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    Applied Physics
    GE-169
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    Topics
    1. Electric Force and Its Applications2. Conservation of Charge3. Charge Quantization4. Electric Fields Due to Point Charge and Lines of Force5. Electric Fields: Ring of Charge and Disk of Charge6. A Point Charge in an Electric Field7. Dipole in an Electric Field8. Flux of a Vector Field9. Flux of an Electric Field10. Gauss’ Law and Its Applications11. Spherically Symmetric Charge Distribution12. Charge Isolated Conductor13. Electric Potential Energy14. Electric Potentials and Related Problems15. Calculating Potential from the Field16. Potential Due to Point and Continuous Charge Distribution17. Potential Due to a Dipole18. Equipotential Surfaces19. Calculating the Field from the Potential20. Electric Current and Current Density21. Resistance, Resistivity, and Conductivity22. Ohm's Law and Its Applications23. The Hall Effect24. Magnetic Force on a Current25. The Biot-Savart Law26. Line of Magnetic Field (B)27. Two Parallel Conductors28. Ampere's Law29. Solenoids and Toroids30. Faraday's Experiments and Law of Induction31. Lenz's Law32. Motional EMF33. Induced Electric Fields34. The Basic Equations of Electromagnetism35. Induced Magnetic Fields36. The Displacement Current37. Reflection and Refraction of Light Waves38. Total Internal Reflection39. Two Source Interference40. Double-Slit Interference and Related Problems41. Interference from Thin Films42. Diffraction and Wave Theory43. Single-Slit Diffraction and Related Problems44. Polarization of Electromagnetic Waves45. Polarizing Sheets and Related Problems
    GE-169›Single-Slit Diffraction and Related Problems
    Applied PhysicsTopic 43 of 45

    Single-Slit Diffraction and Related Problems

    11 minread
    1,874words
    Intermediatelevel

    Single-Slit Diffraction and Related Problems

    Single-slit diffraction is a fundamental phenomenon in wave optics, where light passes through a narrow slit and spreads out, creating a pattern of bright and dark regions on a screen. The diffraction pattern results from interference between light waves emerging from different parts of the slit.

    1. Diffraction from a Single Slit

    When monochromatic light passes through a single slit, it behaves as a set of point sources of secondary wavelets, according to Huygens' principle. These wavelets interfere with each other, leading to a characteristic diffraction pattern with a central bright fringe, flanked by alternating dark and bright fringes.

    Key Features of the Single-Slit Diffraction Pattern:

    • Central Maximum: The brightest and widest band, located directly in front of the slit.
    • Secondary Maxima: Weaker bright fringes that occur between the dark fringes.
    • Dark Fringes: Points where destructive interference occurs, creating completely dark spots.

    2. Condition for Dark Fringes (Destructive Interference)

    The dark fringes in a single-slit diffraction pattern occur when the path difference between the light waves from the edges of the slit is an integer multiple of the wavelength. The condition for destructive interference (dark fringes) is given by:

    asin⁡(θ)=mλa \sin(\theta) = m \lambdaasin(θ)=mλ

    Where:

    • aaa is the width of the slit,
    • θ\thetaθ is the angle of diffraction,
    • λ\lambdaλ is the wavelength of the light,
    • mmm is an integer (1, 2, 3, ...) representing the order of the minima (first, second, third, etc.).

    For the central maximum (bright fringe), the light from all points in the slit arrives in phase, leading to constructive interference.

    Angular Position of the Minima:

    • The angular positions of the first minima (dark fringes) on either side of the central maximum can be found by substituting m=1,2,3,…m = 1, 2, 3, \dotsm=1,2,3,….

      For example:

      • The first dark fringe occurs when m=1m = 1m=1,
      • The second dark fringe occurs when m=2m = 2m=2, and so on.

    Width of the Central Maximum:

    The angular width of the central maximum (the region between the first minima on either side) is:

    Δθ=2λa\Delta \theta = \frac{2\lambda}{a}Δθ=a2λ​

    This is the angular separation between the first dark fringes on either side of the central maximum.


    3. Intensity Distribution in Single-Slit Diffraction

    The intensity of light in the diffraction pattern varies across the screen, and the distribution of light intensity I(θ)I(\theta)I(θ) as a function of the angle θ\thetaθ is given by:

    I(θ)=I0(sin⁡(β)β)2I(\theta) = I_0 \left( \frac{\sin(\beta)}{\beta} \right)^2I(θ)=I0​(βsin(β)​)2

    Where:

    • I0I_0I0​ is the intensity at the central maximum,
    • β=πaλsin⁡(θ)\beta = \frac{\pi a}{\lambda} \sin(\theta)β=λπa​sin(θ),
    • λ\lambdaλ is the wavelength of light,
    • aaa is the slit width,
    • θ\thetaθ is the angle.

    The central maximum is the brightest, and the intensity gradually decreases as you move away from the center. The first minima occurs at β=π\beta = \piβ=π, and subsequent minima occur at multiples of π\piπ.


    4. Single-Slit Diffraction Example Problems

    Example 1: Angular Position of the First Minimum

    Problem: A monochromatic light of wavelength 600 nm600 \, \text{nm}600nm passes through a slit of width 0.1 mm0.1 \, \text{mm}0.1mm. What is the angle for the first dark fringe in the diffraction pattern if the screen is placed 5 meters away?

    Solution:

    • Given:
      • Wavelength of light: λ=600 nm=6×10−7 m\lambda = 600 \, \text{nm} = 6 \times 10^{-7} \, \text{m}λ=600nm=6×10−7m,
      • Slit width: a=0.1 mm=1×10−4 ma = 0.1 \, \text{mm} = 1 \times 10^{-4} \, \text{m}a=0.1mm=1×10−4m,
      • Order of the dark fringe: m=1m = 1m=1 (first dark fringe),
      • Distance to the screen: L=5 mL = 5 \, \text{m}L=5m.

    Using the condition for destructive interference:

    asin⁡(θ)=mλa \sin(\theta) = m \lambdaasin(θ)=mλ

    For the first dark fringe (m=1m = 1m=1):

    (1×10−4)sin⁡(θ)=6×10−7(1 \times 10^{-4}) \sin(\theta) = 6 \times 10^{-7}(1×10−4)sin(θ)=6×10−7 sin⁡(θ)=6×10−71×10−4=6×10−3\sin(\theta) = \frac{6 \times 10^{-7}}{1 \times 10^{-4}} = 6 \times 10^{-3}sin(θ)=1×10−46×10−7​=6×10−3

    For small angles, sin⁡(θ)≈θ\sin(\theta) \approx \thetasin(θ)≈θ, so:

    θ≈6×10−3 radians\theta \approx 6 \times 10^{-3} \, \text{radians}θ≈6×10−3radians

    To find the linear position yyy on the screen for the first dark fringe, we use the approximation:

    y=Lθ=5×6×10−3=0.03 m=3 cmy = L \theta = 5 \times 6 \times 10^{-3} = 0.03 \, \text{m} = 3 \, \text{cm}y=Lθ=5×6×10−3=0.03m=3cm

    So, the first dark fringe occurs at an angle of approximately 6×10−36 \times 10^{-3}6×10−3 radians and is located 3 cm3 \, \text{cm}3cm from the central maximum.


    Example 2: Width of the Central Maximum

    Problem: A single-slit diffraction pattern is produced with light of wavelength 500 nm500 \, \text{nm}500nm passing through a slit of width 0.25 mm0.25 \, \text{mm}0.25mm. What is the angular width of the central maximum?

    Solution:

    • Given:
      • Wavelength: λ=500 nm=5×10−7 m\lambda = 500 \, \text{nm} = 5 \times 10^{-7} \, \text{m}λ=500nm=5×10−7m,
      • Slit width: a=0.25 mm=2.5×10−4 ma = 0.25 \, \text{mm} = 2.5 \times 10^{-4} \, \text{m}a=0.25mm=2.5×10−4m.

    The angular width of the central maximum is the angular separation between the first minima on both sides, which is:

    Δθ=2λa\Delta \theta = \frac{2\lambda}{a}Δθ=a2λ​

    Substituting the given values:

    Δθ=2×5×10−72.5×10−4=4×10−3 radians\Delta \theta = \frac{2 \times 5 \times 10^{-7}}{2.5 \times 10^{-4}} = 4 \times 10^{-3} \, \text{radians}Δθ=2.5×10−42×5×10−7​=4×10−3radians

    So, the angular width of the central maximum is 4×10−34 \times 10^{-3}4×10−3 radians, or 0.004 radians0.004 \, \text{radians}0.004radians.


    Example 3: Intensity at a Given Angle

    Problem: A monochromatic light of wavelength 650 nm650 \, \text{nm}650nm passes through a slit of width 0.2 mm0.2 \, \text{mm}0.2mm. What is the intensity at an angle θ=30∘\theta = 30^\circθ=30∘ if the intensity at the central maximum is I0=100 arbitrary unitsI_0 = 100 \, \text{arbitrary units}I0​=100arbitrary units?

    Solution:

    • Given:
      • Wavelength: λ=650 nm=6.5×10−7 m\lambda = 650 \, \text{nm} = 6.5 \times 10^{-7} \, \text{m}λ=650nm=6.5×10−7m,
      • Slit width: a=0.2 mm=2×10−4 ma = 0.2 \, \text{mm} = 2 \times 10^{-4} \, \text{m}a=0.2mm=2×10−4m,
      • Angle: θ=30∘\theta = 30^\circθ=30∘,
      • Intensity at the central maximum: I0=100 arbitrary unitsI_0 = 100 \, \text{arbitrary units}I0​=100arbitrary units.

    First, calculate β\betaβ:

    β=πaλsin⁡(θ)\beta = \frac{\pi a}{\lambda} \sin(\theta)β=λπa​sin(θ) β=π×2×10−46.5×10−7×sin⁡(30∘)=π×2×10−46.5×10−7×12\beta = \frac{\pi \times 2 \times 10^{-4}}{6.5 \times 10^{-7}} \times \sin(30^\circ) = \frac{\pi \times 2 \times 10^{-4}}{6.5 \times 10^{-7}} \times \frac{1}{2}β=6.5×10−7π×2×10−4​×sin(30∘)=6.5×10−7π×2×10−4​×21​ β=π×10−46.5×10−7≈484.78\beta = \frac{\pi \times 10^{-4}}{6.5 \times 10^{-7}} \approx 484.78β=6.5×10−7π×10−4​≈484.78

    Now, using the intensity formula:

    I(θ)=I0(sin⁡(β)β)2I(\theta) = I_0 \left( \frac{\sin(\beta)}{\beta} \right)^2I(θ)=I0​(βsin(β)​)2

    Since β\betaβ is large, sin⁡(β)≈1β\sin(\beta) \approx \frac{1}{\beta}sin(β)≈β1​, so:

    I(θ)≈I0(1β)2=100×(1484.78)2I(\theta) \approx I_0 \left( \frac{1}{\beta} \right)^2 = 100 \times \left( \frac{1}{484.78} \right)^2I(θ)≈I0​(β1​)2=100×(484.781​)2 I(\theta) \approx 100 \times (4.12 \times 10^{-5})^2 = 100 \times 1.69 \
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    Diffraction and Wave Theory
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    Polarization of Electromagnetic Waves

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