Diffraction Of Light

Diffraction Of Light

Vishal kumarUpdated on 02 Jul 2025, 07:01 PM IST

Diffraction of light refers to the bending and spreading of light waves when they encounter an obstacle or pass through a narrow aperture. This phenomenon is a fundamental concept in wave optics and plays a crucial role in understanding the behaviour of light. In real life, diffraction is observed in various contexts, such as the colourful patterns seen when light passes through a diffraction grating, the spreading of light around the edges of objects, and the design of optical instruments like telescopes and microscopes to enhance resolution. Understanding diffraction helps improve technologies in fields like imaging, spectroscopy, and even everyday applications like the design of optical sensors and lasers. This article explores the principles of light diffraction and its significant impact on both scientific advancements and practical uses.

This Story also Contains

  1. Diffraction
  2. Solved Examples Based on Diffraction of Light
  3. Summary

Diffraction

Diffraction of light refers to the bending and spreading of light waves when they encounter an obstacle or pass through a narrow aperture. This phenomenon is a fundamental concept in wave optics and plays a crucial role in understanding the behaviour of light. In everyday life, diffraction can be observed in the spreading of light from a streetlamp through a fog, the patterns seen when light passes through a fine mesh or slit, and the iridescent colours of a CD or DVD.

The phenomenon of bending of light around the corners of an obstacle of the size of the wavelength of light is called diffraction.

The phenomenon resulting from the superposition of secondary wavelets originating from different parts of the same wavefront is defined as a diffraction of light.

Diffraction is the characteristic of all types of waves.

The wavelength of the wave is directly proportional to its degree of diffraction.

From the above figure, we can say that if slit width is more then wave will detract less.

Condition for Diffraction

For diffraction to occur, several conditions must be met:

  1. Wave Nature of Light: Light must be treated as a wave phenomenon rather than a particle phenomenon.

  2. Obstacle or Aperture Size: The size of the obstacle or aperture must be comparable to the wavelength of the light. If the obstacle or aperture is much larger than the wavelength, diffraction effects will be minimal.

  3. Coherent Light Source: The light source should be coherent, meaning that the light waves should have a constant phase difference and the same frequency. This is often achieved using monochromatic light sources, such as lasers.

  4. Narrow Aperture or Sharp Edges: The aperture should be narrow, or the edges should be sharp, to observe significant diffraction patterns. This allows the light waves to bend around the edges and interfere with each other, creating visible diffraction patterns.

When these conditions are met, diffraction causes light waves to spread out and create interference patterns, which can be observed as a series of bright and dark fringes. This principle is applied in various fields such as microscopy, astronomy, and the design of optical instruments.

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Solved Examples Based on Diffraction of Light

Example 1: The penetration of light into the region of geometrical shadow is called :

1)Polarization

2) Diffraction

3)Interference

4)Refraction

Solution:

Diffraction - The phenomenon of bending of light around the corners of an obstacle of the size of the wavelength of light is called diffraction.

So, the penetration of light into the region of the geometrical shadow is called diffraction

Hence, the answer is the option (2).

Example 2: The orange light of wavelength $6000 \times 10^{-10} \mathrm{~m}$ illuminates a single slit of width. The maximum possible number of diffraction minima produced on both sides of the central maximum is______.

1) 198

2)99

3)45

4)30

Solution:

Condition for minimum,
$
\begin{aligned}
& d \sin \theta=n \lambda \\
& \therefore \sin \theta=\frac{\mathrm{n} \lambda}{\mathrm{d}}<1 \\
& \mathrm{n}<\frac{\mathrm{d}}{\lambda}=\frac{6 \times 10^{-5}}{6 \times 10^{-7}}=100
\end{aligned}
$
$\therefore \quad$ Total number of minima on one side $=99$
Total number of minima $=198$

Hence, the answer is the option (1).

Example 3: In free space, an electromagnetic wave of 3 GHz frequency strikes over the edge of an object of size $\frac{\lambda}{100}$, where $\lambda$ is the wavelength of the wave in free space. The phenomenon, which happens there will be

1)Reflection

2)Refraction

3)Diffraction

4)Scattering

Solution:

For reflection size of the obstacle must be much larger than the wavelength, for diffraction size should be in order of wavelength and for scattering size of the obstacle must be smaller than the wavelength of the wave.

When an electromagnetic wave of frequency strikes over the edge of an object its wavelength gets changed due to the electromagnetic wave being absorbed. Then this phenomenon is known as scattering. Since the object is of size $\frac{\lambda}{100}$ much smaller than the wavelength $\lambda$, scattering will occur.

Hence, the answer is the option (4).

Example 4: A beam of light of wavelength 600 nm from a distant source falls on a single slit 1.00 mm wide and the resulting diffraction pattern is observed on a screen 2 m away. The distance between the first dark fringes on either side of the central bright fringe is

1)1.2 cm

2)1.2 mm

3)2.4 cm

4)2.4 mm

Solution:

$
\lambda=600 \mathrm{~nm}=6 \times 10^{-7} \mathrm{~m}, \mathrm{a}=1 \mathrm{~mm}=10^{-3} \mathrm{~m}, \mathrm{D}=2 \mathrm{~m}
$

Distance between the first dark fringes on either side of the central bright fringe $=$ width of central maximum
$
=\frac{2 \lambda \mathrm{D}}{\mathrm{a}}=\frac{2 \times 6 \times 10^{-7} \times 2}{10^{-3}}=24 \times 10^{-4} \mathrm{~m}=2.4 \mathrm{~mm}
$

Hence, the answer is the option (3).

Example 5: Diffraction pattern from a single slit of width 0.25 mm is observed with light of wavelength 4890 Angstrom. The angular separation between first-order minimum and third-order maximum, falling on the same side, is:

1) $5.89 \times 10^{-3} \mathrm{rad}$
2) $5.89 \times 10^{-7} \mathrm{rad}$
3) $5.89 \times 10^{-10} \mathrm{rad}$
4) $5.89 \times 10^{-4} \mathrm{rad}$

Solution:

In a single slit diffraction pattern, positions of secondary maxima and minima are given by,

$\theta_{\max }= \pm(2 \mathrm{n}+1) \frac{\lambda}{2 \mathrm{~d}}$ and $\theta_{\min }= \pm \mathrm{n} \frac{\lambda}{\mathrm{d}}$, respectively.
$\therefore \quad \theta_{1 \min }=\frac{\lambda}{\mathrm{d}}$ and $\theta_{3 \max }=\frac{7 \lambda}{2 \mathrm{~d}}$
Angular separation
$
\begin{aligned}
& \text { Angular separation }=\theta_{3 \max }-\theta_{1 \min }=\frac{7 \lambda}{2 \mathrm{~d}}-\frac{\lambda}{\mathrm{d}} \\
& =\frac{5 \lambda}{2 \mathrm{~d}}=\frac{5}{2} \times \frac{5890 \times 10^{-10}}{0.25 \times 10^{-3}}=5.89 \times 10^{-3} \mathrm{rad}
\end{aligned}
$

Hence, the answer is the option (1).

Summary

Diffraction of light is the bending and spreading of light waves when they pass through a narrow aperture or around an obstacle, revealing the wave nature of light. This phenomenon is crucial for understanding various optical behaviours and is observable in everyday life, such as in the patterns seen when light passes through a fine mesh or the iridescent colours on a CD. Diffraction principles are applied in numerous fields, including microscopy, astronomy, and the design of optical instruments, enhancing resolution and providing deeper insights into the structure of matter.

Frequently Asked Questions (FAQs)

Q: How does diffraction affect the design of metamaterials?
A:
Metamaterials are engineered materials with properties not found in nature, often designed to manipulate electromagnetic waves in unusual ways. Diffraction principles are crucial in their design. By creating subwavelength structures that cause specific diffraction effects, engineers can control how waves propagate through the material. This allows for exotic effects like negative refraction or the creation of "superlenses" that overcome the diffraction limit.
Q: What is the role of diffraction in the operation of acousto-optic devices?
A:
Acousto-optic devices use the interaction between sound and light waves to manipulate optical beams. Diffraction is central to their operation. Sound waves create a periodic variation in the refractive index of a material, effectively creating a diffraction grating. Light passing through this dynamic grating is diffracted, allowing the sound waves to control the direction or frequency of the light.
Q: How does diffraction contribute to the formation of speckle patterns in laser light?
A:
Speckle patterns are the grainy appearance of laser light when it illuminates a rough surface. These patterns result from the interference of coherent light waves that have been diffracted by the microscopic irregularities on the surface. Each point on the rough surface acts as a source of diffracted waves, which then interfere to create the characteristic speckle pattern.
Q: What is the relationship between diffraction and the resolution of digital cameras?
A:
Diffraction affects digital camera resolution, especially when using small apertures (high f-numbers). As the aperture size decreases, diffraction increases, causing each point of light to spread out over multiple pixels. This diffraction limit can reduce the overall sharpness of the image, even if the sensor has a high pixel count. Camera designers must balance this effect with other factors like depth of field.
Q: How does diffraction contribute to the formation of optical vortices?
A:
Optical vortices are regions in an optical field where the phase is indeterminate, often resulting in a dark core surrounded by a bright ring. Diffraction plays a crucial role in creating and shaping these vortices. Special diffractive elements, like spiral phase plates or computer-generated holograms, can impart an azimuthal phase structure to a beam, causing it to diffract into a vortex shape.
Q: How does diffraction affect the performance of telescopes?
A:
Diffraction sets a fundamental limit on telescope resolution. Even with perfect optics, a point source of light forms an Airy disk due to diffraction at the telescope's aperture. The size of this disk determines the telescope's ability to resolve close objects. Larger apertures produce smaller Airy disks, allowing better resolution, which is why larger telescopes can see finer details.
Q: What is the Talbot effect in diffraction?
A:
The Talbot effect is a near-field diffraction effect where a periodic structure (like a diffraction grating) creates repeated images of itself at regular distances from the grating. These self-images occur at integer multiples of the Talbot distance, which depends on the grating period and the wavelength of light. This effect has applications in imaging, metrology, and lithography.
Q: What is the significance of the Fresnel number in diffraction?
A:
The Fresnel number is a dimensionless quantity used in diffraction theory to determine whether a diffraction problem should be treated using near-field (Fresnel) or far-field (Fraunhofer) approximations. It's defined as F = a²/(λL), where a is the characteristic size of the aperture, λ is the wavelength, and L is the distance to the observation plane. When F is much less than 1, far-field approximations are valid.
Q: How does diffraction affect the design of photonic crystals?
A:
Photonic crystals are materials with periodic structures designed to control the flow of light. Diffraction is a key principle in their operation. The periodic structure causes light to diffract in specific ways, creating photonic band gaps where certain wavelengths cannot propagate. By carefully designing the crystal structure, engineers can control how light diffracts within the material, enabling various optical devices and effects.
Q: How does diffraction affect the operation of diffraction gratings in spectrometers?
A:
In spectrometers, diffraction gratings use the principle of diffraction to separate light into its component wavelengths. As light diffracts from the grating's periodic structure, different wavelengths are sent in different directions due to constructive interference at specific angles. The grating equation relates the diffraction angle to the wavelength and grating spacing, allowing precise spectral analysis.