The Setup
A Ray's Journey
Imagine a ray of light entering a rectangular glass slab. It refracts at the first vertical face, travels through the dense glass, and strikes the top horizontal face. The problem presents a strict condition: we want the ray to emerge only from the opposite vertical face CD.
What does this mean physically? It implies that the ray must be completely trapped inside the slab when it hits the top face AD. It must not escape into the surrounding water. This phenomenon, where light is perfectly reflected back into the denser medium, is known as Total Internal Reflection (TIR).
The Boundary Condition
Total Internal Reflection
For TIR to occur at the top face AD, the angle of incidence there—let's call it r2—must be greater than or equal to the critical angle θC of the glass-water interface.
We are tasked with finding the maximum possible entry angle, αmax. By Snell's Law, a larger entry angle α will result in a larger angle of refraction r1. As we will see shortly, a larger r1 forces r2 to become smaller. Therefore, to push α to its absolute maximum limit, we must push r2 to its absolute minimum limit, which is exactly the critical angle.
The Geometric Bridge
Now, let's look at the geometry of the refracted ray inside the slab. The normal at the first face AB is horizontal, while the normal at the top face AD is vertical. These two normals intersect at a perfect 90∘ angle, forming a right-angled triangle with the ray's path.
Because the sum of angles in a triangle is 180∘, the angle of refraction r1 and the angle of incidence r2 must be complementary. They add up to exactly 90∘.
Since r1 and r2 are complementary, when r2 is at its minimum, r1 will be at its maximum. Let's substitute the critical angle for r2 to find the maximum value of r1.
(r1)max=90∘−(r2)min
(r1)max=90∘−θC
Applying Snell's Law at the Entry Point
Let's bring our focus back to the first face, AB. The ray is entering from water (refractive index n2) into the glass (refractive index n1). Applying Snell's Law at this interface gives us:
n2sinαmax=n1sin(r1)max
Now, we substitute our geometric expression for (r1)max into Snell's Law.
n2sinαmax=n1sin(90∘−θC)
From basic trigonometry, we know that sin(90∘−θ)=cosθ. This simplifies our equation beautifully.
The Final Mathematical Synthesis
We are almost at the finish line! We need to express cosθC in terms of the given refractive indices. By definition, the sine of the critical angle is the ratio of the outer refractive index to the inner one.
This means the critical angle itself is:
Let's plug this definition of θC right into our cosine term.
sinαmax=n2n1cos(sin−1n1n2)
Finally, to isolate αmax, we take the sine-inverse of the entire expression on the right side.
αmax=sin−1[n2n1cos(sin−1n1n2)]
And there we have it! This is the maximum angle of incidence that guarantees the ray will remain trapped inside the slab and only exit from the opposite face. This elegant interplay of Snell's law and geometry is the exact foundational principle behind optical fibers, which trap light inside them to transmit data over vast distances across the globe!