Imagine a ray of light navigating through a multi-layered optical slab. It starts in a medium with refractive index n1, hits a second medium n2, and eventually faces the ultimate boundary: air. The problem gives us one seemingly simple, yet profoundly powerful inequality: sinθ>n11. This single mathematical statement is the master key that locks the light ray inside the slab forever. Let's unravel why.
The Master Equation
Snell's Law Across Parallel Boundaries
When dealing with multiple parallel optical interfaces, Snell's Law is our best friend. It tells us that the product of the refractive index and the sine of the angle of the ray with the normal is a conserved quantity across all parallel layers.
If we assume the ray manages to refract through medium
n2 and reaches the air interface (where
nair=1) at an angle
θ3, we can write the continuous Snell's Law equation:
n1sinθ=n2sinθ2=1⋅sinθ3
Notice something incredible here? The middle medium
n2 completely drops out of the relationship between the initial medium and the final medium! We can directly equate the first and last states:
sinθ3=n1sinθ
The Mathematical Impossibility
Now, let's bring in our master key
We are given that
sinθ>n11. Let's substitute this inequality into our derived equation:
sinθ3=n1sinθ>n1(n11)=1
We arrive at the conclusion that sinθ3>1. But wait, the sine of any real angle can never exceed 1! What does this mathematical impossibility mean physically? It means that our initial assumption—that the ray reaches and refracts into the air—is fundamentally flawed. The ray must undergo Total Internal Reflection (TIR) either before it reaches the air, or exactly at the air interface. It is physically trapped!
Analyzing the Scenarios
Armed with this absolute truth, let's evaluate the given options.
Option (A): What if n1=n2?
If the two media have the same refractive index, the ray travels in a straight line until it hits the air interface. But as we just proved, it will face TIR at the air boundary because sinθ3>1. The ray does not enter the air. Option A is incorrect.
Option (B): What if n2<n1?
Here, the ray is traveling from a denser to a rarer medium at the first interface. It might suffer TIR right there if the angle is large enough. If it doesn't, it refracts into n2 and travels to the air interface. But we already know it cannot escape into the air! It will suffer TIR at the top boundary, reflect back into n2, and eventually refract back into n1. In either case, it returns to n1. Option B is correct.
Option (C): What if n2>n1?
In this scenario, the ray travels from a rarer to a denser medium, so it bends towards the normal. TIR is impossible at the first interface. The ray safely reaches the air interface. However, the inescapable truth remains: sinθ3>1. The ray undergoes TIR at the air boundary, reflects back into n2, and then refracts back into n1. Option C is correct.
Option (D): What if n2=1?
If n2 is air, the very first interface is the n1-air boundary. The critical angle for this interface is given by sinθc=n11. Since we are explicitly given that sinθ>n11, the incident angle is strictly greater than the critical angle. The ray undergoes TIR immediately and reflects back into n1. Option D is correct.
The Elegance of the Problem
This JEE Advanced problem is a beautiful demonstration of how a single boundary condition can dictate the entire physical reality of a system
By recognizing that Snell's Law is conserved across parallel layers, we bypassed complex intermediate calculations and went straight to the heart of the physics. The light ray, bound by the laws of optics, is forever destined to return to its origin.