36.3 Content
36.3.1 Historical Models of Light
Newton’s Corpuscular Theory (1670s): - Light consists of tiny particles (corpuscles) - Explains reflection and refraction (incorrectly assumed faster in denser media) - Cannot explain diffraction or interference
Huygens’ Wave Theory (1678): - Light is a wave in a medium (ether) - Each point on a wavefront is a source of secondary wavelets - Correctly explains reflection, refraction, and diffraction
Wave theory predicts light is slower in denser media. Particle theory predicts it’s faster. Foucault (1850) proved light is slower in water—confirming wave theory.
36.3.2 Double-Slit Interference
When light passes through two narrow slits, it creates an interference pattern:
\[d\sin\theta = m\lambda\]
where: - \(d\) = slit separation (m) - \(\theta\) = angle to the maximum - \(m\) = order number (0, ±1, ±2, …) - \(\lambda\) = wavelength (m)
For bright fringes (constructive interference): \(m = 0, 1, 2, ...\) For dark fringes (destructive interference): path difference = \((m + \frac{1}{2})\lambda\)
36.3.3 Interactive: Double-Slit Interference
36.3.4 Path Difference
Constructive interference occurs when waves arrive in phase:
\[\Delta = m\lambda\]
Destructive interference occurs when waves arrive out of phase:
\[\Delta = (m + \frac{1}{2})\lambda\]
36.3.5 Diffraction Gratings
A diffraction grating has thousands of slits per millimetre, producing sharp, bright maxima:
\[d\sin\theta = m\lambda\]
The grating equation is identical to double-slit, but: - Maxima are much sharper (many slits reinforce) - Higher orders are clearly separated - Used for precise wavelength measurement
If a grating has N lines per mm, then: \[d = \frac{1}{N \times 1000}\ \text{metres}\]
36.3.6 Interactive: Diffraction Grating
36.3.7 Polarisation
Polarisation is the restriction of a wave’s oscillation to a single plane. Only transverse waves can be polarised—proving light is a transverse wave.
Malus’s Law: When polarised light passes through an analyser:
\[I = I_0\cos^2\theta\]
where: - \(I_0\) = intensity after first polariser - \(\theta\) = angle between polariser axes - \(I\) = transmitted intensity
- \(\theta = 0°\): Maximum transmission (\(I = I_0\))
- \(\theta = 45°\): Half transmission (\(I = 0.5I_0\))
- \(\theta = 90°\): No transmission (\(I = 0\))—crossed polarisers