser beam with perfect spatial and temporal coherence. A laser beam with high spatial coherence, but poor temporal coherence. A laser beam with poor spatial coherence, but high temporal coherence.

5. 5 Many sinusoidal nearby frequencies are needed to construct the above Band of frequencies = Physically, monochromatic sources are fictitious. Quantifying Coherence Wave train

6. 6 y(t) = [Sin t + Sin(1.01 t) + Sin (1.02 t) + Sin(1.03 t) + Sin (1.04 t) + Sin (1.05 t) + Sin (1.06 t) + Sin (1.07 t) + Sin (1.08 t)]/9 0 < t < 800

7. 7 Coherence time: Coherence length: Temporal coherence: The coherence time is the time over which a propagating wave may be considered coherent. In other words, it is the time interval within which its phase is, on average, predictable. The coherence length is the coherence time times the vacuum velocity of light, and thus also characterizes the temporal (not spatial!) coherence via the propagation length (and thus propagation time) over which coherence is lost. Quantifying Coherence  : Spectral width of the source in units of frequency.

8. 8 Red Cadmium= 6438 Å = 10 9 Hz, 30 cm Yellow Sodium = 10 10 Hz, 3 cm = 5893 Å He-Ne Laser= 6328 Å 300 m = 10 6 Hz,

9. 9 A plane wave with an infinite coherence length. Since there are two transverse dimensions, we can define a coherence area (A c ).

10. 10 A wave with a varying profile (wavefront) and infinite coherence length.

11. 11 A wave with a varying profile and finite coherence length. The spatial coherence depends on the emitter size and its distance. where d is the diameter of the light source and D is the distance.

12. 12 The wave with finite coherence length is passed through a pinhole. The emerging wave has infinite coherence area. The coherence length (or coherence time) are unchanged by the pinhole.

13. Interference of water waves Interference is the effect produced by the superposition of waves from two coherent sources passing through the same region.

14. Interference of water waves Two wave sources are said to be coherent: - if the phase difference between the sources is constant, - if they have same frequency, - if the two waves have comparable amplitudes. The interference pattern produced in a ripple tank using two sources of circular waves which are in phase with each other.

15. Constructive & destructive interference The two sources S 1 and S 2 are in phase and coherent. Therefore, the wavelengths of waves from S 1 and S 2 are the same, say λ.

16. Conditions of Interference 16

17. Coherent Sources Constant phase difference Such sources may or may not be in step but are always marching together 17

18. Temporal coherence The interval over which the light wave resembles a sinusoid is the measure of its temporal coherence. Coherence Time of Radiation The average time interval during which the light wave oscillates in a predictable way is known as coherence time of radiation. 18

19. Spatial extent over which the light wave oscillates in a regular predictable way is the coherent length 19

20. Temporal Coherence 20

21. Spatial Coherence 21

22. Interference of light from two bulbs? 22

23. White Light Interference 23

24. 24 Waves of different frequencies (i.e. colors) interfere to form a pulse if they are coherent.

25. 25 Spectrally incoherent light interferes to form continuous light with a randomly varying phase and amplitude

26. Optical Interference Optical interference corresponds to the interaction of two or more light waves yielding a resultant irradiance that deviates from the sum of component irradiance. Wavefront splitting Amplitude splitting 26 Wavefront Division: Involves taking one wavefront and dividing it up into more than one wave. Eg: Young’s double slit interference; Diffraction grating Amplitude Division: Involves splitting a light beam into two beams at a surface of two media of different refractive index. Eg: Michelson interferometer

27. Light waves interfere with each other much like mechanical waves do. All interference associated with light waves arises when the electromagnetic fields that constitute the individual waves combine LINEAR SUPERPOSITION! 27

28. Resultant 28

29. Interference Animation http://www.acs.psu.edu/drussell/demos/superposition/superposition.html 29 The angular spacing of the fringes, θ f, is given by: where d is the separation between slits

30. 30

31. Irradiance 31 Strictly speaking irradiance is power/area. And intensity is power/solid angle.

32. 32

33. Interference term 33

34. 34

35. Time average gives: 35 The interference term The phase difference arising from a combined path length and initial phase difference.

36. 36

37. 37

38. Total constructive interference For maximum irradiance 38 1

39. Total destructive interference For minimum irradiance 39 1

40. Components out of phase Constructive Interference 40

41. Components 90 o out of phase 41

42. 42 Destructive Interference

43. For I 1 =I 2 43 Twin Source Interference Pattern

44. For the spherical wave emitted by two sources, in-phase at the emitter 44

45. 45

46. Photo shows an interference pattern by two holes 46

47. Interference by two plane polarized light wave For constructive interference For destructive interference 47

48. 48 Wavefront splitting Interferometer Young’s Double Slit Experiment 48

49. Wavefront splitting interferometer Young’s Double Slit Diffraction Grating Amplitude splitting interferometer Fringes of equal inclination Fringes of equal thickness 49

50. 50 Young’s Double Slit Experiment

51. 51 Young’s double slit

52. 52 Path difference:

53. 53 D

54. 54 For a bright fringe, For a dark fringe, m: any integer Path difference: http://www.acs.psu.edu/drussell/demo s/superposition/superposition.html

55. 55 Destructive interference

56. 56 Constructive Interference

57. Double slit: A closer look Curves of equal-path difference are Hyperboloids of revolution

59. http://fp.optics.arizona.edu/milster/505%20Lecture/Lecture%20Notes%20and%20Slides/Chapter%204- %20Basic%20Interference/OLD%20NOTES/Basic%20Interference%20-%20Part%20B%20.pdf

60. Transverse Section: Straight fringes

61. Longitudinal section: Circular fringes

62. Transverse section –Straight fringes S S  d P D N O x  62

63. The distance of m th bright fringe from central maxima Fringe separation/ Fringe width Path difference 63

64. Interference Animation 64 The angular spacing of the fringes, θ f, is given by: where d is the separation between slits

65. 65 For two beams of equal irradiance (I 0 )

66. 66 Visibility of the fringes (V) Maximum and adjacent minimum of the fringe system

67. 67 Photograph of real fringe pattern for Young’s double slit

68. 68 The two waves travel the same distance –Therefore, they arrive in phase S S'S'

69. 69 The upper wave travels one wavelength farther –Therefore, the waves arrive in phase S S'S'

70. 70 The upper wave travels one-half of a wavelength farther than the lower wave. This is destructive interference S S'S'

71. 71 Young’s Double Slit Experiment provides a method for measuring wavelength of the light This experiment gave the wave model of light a great deal of credibility. Uses for Young’s Double Slit Experiment

72. Longitudinal section –Circular fringes P O rnrn S S d D N  72

73. At the central spot, Path difference = d For central bright fringe: d = m o λ 73 P O rnrn S S d D N 

74. Radius of n th bright ring For small  m 74 P O rnrn S S d D N 

75. Thin mica plate Pohl’s fringesLongitudinal Section

76. 76 Fresnel double mirror P1 P2

77. 77 Fresnel biprism

78. 78 Lloyd’s mirror

79. 79 Billet’s split lens

80. 80 Wavefront splitting interferometers Young’s double slit Fresnel double mirror Fresnel double prism Lloyd’s mirror

81. 81 For a bright fringe, For a dark fringe, Extra phase difference ±  in Lloyd’s mirror

82. 82 1. Optics Author: Eugene Hecht Class no. 535 HEC/O Central library IIT KGP

83. 83 Division of Amplitude 83

84. nfnfnfnf n2n2n2n2 n1n1n1n1 B d DA C tttt iiii tttt tttt A B C D Thin Film Interference

85. Optical path difference for the first two reflected beams AC = 2d tan  t tttt tttt A B C D tttt iiii iiii

86. Path Difference

87. Phase shift (in the case of external reflection) Consider a soap film: n 1 = n 2 = n For n 1 > n f > n 2, or n 1 < n f < n 2, the ±π phase shift will not be present

88. Condition for maxima(  = 2mπ) Condition for minima(  = (2m+1)π) Note: Odd and even multiple of ( f /4)

89. -Since d is constant, the locus of each interference fringe is determined by a constant value of  which depends on a constant angle  i. -This gives circular fringe around the centre point. -An extended source produces a range of constant  values at one viewing position so the complete pattern is obviously a set of concentric fringes formed at infinity. -These are fringes of equal inclination and are called Haidinger fringes.

90. Fringes of equal inclination

91. d n2n2n2n2 n1n1n1n1 Beam splitter Extendedsource PIPIPIPI P2P2P2P2 P x f Focalplane Dielectricslab Haidinger’s Bands: Fringes of equal inclination

92. Fringes of equal thickness - Fringes observed when optical thickness n f d is dominant rather than  i. - Ex: Oil slicks - Each fringe is the locus of all points in the film for which the optical thickness is a constant. - In general n f does not vary, so the fringes correspond to regions of constant film thickness. - When the thickness d is not constant and the faces of the slab form a wedge. The interfering rays are not parallel but meet at points (real or virtual) near the wedge. - The resulting interference fringes are localized near the wedge.

93. Fizeau Fringes Extended source Beam splitter x n2n2n2n2 n n d =x   : Wedge angle

94. Wedge between two plates 1 2 glass air D t x Path difference = 2t Phase difference  = 2kt -  (phase change for 2, but not for 1) Maxima 2t = (m + ½) o /n Minima 2t = m o /n

95. Fizeau Fringes: fringes of equal thickness These are termed Fizeau fringes. Conditions for maximum (For small values of  i ) d is the thickness at a particular point d =x 

96. Consecutive fringes are separated by

97. Newton’s Ring Ray 1 undergoes a phase change of 180  on reflection, whereas ray 2 undergoes no phase change R = radius of curvature of lens x = radius of Newton’s ring

101. Reflected Newton’s Ring

103. Thin Wedge

104. Enlarged wedge

105. Colour of thin oil films

106. Thin oil film

107. Fringe system of constant inclination (Haidinger Fringe Pattern) Michelson, Fabry-Perot. (Thickness is constant, but variation of angles gives fringes of different order (m)). Fringe system of constant thickness (Fizeau Fringe pattern) Newton’s ring, Thin wedge film, Uneven thin oil film. (Variation of thickness gives fringes of different order). Order of Fringe Haidinger Pattern: (Ex: Fabry-Perot Interferometer) Central region corresponds to maximum value of m. Fizeau Pattern: (Ex: Newton’s rings) Central region corresponds to minimum value of m.