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Interference and Diffraction

Interference and Diffraction. Chs 37 and 38. Huygen’s Principle. Any wave (including electromagnetic waves) is able to propagate because the wave here affects nearby points there In a sense, the wave is the source for more of the wave

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Interference and Diffraction

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  1. Interference and Diffraction Chs 37 and 38 Huygen’s Principle • Any wave (including electromagnetic waves) is able to propagate because the wave here affects nearby points there • In a sense, the wave is the source for more of the wave • A wave here creates waves in all the forward directions • For a plane wave, the generated waves add up to make more plane waves • Mathematically, this works, but for plane waves, no one does it this way

  2. Diffraction Through a Tiny Hole r • The waves come out in all directions • It is only because the whole wave makes new waves that the waves add up to only go forwards • What if we let the wave pass through a tiny hole? • Smaller than a wavelength • Only one point acts as source • Waves spread out in all directions • What’s interesting is that oscillations depend on distance from slit Diffraction is bending

  3. Ans E

  4. Interference Through Two Slits • Now imagine we have two slits, equally sized • Each slit creates its own waves • In some directions, crests add with crests to make bigger “brighter” crests • In others, crests combine with troughs to make minimum areas • In the end, what you get is a pattern of alternating light and dark bands • We’re about to need an obscure math identity:

  5. Two Slit Interference d  r2 r1 • What do the EM waves look like far away? • Let the separation of the slits be d • Let’s find total E-field at point P d sin P

  6. Two Slit Interference (2) • Where is it bright? • Where is it dark?

  7. Ans E

  8. Solve on Board

  9. Phases • When you combine two (or more) waves, you need to know the phase shift between them: • The angle is the phase shift • When the phase shift is zero, the waves add constructively • The result is bigger • Same thing for any even multiple of  • When the phase shift is , the waves add destructively • The result is smaller • Same thing for any odd multiple of  • To find maximum/minimum effects, set phase shift to even/odd multiples of 

  10. Phase Shift From Traveling 1 m • As a wave passes through any material, its phase shifts • For a distance d, we have: • Recall, wavelength  changes inside a material Light of wavelength 0.5 m takes two paths, both of length 1 m, one through air, the other through glass (n = 1.5). What is the difference in phase between the two waves in the end? A) 0 B)  C) 2 D) 3 E) None of the above

  11. Solve on board

  12. Four Slit Interference • What if we have more than two slits? • Four slits, each spaced distance d apart • Treat it as two double slits r3,4 r1,2 P • For four slits, every third band is bright

  13. More Slits and Diffraction gratings N = 8N = 16N = 32 • This process can be continued for more slits • For N slits, every N – 1’th band is bright • For large N, bands become very narrow • A device called a diffraction grating is just transparent with closely spaced regular lines on it • You already used it in lab • Diffraction gratings are another way to divide light into different colors • More accurate way of measuring wavelength than a prism • Commonly used by scientists

  14. Ans D

  15. Resolution of Diffraction Gratings • Note that the angle depends on the wavelength • With a finite number of slits, nearby wavelengthsmay overlap • The width of the peaks is about • The difference between peaks is • We can distinguish two peaks if: N = 8 1.1 • This quantity (mN) is called the resolving power • Even if N is very large, effectively N is how many slits the light beam actually falls on

  16. Diffraction through a single slit x a r rave • What if our slit is NOT small compared to a wavelength? • Treat it as a large number of closely spaced sources, by Huygen’s principle • Let the slit size be a, and rave the distance to the center • Let x be the distance of some point from the center • The distance r will be slightly different from here to P P

  17. Diffraction through a single slit (2) • Very similar to equation for multi-slit diffraction, but . . . • a is the size of the slit • This equation is for dark, not light • Note m= 0 is missing • Central peak twice as wide

  18. Solve on board

  19. If you used a little wider slit, the pattern would A) Get wider and dimmer B) Get wider and brighter C) Get narrower and dimmer D) Get narrower and brighter

  20. Screens and Small Angles x L • Usually your slit size/separation is large compared to the wavelength • Multi-slit: Diffraction: • When you project them onto a screen, you need to calculate locations of these bright/dark lines • For small angles, sin and tan are the same

  21. Diffraction and Interference Together a = d/5 • Now go through two finite sized slits • Result is simply sum of each slit • Resulting amplitude looks like: a d a • Resulting pattern has two kinds of variations: • Fast fluctuations from separation d • Slow fluctuations from slit size a

  22. Diffraction Limit: a a D • When light goes through a “small” slit, its direction gets changed • Can’t determine direction better than this • If we put light through rectangular (square) hole,we get diffraction in both dimensions • A circular hole of diameter D is a trifle smaller, which causes a bit more spread in the outgoing wave • For homework, use this formula; for tests, the approximate formula is good enough

  23. Ans D

  24. Diffraction Limit (2) If the pupil of your eye in good light is 2 mm in diameter, what’s the smallest angle you can see using 500 nm visible light? • A degree is 1/360 of a circle, an arc-minute is 1/60 of a degree, an arc-second is 1/60 of an arc minute • Telescopes require large apertures to see small angles

  25. Reflection and Phase Shift  phase shift  phase shift 0 phase shift • When you reflect off of a mirror, the reflected wave must cancel the incoming wave • It has a  phase shift • When you go from a low index of refraction medium to a high one, some of the wave is reflected • It also has a  phase shift • When you go from a high index of refraction medium to a low one, some of the wave is reflected • This has a 0 phase shift

  26. Concept Question Suppose we are in a glass medium, and we have a wave that goes from glass to air to glass. If the layer of air is much smaller than one wavelength, then the two reflected waves will add A) Constructively B) Destructively C) Insufficient Info • First transition: high to low • no phase shift • Second transition: low to high •  phase shift • Compared to each other, the two waves are  out of phase with each other • They will have a tendency to cancel • Very little effect from layer if thinner than a wavelength

  27. Interference from Thin Films • Suppose we go through a thin soap film • Index goes up then down • Front surface: • Phase shift of  from reflection (low-high) • Back surface: • Phase shift of 2t/ from traveling • Phase shift of 0 from reflection • Phase shift of 2t/ from traveling • Total phase shift between two reflected waves: • Weak reflection when odd times : • Strong reflection when even • Same results for index down then up • Opposite for: • Index up, then up • Index down, then down t

  28. Applications of Thin Film Interference narrow air gap • What if the light isn’t monochromatic? • Some wavelengths are enhanced, others are not • Soap bubbles • Oil on water • Newton’s rings: convex lens on flat glass plate • Air gap changes thickness in circular pattern • Alternating light/dark regions d

  29. Solve on Board

  30. Michelson Interferometer • Hanford, Washington • Interference easy to measure • Can see much smaller than one wavelength • LIGO, state of the art, can see 10-15 m! Mirrors Laser Detector

  31. Crystal Scattering of X-rays • Mysterious rays were discovered by Röntgen in 1895 • Suspected to be short-wavelength EM waves • Order 1-0.1 nm wavelength • Scattered very weakly off of atoms • Bragg, 1912, measured wavelength accurately   d dcos • Scattering strong only if waves are in phase • Must be integer multiple of wavelength dcos

  32. Polarization B0 E0 E0 B0 • Recall that light waves have electric and magnetic fields perpendicular to the direction of motion • But there are two independent ways of arranging this • Called polarization • Our eyes can’t tell these two polarizations apart • But some instruments can measure or take advantage of polarization • We describe polarization by telling which direction the electric field points, e.g. vertically or horizontally • A polarizer polarizes light along its transmission axis. • Malus’s Law

  33. Methods of Producing Polarization (1) ++++++ – – – – – – E0 n1 P n2 • Direct production • Antennas produce waves that are automatically polarized • Scattering • Light waves of all orientations hit small targets • Target has vibrating charges, like an antenna • Reflection and Brewster’s Angle: • When light hits a substance, some of it reflects and some refracts • Fraction of each depends on polarization • There’s a special angle – Brewster’s angle – where reflected is completely polarized

  34. Methods of Producing Polarization (2) E0 E0 E0 E0 E0 • Birefringent Crystals • Index of refraction has to do with electric fields from the wave pushing atoms around • In some crystals, it is easier to push them one way than another • Index of refraction depends on polarization • You can use such birefringent crystals to sort light based on polarization • Selective absorption • Similarly, some materials absorb one polarization better than another

  35. Some uses for Polarization E0 Sugar water E0 • Polarized Sun Glasses • “Glare” comes mostly from light scattered in the atmosphere and reflected from water • Mostly polarized • Sun glasses use selective absorption to eliminate it • Optical Activity • Some materials are capable of rotating the plane of polarization • These materials are not mirror-symmetric • Enantiomers, especially biological molecules • Studying rotation of polarized light detects presence of these molecules • Someday use these to detect life on other planets?

  36. Ans A

  37. Solve on Board

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