The Inescapable Light
A Tale of Total Internal Reflection
Imagine a beam of light trying to escape from a denser medium into a rarer one. If the angle is just right, the boundary acts like a perfect mirror, trapping the light inside. This phenomenon is known as Total Internal Reflection (TIR). In this fascinating problem, we explore what happens when we introduce a new transparent slab into the mix. Will the light finally escape, or is it doomed to return?
The Master Condition
Let's start by analyzing the initial setup. We are given that a light ray is incident from Medium II (with refractive index n2) towards Medium I (with refractive index n1). The angle of incidence, θ, is infinitesimally greater than the critical angle for these two media.
Mathematically, the critical angle θc12 is defined by sinθc12=n2n1. Since our incident angle θ is greater than this critical angle, we can write our master condition:
This simple inequality is the cornerstone of our entire proof. Keep it close!
Case A
The Impenetrable Wall (n3<n1)
Now, let's introduce the transparent slab (Medium III) with refractive index n3. In our first case, we assume n3 is even smaller than n1. This means n3<n1<n2.
What happens at the boundary between Medium II and the new slab? We need to check the new critical angle, θc23, which is given by sinθc23=n2n3.
Because n3<n1, it naturally follows that n2n3<n2n1. This implies that the new critical angle is smaller than the original one:
Since our incident angle θ is already greater than the original critical angle, it is definitely greater than this new, smaller critical angle. Therefore, the light ray doesn't even penetrate the slab! It undergoes Total Internal Reflection right at the first boundary and is immediately reflected back into Medium II.
Case B
The Deceptive Entry (n3>n1)
What if the slab has a higher refractive index, such that n3>n1? In this scenario, the light might actually enter the slab. Let's assume it does, and it refracts at an angle i.
We can apply Snell's law at the boundary between Medium II and Medium III:
Once the light is inside the slab, it travels towards the upper boundary separating Medium III and Medium I. Will it escape here? For TIR to occur at this upper boundary, the angle of incidence (which is i) must be greater than the critical angle for these two media, θc31.
The condition for TIR at the upper boundary is:
Which can be rewritten as:
The Mathematical Climax
Now, let's bring all our pieces together. From Snell's law, we know that n3sini is exactly equal to n2sinθ.
And remember our master condition from the very beginning? We established that n2sinθ>n1.
By simply substituting n3sini for n2sinθ in our master condition, we get:
This is exactly the condition required for Total Internal Reflection at the upper boundary!
Conclusion
Because the condition is perfectly satisfied, the light ray cannot escape into Medium I. It undergoes TIR at the upper boundary, bounces back down through the slab, and finally refracts back into Medium II.
We have elegantly proven that whether the slab's refractive index is lower or higher than Medium I, the light is ultimately trapped. For any value of n3, the light will always find its way back to Medium II. The physics of light, governed by the beautiful simplicity of Snell's law, ensures its inevitable return.