1 / 20

3.38. Diffraction

3.38. Diffraction. Diffraction is a scale phenomenon that can only be described by use of waves. Consider a plane wave front of wavelength l incident on an aperture of width a. How does the wave change when it propagates through the aperture?

Download Presentation

3.38. Diffraction

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. 3.38. Diffraction • Diffraction is a scale phenomenon that can only be described by use of waves. • Consider a plane wave front of wavelength l incident on an aperture of width a. • How does the wave change when it propagates through the aperture? • We can understand the changes by using Huygens’ principle. • There are two cases to consider • Aperture width a greater than wavelength • Aperture width comparable to the wavelength.

  2. 3.38. Diffraction • Aperture width a greater than wavelength l. • Here plane wave front of wavelength l incident the aperture of width a. • In the aperture we can set up many secondary sources. • These produce secondary wavelets. • In the centre of the aperture the leading edges of the wavelets produces a plane wave front. • At the edges, the wavelets form a curved wavefront. • Hence the wave front appears to propagate through the aperture as if it were a plane wave in the centre but is only disrupted at the edges.

  3. a > l

  4. 3.38. Diffraction • Aperture width a comparable to wavelength l. • Here plane wave front of wavelength l incident the aperture of width a. • In the aperture we can set up many secondary sources. • These produce secondary wavelets. • In the centre of the aperture the leading edges of the wavelets produces a plane wave front. • At the edges, the wavelets form a curved wavefront. • Hence the wave front appears to propagate through the aperture as if it were a plane wave in the centre but is only disrupted at the edges.

  5. a ~ l

  6. Source 1 Detector , x Source 2 3.39 Interference Consider two light sources that produce harmonic waves of equal amplitude A but equal frequency f. A detector is placed a distance x1 from source 1 and a distance x2 from source 2. x1 x2 How does the signal recorded by a detector vary as we vary the distances x1 and x2? Need to use the principle of linear superposition to obtain the answer.

  7. Let the wave function for source 1 be • y1(x,t) = Asin(kx1-wt + f1(t)) • and for source 2 • y2(x,t) = Asin(kx2-wt + f2(t)) • From principle of linear superposition we have • yt(x,t) = y1(x,t) + y2(x,t) • yt(x,t) = Asin(kx1-wt + f1(t)) + Asin(kx2-wt + f2(t)) • Which becomes

  8. Term that depends on separation of sources Harmonic wave at ave distance • Thus at x we have a harmonic wave with phase that depends on the average distance of the detector from the sources multiplied by a term that depends solely on the difference in distance between the two sources. • Let us assume that the initial phase of each wave is zero. We will discuss the significance of the initial phase later. • The displacement at the point x is given by

  9. The detector responds to the intensity of the signal. Hence we find If we use the relationship We find

  10. When k(x1-x2) = 2nπ (n = integer) the intensity is a maximum When k(x1-x2) = (2n+1)π (n = integer) the intensity is zero Thus there is a periodic modulation of the intensity that depends on the difference in distance between the two sources and the detector. The term (x1-x2) is known as the path difference.

  11. The term (x1-x2) is known as the path difference. For an intensity maximum k(x1-x2) = 2nπ But k = 2π/l So (x1-x2) = nl Thus when the path difference is an integer number of wavelengths there is an intensity maximum For an intensity minimum k(x1-x2) = (2n+1)π But k = 2π/l So (x1-x2) = (n+1/2)l Thus when the path difference is a half integer number of wavelengths there is an intensity minimum.

  12. If we now include the initial phase for each of the waves how is the intensity pattern affected? • We find that the displacement is given by • The intensity becomes

  13. We can understand the effect of the initial phase with reference to the cosine term in the intensity • The difference between f1(t) and f2(t) remains constant for all time then the interference pattern remains constant. • If the difference between f1(t) and f2(t) varies in a random fashion then we find that the value of the cosine term fluctuates randomly between +1 and -1. • As a result the intensity pattern varies in an unpredictable fashion and the fringes are “washed out”.

  14. If f1(t) - f2(t) remains constant for all time the sources are said to be coherent. • Example of a coherent source - loud speakers connected to the same frequency source • For coherent sources the intensity I(x,t) is given by • If f1(t) - f2(t) varies randomly as a function of time the sources are said to be incoherent. • Example of incoherent source - car headlights • For incoherent sources the intensity I(x,t) is given by

  15. 3.40 Young’s Slits Experiment: Interference from two sources Two slits s1 and s2 are separated by a distance d. A screen is placed a distance L from the slits (L>>d). The nth bright interference fringe is seen a B a height yn from the centre of the screen. The slits are illuminated by a white light source located behind the pinhole p. This ensures that the slits are illuminated by coherent radiation.

  16. 3.40 Young’s Slits Experiment: Interference from two sources S1B = x1 S2B = x2 S2B - S1B = x2 - x1 x2 - x1 = r r = dsina yn = Ltana For the nth bright fringe the path difference between S2B and S1B must be an integer number of wavelengths. x2 - x1 = nl r = nl

  17. 3.40 Young’s Slits Experiment: Interference from two sources S1B = x1 S2B = x2 S2B - S1B = x2 - x1 x2 - x1 = r r = dsina yn = Ltana Now the angle a is small and so sina = tana. Hence r= ynd/L so ynd/L = nl Thus yn = Lnl/d The spacing between successive fringes is ∆ = Ll/d

  18. 3.41 Single slit diffraction Consider a slit of width a. A plane wave is incident on the slit. A set of secondary sources are set up in the slit. We find that at an angle b the source at 1 is p ( l/2) out of phase with the source at 5. The source at 5 is p ( l/2) out of phase with the source at 9. Also the source at 5 is at the centre of the slit. So when the condition asinb = ml is satisfied destructive interference occurs.

More Related