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Question

The refracting angle of a prism is $A$. The refractive index of the material of the prism is $\frac{1+\cos A}{\sin A}$. The angle of minimum deviation is:

The correct answer is
$180^\circ - 2A$

Understanding Prism Optics: Calculating Minimum Deviation

This problem involves understanding the relationship between a prism's geometry, its material properties, and how it affects light, specifically focusing on the angle of minimum deviation. We are given the refracting angle $A$ and a specific expression for the refractive index $\mu$ of the prism material. Our goal is to find the angle of minimum deviation, often denoted as $\delta_{min}$.

Key Concepts and Formulas

  • The relationship between the refractive index ($\mu$), refracting angle ($A$), and the angle of minimum deviation ($\delta_{min}$) for a prism is given by the prism formula: $ \mu = \frac{\sin\left(\frac{A+\delta_{min}}{2}\right)}{\sin\left(\frac{A}{2}\right)} $
  • We will also need some basic trigonometric identities to simplify the given refractive index expression:
    • $1 + \cos \theta = 2\cos^2\left(\frac{\theta}{2}\right)$
    • $\sin \theta = 2\sin\left(\frac{\theta}{2}\right)\cos\left(\frac{\theta}{2}\right)$

Step-by-Step Derivation

Let's break down the calculation step-by-step:

  1. Simplify the Refractive Index: We are given the refractive index $\mu = \frac{1+\cos A}{\sin A}$. Let's use the trigonometric identities mentioned above to simplify this expression. Replace $1 + \cos A$ with $2\cos^2\left(\frac{A}{2}\right)$ and $\sin A$ with $2\sin\left(\frac{A}{2}\right)\cos\left(\frac{A}{2}\right)$. $ \mu = \frac{2\cos^2\left(\frac{A}{2}\right)}{2\sin\left(\frac{A}{2}\right)\cos\left(\frac{A}{2}\right)} $ Now, cancel out the common terms ($2$ and $\cos\left(\frac{A}{2}\right)$), assuming $\cos\left(\frac{A}{2}\right) \neq 0$ (which is true for typical prism angles $A$). $ \mu = \frac{\cos\left(\frac{A}{2}\right)}{\sin\left(\frac{A}{2}\right)} $ Recall that $\cot \theta = \frac{\cos \theta}{\sin \theta}$. Therefore, $ \mu = \cot\left(\frac{A}{2}\right) $
  2. Apply the Prism Formula: Now we substitute this simplified expression for $\mu$ into the prism formula: $ \cot\left(\frac{A}{2}\right) = \frac{\sin\left(\frac{A+\delta_{min}}{2}\right)}{\sin\left(\frac{A}{2}\right)} $
  3. Solve for the Angle of Minimum Deviation ($\delta_{min}$): To solve for $\delta_{min}$, we can first rewrite $\cot\left(\frac{A}{2}\right)$ as $\frac{\cos\left(\frac{A}{2}\right)}{\sin\left(\frac{A}{2}\right)}$. $ \frac{\cos\left(\frac{A}{2}\right)}{\sin\left(\frac{A}{2}\right)} = \frac{\sin\left(\frac{A+\delta_{min}}{2}\right)}{\sin\left(\frac{A}{2}\right)} $ Multiply both sides by $\sin\left(\frac{A}{2}\right)$: $ \cos\left(\frac{A}{2}\right) = \sin\left(\frac{A+\delta_{min}}{2}\right) $ We know the trigonometric identity $\cos \theta = \sin\left(\frac{\pi}{2} - \theta\right)$ or $\sin(90^\circ - \theta)$. Using degrees, we have $\cos\left(\frac{A}{2}\right) = \sin\left(90^\circ - \frac{A}{2}\right)$. Substituting this into our equation: $ \sin\left(90^\circ - \frac{A}{2}\right) = \sin\left(\frac{A+\delta_{min}}{2}\right) $ For the sine function, if $\sin x = \sin y$, then $x = y$ (considering the principal values relevant for prism angles). Therefore, we can equate the arguments: $ 90^\circ - \frac{A}{2} = \frac{A+\delta_{min}}{2} $ Multiply the entire equation by 2: $ 180^\circ - A = A + \delta_{min} $ Now, isolate $\delta_{min}$: $ \delta_{min} = 180^\circ - A - A $ $ \delta_{min} = 180^\circ - 2A $

Conclusion on Minimum Deviation

By simplifying the given refractive index expression and applying the standard prism formula for minimum deviation, we find that the angle of minimum deviation is $180^\circ - 2A$. This result depends directly on the prism's refracting angle $A$ and the specific refractive index provided.

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Important Questions from Refraction and Reflection

  1. A convex lens of focal length f will form a magnified real image of an object, if the object is placed.

  2. A ray of light travelling in the direction \(\frac{1}{2} (\hat i + \sqrt 3 \hat j)\) is incident on a plane mirror. After reflection it travels along the direction  \(\frac{1}{2} (\hat i - \sqrt 3 \hat j)\)  The angle of incidence is:

  3. Twinkling of stars is due to atmospheric

  4. An optical fibre has a core material of refractive index of 1.55 and cladding material of refractive index of 1.50. The numerical aperture of the fibre is

  5. An object is placed on the principal axis of a convex lens at a point between F 1 and 2 F 1 (F 1 is the principal focus to the left of the lens). The image formed is:

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