Notes on Unit 1: Reflection and Refraction of Light

Unit 1: Reflection and Refraction of Light

1. Nature of Light
  • Light is an electromagnetic radiation and a form of energy transfer from source to observer.
  • Light shows a dual nature: acts like a particle in some experiments and like a wave in others.
  • Historical perspectives:
    • Newton: particle theory of light (emission from objects into eyes).
    • Huygens: wave theory proposing light as wave motion.
    • Thomas Young (1801): demonstrated interference of light, supporting the wave model.
    • Maxwell (1865): electromagnetic wave theory; light as a high-frequency wave with fixed speed in vacuum, c.
  • Speed of light in vacuum: c3×108 ms1.c \,\approx \,3 \times 10^{8} \ \mathrm{m\,s^{-1}}.
  • Einstein (1905): quantum model introducing photons; later work by Planck and Bohr refined this idea.
  • Timeline activity mentioned: Physicists and contributions to light (dates: 1800, 1780, 1850, 1900, 1950, 1970).
2. Reflection and Refraction (Overview)
  • Reflection and refraction occur at boundaries between transparent media.
  • Reflection involves light returning into the original medium; refraction involves bending into the new medium due to a change in light speed.
  • Focus areas: reflection at boundaries, refraction at boundaries, Snell’s Law, Huygens’s Principle, total internal reflection, and practical applications (e.g., fiber optics).
3. Reflection
  • Definition: Reflection occurs when light meets a boundary and bounces back.
  • Two major types:
    • Specular reflection: reflection from a smooth surface; reflected rays are parallel.
    • Examples: mirror, glass surface, calm water.
    • Diffuse reflection: reflection from a rough surface; reflected rays scatter in many directions.
    • Examples: bricks, wood, wall paint, skin.
  • Law of Reflection:
    • The angle of incidence equals the angle of reflection when measured with respect to the normal.
    • Notation: θ<em>i=θ</em>r\theta<em>i = \theta</em>r where angles are measured from the normal, not the surface plane.
  • Example types:
    • Simple incidence on a flat surface (e.g., 30° with the plane yields a reflected angle of 30° with the normal).
    • Two mirrors at right angles problem: determine outgoing directions after successive reflections.
4. Refraction and Snell’s Law
  • Refraction: bending of light as it passes from one medium to another due to speed change.
  • Why refraction occurs: difference in optical density (speed of light differs in media).
  • Key relation between speed and refractive index:
    • Refractive index: n=cvn = \frac{c}{v} where cc is the speed of light in vacuum and vv is the speed in the medium.
    • Light speed in medium: v=cnv = \frac{c}{n}
  • Snell’s Law (law of refraction):
    • n<em>1sinθ</em>1=n<em>2sinθ</em>2n<em>1 \sin \theta</em>1 = n<em>2 \sin \theta</em>2 where θ<em>1\theta<em>1 is the angle of incidence, θ</em>2\theta</em>2 is the angle of refraction, and n<em>1,n</em>2n<em>1, n</em>2 are the refractive indices of the two media.
  • Invariance of frequency across boundary:
    • Frequency remains constant when light crosses a boundary: f<em>1=f</em>2f<em>1 = f</em>2.
    • Wavelength changes with medium because the wave speed changes while frequency stays fixed:
    • λ<em>1=v</em>1f\lambda<em>1 = \frac{v</em>1}{f} and λ<em>2=v</em>2f\lambda<em>2 = \frac{v</em>2}{f}.
    • Therefore, λ<em>1λ</em>2=v<em>1v</em>2\frac{\lambda<em>1}{\lambda</em>2} = \frac{v<em>1}{v</em>2} and since v=c/nv = c/n, \frac{\lambda1}{\lambda2} = \frac{n2}{n1}\n.
  • Consequences of refraction:
    • If light enters a medium where speed is lower (higher n), the angle of refraction is smaller (bends toward the normal).
    • If light enters a medium where speed is higher (lower n), the angle of refraction is larger (bends away from the normal).
    • These behaviors reverse when light moves from lower to higher density (lower to higher n).
5. Huygens’s Principle
  • Proposed by Huygens (1678) as a geometrical method to derive reflection and refraction laws.
  • Core idea: every point on a wavefront acts as a source of secondary spherical wavelets; the new wavefront is the tangent to these wavelets after time (\Delta t).
  • It supports the wave-model view of light rather than the particle view.
6. Refractive Index (Table) and Notable Values (n)
  • Common refractive indices (approximate, 20°C, 1 atm unless noted):
    • Air: n1.000n \approx 1.000
    • Water: n1.333n \approx 1.333
    • Diamond: n2.419n \approx 2.419
    • Glass (crown): n1.52n \approx 1.52
    • Glass (flint): n1.66n \approx 1.66
    • Fluorite: n1.434n \approx 1.434
    • Fused quartz (SiO₂): n1.458n \approx 1.458
    • Ethyl alcohol: n1.361n \approx 1.361
    • Glycerine: n1.473n \approx 1.473
    • Ice (H₂O) at 0°C: n1.309n \approx 1.309
    • Benzene: n1.501n \approx 1.501
    • Carbon disulfide: n1.628n \approx 1.628
    • Carbon tetrachloride: n1.461n \approx 1.461
    • Sodium chloride (NaCl): n1.544n \approx 1.544
    • Zircon: n1.923n \approx 1.923
    • Ammonia: not listed in the table but often around 1.000–1.35 depending on phase and wavelength
  • Note on air index for gases: shown as 1.000 at 0°C, 1 atm in the table.
7. Frequency vs Wavelength Across Boundaries
  • Frequency remains constant across media:
    • f<em>1=f</em>2.f<em>1 = f</em>2.
  • Wavelength changes because speed changes:
    • λ=vf.\lambda = \frac{v}{f}.
  • Because v=cnv = \frac{c}{n}, the wavelength ratio relates to refractive indices:
    • λ<em>1λ</em>2=v<em>1v</em>2=n<em>2n</em>1.\frac{\lambda<em>1}{\lambda</em>2} = \frac{v<em>1}{v</em>2} = \frac{n<em>2}{n</em>1}.
  • In short, crossing a boundary changes wavelength but not frequency.
8. Total Internal Reflection (TIR)
  • Occurs when light attempts to move from a medium with a higher refractive index (denser) to a medium with a lower index (less dense) and hits the boundary at a sufficiently large incidence angle.
  • Critical angle θc\theta_c is defined by the condition that the refracted ray travels along the boundary (angle of refraction = 90°):
    • From Snell’s Law: n<em>1sinθ</em>c=n<em>2sin90°=n</em>2.n<em>1 \sin \theta</em>c = n<em>2 \sin 90° = n</em>2.
    • Therefore, θ<em>c=arcsin(n</em>2n<em>1)\theta<em>c = \arcsin\left(\frac{n</em>2}{n<em>1}\right), valid for n1 > n_2.
  • For incidence angles greater than the critical angle, the light is totally internally reflected.
  • Applications:
    • Fiber optics: light is guided through cores with total internal reflection, minimal loss.
    • Medical uses and telecommunications.
  • Example problems (typical outcomes):
    • Example: Flint glass (n = 1.66) in air (n ≈ 1): θc=arcsin(11.66)37exto.\theta_c = \arcsin \left(\frac{1}{1.66}\right) \approx 37^ ext{o}.
    • Sound analog: Air (v ≈ 342 m/s) to concrete (v ≈ 1840 m/s) boundary yields:
    • sinθ<em>c=v</em>extairv<em>extconcrete=34218400.186θ</em>c10.7exto.\sin \theta<em>c = \frac{v</em>{ ext{air}}}{v<em>{ ext{concrete}}} = \frac{342}{1840} \approx 0.186 \Rightarrow \theta</em>c \approx 10.7^ ext{o}.
  • Note: For TIR, the incident light must originate in the denser (slower) medium.
9. Worked Examples and Applications (Snell’s Law and TIR)
  • Example: Water entry from air at 24.5° with refractive water index around 1.36.
    • Given: incident angle θ<em>1=24.5exto\theta<em>1 = 24.5^ ext{o}, n</em>11.00n</em>1 \approx 1.00 (air), n21.36n_2 \approx 1.36 (water).
    • Compute θ<em>2\theta<em>2 using Snell’s Law: sinθ</em>2=n<em>1n</em>2sinθ1=11.36sin24.5exto.\sin \theta</em>2 = \frac{n<em>1}{n</em>2} \sin \theta_1 = \frac{1}{1.36} \sin 24.5^ ext{o}.
    • With sin24.5exto0.416\sin 24.5^ ext{o} \approx 0.416, we get sinθ<em>20.306\sin \theta<em>2 \approx 0.306, so θ</em>217.8exto\theta</em>2 \approx 17.8^ ext{o}.
  • Example: A beam in air incident at 37° on a surface to a material with refracted angle 25°.
    • Using Snell’s Law to find the material’s refractive index: n<em>2=n</em>1sinθ<em>1sinθ</em>2=1.0×sin37extosin25exto.n<em>2 = \frac{n</em>1 \sin \theta<em>1}{\sin \theta</em>2} = \frac{1.0 \times \sin 37^ ext{o}}{\sin 25^ ext{o}}.
    • Since sin37exto0.6018\sin 37^ ext{o} \approx 0.6018 and sin25exto0.4226\sin 25^ ext{o} \approx 0.4226, n20.60180.42261.425.n_2 \approx \frac{0.6018}{0.4226} \approx 1.425.
    • Speed in the material: v<em>2=cn</em>23.00×1081.4252.11×108 ms1.v<em>2 = \frac{c}{n</em>2} \approx \frac{3.00 \times 10^8}{1.425} \approx 2.11 \times 10^8\ \mathrm{m\,s^{-1}}.
  • Example: Coconut oil (n ≈ 1.48) and incidence 25.5° with a given diagram.
    • Method: apply Snell’s Law to determine corresponding angles at interfaces using the given refractive index.
  • Example: An acrylic cube under water (n = 1.49) and total internal reflection at the top face: determine the incident angle for TIR.
    • Method: use the critical angle formula with n1 = 1.49 (acrylic) and n2 ≈ 1.33 (water) or the relative boundary as given to find the threshold for TIR.
10. Summary of Key Formulas
  • Refractive index: n=cvn = \frac{c}{v}
  • Speed in medium: v=cnv = \frac{c}{n}
  • Snell’s Law: n<em>1sinθ</em>1=n<em>2sinθ</em>2n<em>1 \sin \theta</em>1 = n<em>2 \sin \theta</em>2
  • Frequency continuity: f<em>1=f</em>2f<em>1 = f</em>2
  • Wavelength relation across boundary (with constant frequency): λ<em>1λ</em>2=v<em>1v</em>2=n<em>2n</em>1\frac{\lambda<em>1}{\lambda</em>2} = \frac{v<em>1}{v</em>2} = \frac{n<em>2}{n</em>1}
  • Wavelength: λ=vf\lambda = \frac{v}{f}
  • Total Internal Reflection: \thetac = \arcsin\left(\frac{n2}{n1}\right)\quad (n1 > n_2)
  • Condition for TIR: θ<em>1>θ</em>c\theta<em>1 > \theta</em>c
11. Applications of Internal Reflection
  • Fiber optics: light transmitted with minimal loss along fibers; loss mainly at ends or due to absorption.
  • Medical applications: endoscopy and diagnostic fiber-optic tools.
  • Telecommunications: use of fiber cables for data transmission.
12. Quick Practice Problems (Representative Solutions)
  • Problem: An optical fiber core (n1 = 1.55) and cladding (n2 = 1.42).
    • (a) Critical angle: θ<em>c=arcsin(n</em>2n1)=arcsin(1.421.55)66.5exto.\theta<em>c = \arcsin\left(\frac{n</em>2}{n_1}\right) = \arcsin\left(\frac{1.42}{1.55}\right) \approx 66.5^ ext{o}.
    • (b) If light tries to exit at angles greater than this, TIR occurs.
  • Problem: Air-to-water interface: incident angle 24.5°, water speed v ≈ 2.22 × 10^8 m/s.
    • Water index: n2=cv=3.0×1082.22×1081.36.n_2 = \frac{c}{v} = \frac{3.0 \times 10^8}{2.22 \times 10^8} \approx 1.36.
    • Snell: sinθ<em>2=n</em>1n<em>2sinθ</em>1=11.36sin24.5exto0.306θ217.8exto.\sin \theta<em>2 = \frac{n</em>1}{n<em>2} \sin \theta</em>1 = \frac{1}{1.36} \sin 24.5^ ext{o} \approx 0.306 \Rightarrow \theta_2 \approx 17.8^ ext{o}.
  • Problem: Incident angle 37° from air into a block with refracted angle 25°.
    • Material index: n<em>2=n</em>1sinθ<em>1sinθ</em>2=1.0×sin37extosin25exto0.60180.42261.425.n<em>2 = \dfrac{n</em>1 \sin \theta<em>1}{\sin \theta</em>2} = \dfrac{1.0 \times \sin 37^ ext{o}}{\sin 25^ ext{o}} \approx \dfrac{0.6018}{0.4226} \approx 1.425.
    • Speed in material: v<em>2=cn</em>23.0×1081.4252.11×108 ms1.v<em>2 = \dfrac{c}{n</em>2} \approx \dfrac{3.0 \times 10^8}{1.425} \approx 2.11 \times 10^8\ \mathrm{m\,s^{-1}}.