/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 49 A circular beam of light of diam... [FREE SOLUTION] | 91Ó°ÊÓ

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A circular beam of light of diameter \(d=2 \mathrm{~cm}\) falls on a plane surface of glass. The angle of incidence is \(60^{\circ}\) and refractive index of glass is \(\mu=3 / 2 .\) The diameter of the refracted beam is (A) \(4.0 \mathrm{~cm}\) (B) \(3.0 \mathrm{~cm}\) (C) \(3.26 \mathrm{~cm}\) (D) \(2.52 \mathrm{~cm}\)

Short Answer

Expert verified
The diameter of the refracted beam is approximately \(3.26 \text{ cm}\) (option C).

Step by step solution

01

Applying Snell's Law

We will use Snell's Law, which is given by: \[n_1\sin\theta_1 = n_2\sin\theta_2\] Where, \(n_1\) is the refractive index of the medium through which the light is incident (air), \(n_2\) is the refractive index of the medium through which the light is refracted (glass), \(\theta_1\) is the angle of incidence, and \(\theta_2\) is the angle of refraction. Since the refractive index of air is \(1\), we can find the angle of refraction, \(\theta_2\) as follows: \[\sin\theta_2 = \frac{n_1\sin\theta_1}{n_2}\]
02

Calculate the angle of refraction

Now, let's calculate the angle of refraction \(\theta_2\) using the values given in the problem: wavelength of light in air = 60º refractive index of glass, \(\mu\) = \(3/2\) \[\sin\theta_2 = \frac{\sin 60^\circ}{\frac{3}{2}} = \frac{1}{2(\frac{3}{2})} = \frac{1}{3}\] To obtain the angle of refraction, we can take the arcsin of \(\sin\theta_2\): \[\theta_2 = \arcsin\frac{1}{3}\]
03

Calculate the diameter of refracted beam

Consider the incident and refracted beams as right-angled triangles with height \(h\) and base length equal to half the diameter (\(d/2\)). Now, apply the tangent function to the incident and refracted beams: For the incident beam, \[\tan 60^\circ = \frac{h}{d_1/2}\] As for the refracted beam, \[\tan \theta_2 = \frac{h}{d_2/2}\] Now, divide the equation of the refracted beam by the incident beam equation: \[\frac{\tan \theta_2}{\tan 60^\circ} = \frac{d_1/2}{d_2/2}\] Plug in the values, \(\tan 60^\circ\) and \(\tan \theta_2\), as well as the diameter of the incident beam, \(d_1 = 2 \text{ cm}\), into the equation: \[\frac{\tan (\arcsin(1/3))}{\tan 60^\circ} = \frac{2}{d_2}\] Solve for the diameter of the refracted beam (\(d_2\)): \[d_2 = 2 \cdot \frac{\tan 60^\circ}{\tan (\arcsin(1/3))}\]
04

Find the diameter of the refracted beam

All we need to do now is evaluate the expression and round the result to a reasonable accuracy: \[d_2 = 2 \cdot \frac{\tan 60^\circ}{\tan (\arcsin(1/3))} \approx 3.26 \text{ cm}\] Hence, the diameter of the refracted beam is \(3.26 \text{ cm}\) (option C).

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Key Concepts

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

Angle of Incidence
When light moves from one medium to another, it typically changes direction and speed, a phenomenon called refraction. The angle of incidence is crucial in understanding this behavior. It is the angle between the incoming light beam and the normal (an imaginary line perpendicular to the surface) drawn at the point of incidence.
  • The angle of incidence helps in determining how the light will bend when entering a different medium.
  • This angle is usually measured in degrees.
  • In the provided problem, the angle of incidence is \(60^\u200bc\), meaning the light beam hits the glass at an angle of 60 degrees relative to the normal.
Knowing the angle of incidence is the first step in applying Snell's Law, which we will discuss shortly. This angle helps in predicting the light path as it enters or exits a medium like glass.
Refractive Index
The refractive index is a measure of how much light slows down and bends when entering a new medium, like glass from air. It is usually denoted by the symbol \(n\).
  • The refractive index of a material determines the extent to which light will bend upon entering it.
  • A higher refractive index means light slows down more and bends at a greater angle.
  • For air, the refractive index is typically 1, whereas, for glass, it can be around 1.5, as in this problem, where it is given as \(\mu=\frac{3}{2}\).
This refractive index is an essential component when using Snell's Law, which calculates how much the light will deviate from its original path when it passes through the boundary of two different media.
Angle of Refraction
The angle of refraction is the angle between the refracted beam of light and the normal line in the new medium.
  • This angle can be calculated using Snell's Law, combining the angle of incidence and the refractive indexes of the two media involved.
  • In our example problem, as the light moves from air into glass, the angle of refraction can be found using: \(\sin\theta_2 = \frac{\sin 60^\circ}{\frac{3}{2}}\).
  • Upon calculation, the angle \(\theta_2\), which is the angle of refraction, ends up being the arcsin of \(\frac{1}{3}\).
Understanding this angle is vital for determining the path of light within the second medium, such as finding the diameter of the refracted beam that results from the incident beam entering the glass sheet.

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Most popular questions from this chapter

On a hot summer night, the refractive index of air is smallest near the ground and increases with height from the ground. When a light beam is directed horizontally, the Huygens' principle leads us to conclude that as it travels, the light beam [2015] (A) goes horizontally without any deflection (B) bends downwards (C) bends upwards (D) becomes narrower

A thin rod of length \(f / 3\) is placed along the optic axis of a concave mirror of focal length \(f\) such that its image, which is real and elongated, just touches the rod. The magnification is (A) 2 (B) 4 (C) \(2.4\) (D) \(1.5\)

At a point on the screen in YDSE, third maximum is observed at \(t=0\). Now screen is slowly moved with constant speed away from the slits in such a way that the centre of slits and centre of screen lie on same line always and at \(t=1 \mathrm{~s}\), the intensity at that point is observed to be \(\left(\frac{3}{4}\right)^{\text {th }}\) of maximum intensity in between second and third maximum. The speed of screen will be \((D=1 \mathrm{~m})\) (A) \(\frac{5}{13} \mathrm{~m} / \mathrm{s}\) (B) \(\frac{5}{12} \mathrm{~m} / \mathrm{s}\) (C) \(\frac{12}{5} \mathrm{~m} / \mathrm{s}\) (D) \(\frac{13}{5} \mathrm{~m} / \mathrm{s}\)

\(A B C\) is a right-angled prism kept in air. A ray (1) is incident on the face \(A B\) along the normal. Refractive index of the material of prism is the minimum value that will be required so that ray (1) undergoes total internal reflection at the face \(A C\). Another ray ( 2 ) is incident on the face \(A B\) such that it emerges from face \(A C\) along the normal to \(A C\). A third ray (3) falls on the face \(B C\) and emerges from face \(A C\) such that its angle of emergence is the same as that of incidence. Assuming light \((1),(2)\), and (3) have the same wavelength, then match the following. \(A\)(A) Refractive index of the material 1\. 120 of prism is (B) Angle of incidence in degree of \(2.90\) ray \((2)\) is (C) Deviation in degree suffered by 3\. 2 ray (2) is (D) Deviation in degree suffered by 4\. 60 ray (3) is 5. \(1.5\)

When an object is placed at a distance of \(25 \mathrm{~cm}\) from a mirror, the magnification is \(m_{1} .\) The object is moved \(15 \mathrm{~cm}\) away with respect to the earlier position along principal axis, magnification becomes \(m_{2}\). If \(m_{1} \times m_{2}=4\), the focal length of the mirror is (A) \(10 \mathrm{~cm}\) (B) \(30 \mathrm{~cm}\) (C) \(15 \mathrm{~cm}\) (D) \(20 \mathrm{~cm}\)

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