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When a beam of light goes from denser me...

When a beam of light goes from denser medium (`mu_d`) to rarer medium (`mu_r`), then it is generally observed that magnitude of angle of incidence is half that of angle of refraction. Then magnitude of incident angle will be-(here `mu=mu_d //mu_r`)

A

`2sin^(-1) (mu/2)`

B

`2 cos^(-1)mu`

C

`cos^(-1)(mu/2)`

D

`2cos^(-1)(mu/2)`

Text Solution

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The correct Answer is:
To solve the problem, we will follow these steps: ### Step 1: Understand the relationship between angles of incidence and refraction Given that the angle of incidence \( I \) is half of the angle of refraction \( R \), we can express this relationship as: \[ I = \frac{R}{2} \] or equivalently, \[ R = 2I \] ### Step 2: Apply Snell's Law Snell's Law states that: \[ \frac{\sin I}{\sin R} = \frac{\mu_r}{\mu_d} \] Given that \( \mu = \frac{\mu_d}{\mu_r} \), we can rewrite \( \frac{\mu_r}{\mu_d} \) as \( \frac{1}{\mu} \). Thus, we have: \[ \frac{\sin I}{\sin R} = \frac{1}{\mu} \] ### Step 3: Substitute for \( R \) Substituting \( R = 2I \) into Snell's Law gives us: \[ \frac{\sin I}{\sin(2I)} = \frac{1}{\mu} \] ### Step 4: Use the double angle formula Using the double angle formula for sine, we know that: \[ \sin(2I) = 2 \sin I \cos I \] Substituting this into our equation from Step 3, we get: \[ \frac{\sin I}{2 \sin I \cos I} = \frac{1}{\mu} \] ### Step 5: Simplify the equation Cancelling \( \sin I \) from both sides (assuming \( \sin I \neq 0 \)): \[ \frac{1}{2 \cos I} = \frac{1}{\mu} \] Cross-multiplying gives: \[ \mu = 2 \cos I \] ### Step 6: Solve for \( I \) Rearranging the equation gives: \[ \cos I = \frac{\mu}{2} \] To find \( I \), we take the inverse cosine: \[ I = \cos^{-1}\left(\frac{\mu}{2}\right) \] ### Final Result Thus, the magnitude of the incident angle \( I \) is: \[ I = \cos^{-1}\left(\frac{\mu}{2}\right) \]
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