Angular Width and Linear Width of the Central Maximum

Physics · Wave Optics · NEET

In single-slit diffraction the bright central maximum lies between the two first minima. Its angular width (full angle) is 2*lambda/a and its linear width on a screen is 2*D*lambda/a, where lambda is the wavelength, a is the slit width, and D is the slit-to-screen distance. Memory hook: "central bright is TWICE as wide" - it is 2 times bigger than each side band, and every width formula here starts with a 2 because you count minima on BOTH sides.
ascreenfirst minfirst min2Dλ/aθ = λ/aDSingle-slit central maximum
Light through a slit of width a spreads to the first minima on both sides at angle lambda/a. The bright central maximum spans the full angular width 2*lambda/a and has linear width 2*D*lambda/a on a screen at distance D.

Your doubts, answered

Is the angular width lambda/a or 2 lambda/a?

Both are correct but they mean different things. The first minimum sits at angle theta = lambda/a from the centre. That lambda/a is the HALF angular width (centre to one edge). The FULL angular width is the angle from the first minimum on the left to the first minimum on the right, so you double it: full angular width = 2*lambda/a. In NEET, 'angular width of central maximum' almost always means the full value 2*lambda/a. Read the question: if it says 'width of central maximum' use 2*lambda/a; if it asks 'position of first minimum' use lambda/a.

What is the difference between angular width and linear width?

Angular width is an angle measured in radians (2*lambda/a). Linear width is an actual length on the screen measured in metres or cm. You convert angle to length by multiplying by the screen distance D. So linear width = D * (angular width) = D * 2*lambda/a = 2*D*lambda/a. Angular width does not depend on D; linear width does. Move the screen back and the patch of light gets physically wider, but the angle stays the same.

Why is the central maximum twice as wide as the other bright fringes?

The central maximum stretches from the first minimum on one side to the first minimum on the other side, so it covers two 'units' of width. Every other bright band sits between two neighbouring minima that are only one unit apart. Spacing between successive minima on the screen is D*lambda/a, so a side maximum has width D*lambda/a, but the central one has width 2*D*lambda/a - exactly twice. This is why the central maximum is the brightest and the widest.

How does the central maximum change if I make the slit wider?

Angular width = 2*lambda/a, so a and width are inversely related. Make the slit wider (larger a) and the central maximum gets narrower and sharper. Make the slit very narrow (small a) and it spreads out wide. In the limit of a very wide slit, the pattern shrinks to a single sharp point - that is why ray optics (a straight-line beam) works when the slit is large compared to the wavelength.

What happens to the central maximum when the setup is put in water?

Inside a medium of refractive index n the wavelength shrinks to lambda/n. Since width is proportional to lambda, the angular width becomes 2*lambda/(n*a) - it decreases by the factor n. For water (n = 4/3) the width becomes 3/4 of its air value. Frequency and slit width do not change, only the wavelength does, so the pattern gets narrower.

⚠️ The NEET trap
Angular width of the central maximum = lambda/a
Angular width of the central maximum = 2*lambda/a (because it spans the first minima on BOTH sides). lambda/a is only the half width or the position of the first minimum.
🧠 Central bright counts TWO minima - always start the width formula with a 2.

Real NEET questions

NEET 2019 Odisha

The angular width of the central maximum in the Fraunhofer diffraction for lambda = 6000 A is theta0. When the same slit is illuminated by another monochromatic light, the angular width decreases by 30%. The wavelength of this light is

A · 1800 A
B · 4200 A
C · 6000 A
D · 420 A
Solution: Angular width of central maximum = 2*lambda/a, so it is directly proportional to lambda (slit width a is fixed). A 30% decrease means the new width is 70% of the old, so the new wavelength is 70% of the old wavelength. lambda' = 0.70 * 6000 = 4200 A. Answer (B).
NEET 2016 Phase 2

A linear aperture whose width is 0.02 cm is placed immediately in front of a lens of focal length 60 cm. The aperture is illuminated normally by a parallel beam of wavelength 5 x 10^-5 cm. The distance of the first dark band of the diffraction pattern from the centre of the screen is

A · 0.10 cm
B · 0.25 cm
C · 0.20 cm
D · 0.15 cm
Solution: The first dark band (first minimum) is at the edge of the central maximum, at distance y = f * (lambda/a) = half the linear width. Here f = 60 cm plays the role of D. y = 60 * (5 x 10^-5) / 0.02 = 60 * 0.0025 = 0.15 cm. Answer (D). Note: this is the HALF width; the full central maximum would be 0.30 cm.
NEET 2019

In a double slit experiment, when light of wavelength 400 nm was used, the angular width of the first minima formed on a screen placed 1 m away, was found to be 0.2 degree. What will be the angular width of the first minima, if the entire experimental apparatus is immersed in water? (n_water = 4/3)

A · 0.266 degree
B · 0.15 degree
C · 0.05 degree
D · 0.1 degree
Solution: Angular width is proportional to wavelength. In water the wavelength becomes lambda/n, so the angular width becomes (angular width in air)/n = 0.2 / (4/3) = 0.2 * 3/4 = 0.15 degree. Screen distance D does not affect angular width. Answer (B).

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Frequently asked

What is the formula for the angular width of the central maximum?

Angular width (full) = 2*lambda/a, where lambda is the wavelength of light and a is the slit width. The half angular width (centre to first minimum) is lambda/a.

What is the linear width of the central maximum?

Linear width = 2*D*lambda/a, where D is the distance from the slit to the screen. It is the angular width multiplied by D, giving an actual length on the screen.

Does the angular width depend on the screen distance D?

No. Angular width = 2*lambda/a contains no D, so moving the screen does not change the angle. Only the linear width (2*D*lambda/a) changes with D because the same angle spreads over a longer distance.

Why is the central maximum brighter and wider than the side maxima?

All waves from the slit arrive nearly in phase at the centre, giving maximum intensity. It is also twice as wide (2*D*lambda/a) because it spans the first minima on both sides, while each side maximum is only D*lambda/a wide.

How do you get the linear width from the angular width?

Multiply the angular width by the screen distance D. Since the angle is small, width on screen = D * angle = D * 2*lambda/a = 2*D*lambda/a.