Spherical Mirrors and Wave Mechanics Study Notes

Spherical and Parabolic Mirrors

  • Spherical Mirrors: Formed from silvered spherical glass.
    • Convex (Diverging): Silvered on the inside.
    • Concave (Converging): Silvered on the outside.
  • Key Terms:
    • Centre of curvature (CC): The center of the original sphere.
    • Pole (PP): The center of the mirror surface.
    • Principal axis: Line connecting CC and PP.
    • Principal focus (FF): Converging point for reflected rays (real for concave, virtual for convex).
    • Radius of curvature (rr): Distance from PP to CC.
    • Focal length (ff): Distance from PP to FF.
  • Parabolic Mirrors: Used to produce wide parallel beams or converge light to a single point; common in car headlights and spotlights.

Image Formation by Spherical Mirrors

  • Ray Diagram Rules: Images are located using the intersection of two rays:
    • Ray parallel to the principal axis (reflects through FF or appears to).
    • Ray through CC (reflects back along its own path).
    • Ray through FF (reflects parallel to the principal axis).
  • Concave Mirror Image Cases:
    • Object at infinity: Real, inverted, diminished image at FF.
    • Object at CC: Real, inverted, same size image at CC.
    • Object behind CC: Real, inverted, diminished image between CC and FF.
    • Object between FF and CC: Real, inverted, magnified image behind CC.
    • Object at FF: Image at infinity.
    • Object between FF and PP: Virtual, erect, magnified image behind the mirror.
  • Convex Mirror Image Cases: Always formed behind the mirror; always virtual, erect, and diminished.

Applications and Magnification

  • Applications: Used in satellite dishes, shaving mirrors, telescopes, and driving mirrors.
  • Magnification (MM): The ratio of image size to object size, or image distance to object distance.
    • M=height of the imageheight of the objectM = \frac{\text{height of the image}}{\text{height of the object}}
    • M>1M > 1 is magnified; M<1M < 1 is diminished.
  • Quantitative Examples:
    • Case 1 (Concave): Object height 5.0cm5.0\,cm, f=15cmf = 15\,cm, distance 35cm35\,cm. Image location is 27cm27\,cm in front of mirror, size is 3.75cm3.75\,cm (real and inverted).
    • Case 2 (Convex): Object height 5cm5\,cm, f=15cmf = 15\,cm, distance 10cm10\,cm. Image location is 6.0cm6.0\,cm behind mirror, size is 3.0cm3.0\,cm (virtual and erect). M=0.6M = 0.6.

Introduction to Waves

  • Wave: A disturbance moving through a medium.
  • Electromagnetic Waves: Can travel through a vacuum (e.g., radio, X-rays, gamma rays, UV rays).
  • Mechanical Waves: Require a material medium to transfer (e.g., water, sound waves).
  • Wave Types:
    • Transverse Waves: Displacement is perpendicular to the direction of travel (consist of crests and troughs).
    • Longitudinal Waves: Particles vibrate parallel to the direction of travel (consist of compressions and rarefactions).

Properties and Measurement of Waves

  • Characteristics:
    • Wavelength (λ\lambda): Distance between two successive points in a wave, measured in metres (mm).
    • Frequency (ff): Number of waves passing a point in one second, measured in Hertz (HzHz).
    • Period (TT): Time for a complete wave to pass; T=1fT = \frac{1}{f}.
    • Amplitude: Maximum displacement from the rest position.
  • Wave Equation: v=fλv = f \lambda
  • Calculation Practice:
    • Example 1: For a rope at 3Hz3\,Hz with a wavelength of 0.8m0.8\,m, speed v=3×0.8=2.4m/sv = 3 \times 0.8 = 2.4\,m/s.
    • Example 2: In water with v=2ms1v = 2\,ms^{-1}, displacement-time graph yields amplitude =0.4cm= 0.4\,cm, period T=0.20secondsT = 0.20\,seconds, frequency f=5Hzf = 5\,Hz, and wavelength λ=0.4m\lambda = 0.4\,m.