Animated Solution for Physics - Optics: A monochromatic beam of light is incident at 60∘ on one face of an equilateral prism of refractive index n and emerges from the opposite face making an angle θ(n) with the normal (see figure). For n=3 the value of θ is 60∘ and dndθ=m. The value of m is
Enter Numerical Value:
Visualized Solution
Visualizing the Prism
Let's visualize the path of the monochromatic light beam through the equilateral prism.
At the first surface, angle of incidence i1=60∘, angle of refraction is r1.
At the second surface, angle of incidence is r2, angle of emergence is i2=θ.
For an equilateral prism, the prism angle A=60∘.
We know that r1+r2=A=60∘.
Applying Snell's Law
Applying Snell's law at the first surface:
sin60∘=nsinr1
Applying Snell's law at the second surface:
nsinr2=sinθ
Since r2=60∘−r1, we can write:
nsin(60∘−r1)=sinθ
Differentiating the First Equation
Differentiating sin60∘=nsinr1 with respect to n:
0=sinr1+ncosr1dndr1
Rearranging for dndr1:
dndr1=−ncosr1sinr1=−ntanr1
Differentiating the Second Equation
Differentiating sinθ=nsin(60∘−r1) with respect to n:
cosθdndθ=sin(60∘−r1)+ncos(60∘−r1)(−dndr1)
Substituting the Derivative
Substitute dndr1=−ntanr1 into the equation:
cosθdndθ=sin(60∘−r1)−ncos(60∘−r1)(−ntanr1)
cosθdndθ=sin(60∘−r1)+cos(60∘−r1)tanr1
Evaluating Angles for n=3
Given n=3, let's find the specific angles.
sin60∘=3sinr1⇒23=3sinr1⇒sinr1=21
So, r1=30∘.
Then r2=60∘−30∘=30∘.
sinθ=3sin30∘=23⇒θ=60∘.
Final Calculation
Substitute r1=30∘ and θ=60∘ into the differentiated equation:
cos60∘dndθ=sin(60∘−30∘)+cos(60∘−30∘)tan30∘
21dndθ=sin30∘+cos30∘tan30∘
21dndθ=21+23×31=21+21=1
dndθ=2⇒m=2
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The Sigma Insight: Refraction and Dispersion through Prism
Solution Diagram
The problem asks us to find the rate of change of the angle of emergence θ with respect to the refractive index n of an equilateral prism, evaluated at n=3. This is a beautiful application of Snell's law combined with implicit differentiation.
Analyzing the Setup
Let's visualize the path of the monochromatic light beam through the equilateral prism. The beam hits the first face at an angle of incidence i1=60∘, refracts inside at an angle r1, and emerges from the second face at an angle of emergence i2=θ.
For an equilateral prism, the prism angle A is 60∘. We know from the geometry of prisms that the sum of the internal angles of refraction equals the prism angle:
r1+r2=A=60∘
The Master Equation
To find how θ changes with the refractive index n, we need to set up the equations for refraction. Applying Snell's law at the first surface:
sin60∘=nsinr1
Applying Snell's law at the second surface:
nsinr2=sinθ
Since r2=60∘−r1, we can rewrite the second equation as:
nsin(60∘−r1)=sinθ
Now, we differentiate the first equation with respect to n. The derivative of sin60∘ is zero because the angle of incidence is constant. Using the product rule on the right side, we get:
0=sinr1+ncosr1dndr1
Rearranging this gives us the rate of change of the first refraction angle:
dndr1=−ncosr1sinr1=−ntanr1
Next, we differentiate the second equation with respect to n:
cosθdndθ=sin(60∘−r1)+ncos(60∘−r1)(−dndr1)
We can substitute the expression for dndr1 into this equation. The n cancels out, and the minus signs become plus:
cosθdndθ=sin(60∘−r1)−ncos(60∘−r1)(−ntanr1)
cosθdndθ=sin(60∘−r1)+cos(60∘−r1)tanr1
Final Calculation
We are given that n=3. Let's find the specific angles for this case. From the first equation:
sin60∘=3sinr1
23=3sinr1⇒sinr1=21
So, r1=30∘. Consequently, r2=60∘−30∘=30∘.
Now, let's find the emergent angle θ:
sinθ=3sin30∘=23⇒θ=60∘
Finally, let's substitute these angles into our differentiated equation: