Light waves behave in fascinating ways when encountering obstacles or openings. The Huygens-Fresnel principle explains how waves spread and bend, creating intricate patterns of bright and dark spots. It's like ripples in a pond, but with light!
This principle is crucial for understanding diffraction, a key concept in optics. By treating each point on a wavefront as a source of new waves, we can predict how light will behave when it passes through small openings or around edges.
Huygens-Fresnel Principle and Wavefront Propagation
Huygens-Fresnel principle in diffraction
- Powerful tool for understanding and predicting behavior of light waves in presence of obstacles or apertures
- Combines Huygens' principle each point on wavefront acts as secondary source of spherical wavelets with Fresnel's additions including concept of interference and inclination factor
- Wavefront at any later time determined by superposition of secondary wavelets
- Wavelets interfere with each other resulting in observed diffraction patterns (interference fringes, bending of light around obstacles)
- Explains various diffraction phenomena
- Bending of light around obstacles (diffraction around edges)
- Formation of diffraction fringes (alternating bright and dark bands)
- Spreading of light after passing through aperture (diffraction through slits or circular openings)
Wavefront propagation and diffraction
- Wavefront surface of constant phase in propagating wave
- In light wavefronts perpendicular to direction of propagation represent surfaces of constant optical path length
- According to Huygens-Fresnel principle each point on wavefront acts as source of secondary spherical wavelets propagating outward with same speed as original wave
- Propagation of wavelets and their subsequent interference give rise to diffraction patterns observed when light encounters obstacles or apertures
- Diffraction effects more pronounced when size of obstacle or aperture comparable to wavelength of light (small apertures, edges of objects)
Mathematical Formulation and Limitations
Mathematical formulation of Huygens-Fresnel
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Fresnel-Kirchhoff diffraction formula calculates complex amplitude of diffracted field at point $P$ $U(P) = \frac{1}{i\lambda} \iint_S U(Q) \frac{e^{ikr}}{r} \cos(\mathbf{n}, \mathbf{r}) dS$
- $U(P)$ complex amplitude at point $P$
- $U(Q)$ complex amplitude at point $Q$ on aperture
- $\lambda$ wavelength of light
- $k = \frac{2\pi}{\lambda}$ wave number
- $r$ distance between points $P$ and $Q$
- $\mathbf{n}$ normal vector to aperture surface
- $\mathbf{r}$ vector from $Q$ to $P$
- $dS$ infinitesimal area element on aperture surface
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Formula integrates contributions of secondary wavelets originating from each point on aperture
- Takes into account amplitude, phase, and inclination factor $\cos(\mathbf{n}, \mathbf{r})$ of wavelets
Limitations of Huygens-Fresnel model
- Relies on several assumptions and approximations limiting accuracy in certain situations
- Assumes aperture or obstacle large compared to wavelength of light
- Assumes diffracted field observed at large distance from aperture (far-field approximation)
- Neglects vectorial nature of light treats it as scalar wave may lead to inaccuracies when dealing with polarization effects or highly focused beams
- Does not account for finite size of secondary wavelets can lead to discrepancies in predicted diffraction patterns especially in near-field region
- Despite limitations remains valuable tool for understanding and predicting diffraction phenomena in many practical situations
- Particularly in far-field region and for apertures much larger than wavelength of light (visible light through macroscopic apertures)