Question #49307

In a single slit Fraunhofer diffraction experiment, a light source of wavelength 600 nm is used. Calculate the angular spread of the central maxima and angular positions of second and third minima if the widths of the slit are following:
1 mm
2.2 µm
1

Expert's answer

2014-11-25T00:48:48-0500

Answer on Question #49307, Engineering, Other

In a single slit Fraunhofer diffraction experiment, a light source of wavelength 600nm600\mathrm{nm} is used. Calculate the angular spread of the central maxima and angular positions of second and third minima if the widths of the slit are following:

1 mm

2.2 μ\mu m

Solution:

The Fraunhofer diffraction equation is used to model the diffraction of waves when the diffraction pattern is viewed at a long distance from the diffracting object.

The diffraction at a single slit of width dd is shown in Figure 1. Diffraction occurs in all directions to the right of the slit.



Fig.1. Graph and image of single-slit diffraction

The pattern consists of a central bright fringe (band) flanked by much weaker maxima alternating with dark fringes.

The general condition for a minimum for a single slit is:


mλ=dsinθm \lambda = d \sin \theta


where m=1,2,3,4m = 1,2,3,4 and so on

- dd is the width of the slit,

- θ\theta is the angle at which the minimum intensity occurs, and

- λ\lambda is the wavelength of the light

1. d=1 mmd = 1 \mathrm{~mm}

The angular spread of the central maximum is the angular fringe width of the central maximum.

Thus,


sinθ0=2λd=26001091103=12104\sin \theta_ {0} = \frac {2 \lambda}{d} = \frac {2 * 6 0 0 * 1 0 ^ {- 9}}{1 * 1 0 ^ {- 3}} = 1 2 * 1 0 ^ {- 4}


As the angle is very small we can use the relation, sinθ=θ\sin \theta = \theta.

Hence,


θ0=0.0012rad=0.069\theta_0 = 0.0012 \mathrm{rad} = 0.069^\circ


The positions of second and third minima are:


sinθ2=2λd=600×1091×103=12×104\sin \theta_2 = \frac{2\lambda}{d} = \frac{600 \times 10^{-9}}{1 \times 10^{-3}} = 12 \times 10^{-4}θ2=0.0012rad=0.069\theta_2 = 0.0012 \mathrm{rad} = 0.069^\circsinθ3=3λd=3×600×1091×103=18×104\sin \theta_3 = \frac{3\lambda}{d} = \frac{3 \times 600 \times 10^{-9}}{1 \times 10^{-3}} = 18 \times 10^{-4}θ3=0.0018rad=0.1\theta_3 = 0.0018 \mathrm{rad} = 0.1^\circ


2. d=2 μmd = 2\ \mu\mathrm{m}

The angular spread of the central maximum is the angular fringe width of the central maximum.

Thus,


sinθ0=2λd=2×600×1092×106=0.6\sin \theta_0 = \frac{2\lambda}{d} = \frac{2 \times 600 \times 10^{-9}}{2 \times 10^{-6}} = 0.6


Hence,


θ0=sin10.6=0.644rad=36.9\theta_0 = \sin^{-1} 0.6 = 0.644 \mathrm{rad} = 36.9^\circ


The positions of second and third minima are:


sinθ2=2λd=2×600×1092×106=0.6\sin \theta_2 = \frac{2\lambda}{d} = \frac{2 \times 600 \times 10^{-9}}{2 \times 10^{-6}} = 0.6θ2=sin10.6=0.644rad=36.9\theta_2 = \sin^{-1} 0.6 = 0.644 \mathrm{rad} = 36.9^\circsinθ3=3λd=3×600×1092×106=0.9\sin \theta_3 = \frac{3\lambda}{d} = \frac{3 \times 600 \times 10^{-9}}{2 \times 10^{-6}} = 0.9θ3=sin10.9=1.12rad=64.2\theta_3 = \sin^{-1} 0.9 = 1.12 \mathrm{rad} = 64.2^\circ


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