Light is weird: if you shine a beam on a material covered in finely spaced apertures, it spreads out at specific angles in a phenomenon called diffraction: learn more with our diffraction grating calculator.

Here you will learn:

  • What is diffraction;
  • What is a diffraction grating;
  • What happens when a light beam shines on a diffraction grating;
  • The formula of a diffraction grating: how to calculate the diffraction angles.

What is diffraction

Diffraction is a physical phenomenon that occurs in the presence of periodic, wave-like motions. Under a purely classical analysis, diffraction arises when a wavefront meets a small opening. The opening becomes a secondary propagation point, from which circular waves expand outward.

Diffraction at Bernier and Dorre islands.
The small opening between the Bernier and Dorre islands creates beautiful diffraction patterns. Credits: Google Earth/Maxar Technologies.

If you open more than a slit near the other, the newly formed *wavefronts can interfere, thus reinforcing or dampening each other. We owe this explanation of diffraction to the Huygens-Fresnel principle.

The story is slightly different when it comes to light since it behaves both as a wave (carrying energy) and as a particle (carrying momentum). We need to introduce diffraction gratings.

Diffraction gratings

A diffraction grating is a material covered in regularly spaced multiple small slits. The dimensions involved are micrometric or even nanometric, that's a requirement depending on the characteristic scale of visible light.

When a light beam meets a diffraction grating, the oscillatory nature of photons causes the beam to change direction. The behavior in the presence of multiple slits resembles one of "conventional" waves (like the ones in the ocean).

Diffraction gratings can be reflective (acting as mirrors) or transmissive (acting as lenses). It may sound unlikely, but you can easily find examples of both in everyday life. CDs are good reflective gratings/ Shine a light on them, and they will iridesce, point a laser and you'll see the characteristic pattern. Feathers are transmissive gratings: the phenomenon was first observed thanks to them.

A monochromatic light ray incident on a diffraction grating creates a characteristic interference pattern. As said, each slit in the grating acts as a new propagation point: from there the light creates circular, concentric wavefronts. If we consider the optical path of the light from each slit, we can intuitively think that there will be angles at which the diffracted beams will meet when they are in the same phase. This situation corresponds to constructive interference. If the beams are entirely out of phase at the intersection, we have destructive interference. These two situations correspond, respectively, to bright and dark spots on a screen placed behind the grating. A similar phenomenon occurs in anti-reflective coating: learn more at our thin-film interference calculator.

But how do we calculate the directions at which these spots originate? We need to learn how to find the diffraction angle.

🙋 The oscillatory nature of light was proven by an experiment involving interference after the diffraction of a light beam by a double slit diffraction grating: we are talking of the famous Young experiment.

How to calculate the diffraction angles in a diffraction grating

Our diffraction grating calculator implements the equation to calculate the diffraction angle. Suppose we shine a monochromatic beam with wavelength λ\lambda perpendicular to a diffraction grating with spacing dd. In that case, we find that the angles at which we find constructive interference are given by the equation:

mλ=dsinθmm\cdot \lambda = d\cdot \sin{\theta_{\text{m}}}

Where:

  • mm is any non-negative integer; and
  • θm\theta_{\text{m}} is the mth angle in the diffraction pattern.

🙋 If we take m=0m=0, we would have zero-order diffraction, with the spot being the brightest of the diffraction pattern and subject to no diffraction.

Let's learn how to find the diffraction angles in the more general situation of a non-perpendicular incident beam.

Assuming that the beam hits the diffraction grating with angle θi\theta_{\text{i}} we can calculate the diffraction grating pattern angles with the following formula:

mλ=d[sin(θm)+sin(θi)]m\cdot \lambda = d\cdot \left[\sin{(\theta_{\text{m}})}+\sin{(\theta_{\text{i}})}\right]

This is the formula we implemented in our diffraction grating calculator. We will calculate the first five orders of the diffracted beam, neglecting the trivial order zero. Let's check an example.

Take a laserbeam with λ=650 nm\lambda =650\ \text{nm}, and point it perpendicularly on a CD. The distance between tracks on a compact disk is 1.6 μm1.6\ \text{μm}. Let's calculate the angle of diffraction for m=1, 2, 3, 4, 5m = 1,\ 2,\ 3,\ 4,\ 5:

m=1θ1=arcsinλd=6501600=23.97°m=2θ2=arcsin2λd=26501600=54.34°\begin{align*} &m=1\rightarrow\\ &\theta_1 = \arcsin{\frac{\lambda}{d}}= \frac{650}{1600}= 23.97\degree\\ \\ &m=2\rightarrow\\ &\theta_2 = \arcsin{\frac{2\cdot \lambda}{d}}= \frac{2\cdot 650}{1600}= 54.34\degree\\ \end{align*}

Higher orders yield complex values, and we are not interested in them.

Non-monochromatic beams shining on diffraction gratings

If a non-monochromatic (continuous) light beam shines on a diffraction grating, the various wavelength will deviate at different angles following the formula above. The result is a separation of the colors, with the characteristic emergence of iridescence. Try it with a CD!

Davide Borchia
Wavelength
nm
Grating density
lines/
mm
Angle of incidence
deg
Diffracted images
First order
deg
Second order
deg
Third order
deg
Fourth order
deg
Fifth order
deg
People also viewed…

Schwarzschild radius

Discover the fundamental of black hole physics with our Schwarzschild radius calculator.

Signal-to-noise ratio

This signal-to-noise ratio calculator finds the ratio of the desired signal to the level of the background noise.

Speed of sound

Use the speed of sound calculator to estimate the speed of sound in dry air and water for various temperatures.
main background