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Light of wavelength \(585 \mathrm{nm}\) falls on a slit \(0.0666 \mathrm{~mm}\) wide. (a) On a very large distant screen, how many totally dark fringes (indicating complete cancellation) will there be, including both sides of the central bright spot? Solve this problem without calculating all the angles! (Hint: What is the largest that \(\sin \theta\) can be? What does this tell you is the largest that \(m\) can be?) (b) At what angle will the dark fringe that is most distant from the central bright fringe occur?

Short Answer

Expert verified
(a) 228 dark fringes. (b) At an angle approaching 90°.

Step by step solution

01

Understand the Single-Slit Diffraction Condition

In a single-slit diffraction pattern, dark fringes (minima) occur at angles \( \theta \) such that the path difference creates complete destructive interference. This is given by the formula: \[ a \sin \theta = m \lambda \]where \( a \) is the slit width, \( \lambda \) is the wavelength of the light, and \( m \) is the order of the minimum (m = 1, 2, 3,...). The angle \( \theta \) represents the angle at which these dark fringes appear.
02

Consider the Range of Sin θ

The sine function \( \sin \theta \) has possible values ranging from -1 to 1. This means that the largest value \( \sin \theta \) can achieve is 1, and the smallest is -1. This constraint determines the maximum value \( m \) can take.
03

Calculate the Maximum Order m

To find the maximum order \( m \), use the condition where \( \sin \theta = 1 \):\[ a = m \lambda \]Rearranging gives: \[ m = \frac{a}{\lambda} \]Substitute \( a = 0.0666 \text{ mm} = 66.6 \text{ } \mu \text{m} = 66.6 \times 10^{-6} \text{ m} \) and \( \lambda = 585 \text{ nm} = 585 \times 10^{-9} \text{ m} \) to find \( m \):\[ m = \frac{66.6 \times 10^{-6}}{585 \times 10^{-9}} \approx 114 \]Thus, the possible values of \( m \) extend from -114 to 114, except \( m = 0 \) because that would indicate the central bright spot.
04

Determine the Total Number of Dark Fringes

Since \( m \) ranges from -114 to 114 with 0 counted only once, the total number of dark fringes is:\[ 2 \times 114 = 228 \]This includes all dark fringes on both sides of the central bright spot.
05

Find the Angle of the Most Distant Dark Fringe

The most distant dark fringe occurs at the maximum possible \( m \), which we found to be 114. Substitute \( m = 114 \) into the diffraction condition with \( \sin \theta = 1 \).Since \( \sin \theta = 1 \) corresponds to \( \theta = 90^{\circ} \), this shows that the extreme edges of the diffraction pattern reach the maximum limit of \( \sin \theta \). As \( \theta \) cannot practically exceed this, we confirm that the largest \( \theta \) is just approaching 90°.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Diffraction Pattern
When light passes through a single slit, it doesn't just keep traveling in a straight line. Instead, it spreads out, creating a distinct pattern called a diffraction pattern. This pattern is typically observed on a screen positioned far away from the slit. The pattern consists of alternating bright and dark areas known as fringes. At the center, there is a bright fringe, and on both sides, there are multiple dark and bright fringes.
Different light wavlengths, like the one given in the problem, create different diffraction patterns. This means the specific arrangement of dark and bright fringes is directly related to the properties of the light wave and the slit. In single-slit diffraction, the dark fringes appear at specific angles where the light waves interfere destructively, which we'll explore in the next section.
Destructive Interference
Destructive interference is a key concept when explaining the dark fringes found in a diffraction pattern. This occurs when waves overlap in such a way that they cancel each other out, leading to areas of darkness on the screen. In a single-slit diffraction scenario, this happens when the light traveling through the slit meets itself in such a way that the crest of one wave aligns with the trough of another.
The condition for complete destructive interference (where we see a dark fringe) in single-slit diffraction can be described mathematically by the equation: \[ a \sin \theta = m \lambda \]where:
  • \( a \) is the width of the slit
  • \( \lambda \) is the wavelength of light
  • \( m \) is the integer order marking the fringe (1, 2, 3, ...)
Using this formula, we can predict where the dark fringes will appear by determining the specific angles \( \theta \) where the light interferes destructively.
Path Difference
The path difference in diffraction is the extra distance that some light waves have traveled compared to others. This difference in distance is critical in determining whether we will observe constructive or destructive interference at a certain point on the screen.
In the case of single-slit diffraction, the path difference is given by the width of the slit and the angle at which the light waves meet each other after passing through the slit. For destructive interference, this path difference results in the condition:\[ a \sin \theta = m \lambda \],where the light waves cancel out and we see a dark fringe. This equation is pretty straightforward, but it's powerful because it allows us to understand and predict the formation of dark fringes in the diffraction pattern.
Diffraction Angle Calculation
Calculating the diffraction angle involves determining the specific angles \( \theta \) at which destructive interference occurs. To find these, we use the diffraction condition:\[ a \sin \theta = m \lambda \],where \( m \) is the order of the dark fringe. For the problem at hand, students need to recognize that the range of \( \sin \theta \) is restricted from -1 to 1, which significantly limits \( m \).
Practically, the largest value that \( \sin \theta \) can take is 1, which simplifies the calculation of \( m \):\[ m = \frac{a}{\lambda} \]Given \( a = 0.0666 \text{ mm} \) and \( \lambda = 585 \text{ nm} \), substituting these values allows us to calculate \( m \approx 114 \). Hence, the diffraction angle for the most distant dark fringe approaches 90°, as the sine of 90° is 1. This explanation provides a clear comprehension of the calculation process used in the exercise.

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Most popular questions from this chapter

When viewing a piece of art that is behind glass, one often is affected by the light that is reflected off the front of the glass (called glare), which can make it difficult to see the art clearly. One solution is to coat the outer surface of the glass with a thin film to cancel part of the glare. (a) If the glass has a refractive index of 1.62 and you use \(\mathrm{TiO}_{2},\) which has an index of refraction of \(2.62,\) as the coating, what is the minimum film thickness that will cancel light of wavelength \(505 \mathrm{nm} ?\) (b) If this coating is too thin to stand up to wear, what other thicknesses would also work? Find only the three thinnest ones.

Coherent light with wavelength \(600 \mathrm{nm}\) passes through two very narrow slits, and the interference pattern is observed on a screen \(3.00 \mathrm{~m}\) from the slits. The first-order bright fringe is at \(4.84 \mathrm{~mm}\) from the center of the central bright fringe. For what wavelength of light will the first-order dark fringe be observed at this same point on the screen?

Coherent light of frequency \(6.32 \times 10^{14} \mathrm{~Hz}\) passes through two thin slits and falls on a screen \(85.0 \mathrm{~cm}\) away. You observe that the third bright fringe occurs at \(\pm 3.11 \mathrm{~cm}\) on either side of the central bright fringe. (a) How far apart are the two slits? (b) At what distance from the central bright fringe will the third dark fringe occur?

A uniform thin film of material of refractive index 1.40 coats a glass plate of refractive index \(1.55 .\) This film has the proper thickness to cancel normally incident light of wavelength \(525 \mathrm{nm}\) that strikes the film surface from air, but it is somewhat greater than the minimum thickness to achieve this cancellation. As time goes by, the film wears away at a steady rate of \(4.20 \mathrm{nm}\) per year. What is the minimum number of years before the reflected light of this wavelength is now enhanced instead of canceled?

Coherent light from a sodium-vapor lamp is passed through a filter that blocks everything except for light of a single wavelength. It then falls on two slits separated by \(0.460 \mathrm{~mm}\). In the resulting interference pattern on a screen \(2.20 \mathrm{~m}\) away, adjacent bright fringes are separated by \(2.82 \mathrm{~mm}\). What is the wavelength of the light that falls on the slits?

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