WHAT we start with — Snell's law. This is the only physics input we need:
n1sinθ1=n2sinθ2
WHY this law? Light slows down in a denser medium (v=c/n). At a boundary the wavefronts must stay continuous, so the ray must bend. Snell's law is exactly the bookkeeping of that continuity (it follows from Fermat's least-time principle / phase matching).
HOW we find the critical angle — step by step.
Step 1. Send light from medium 1 (denser, n1) into medium 2 (rarer, n2), so n1>n2.
Why this step? TIR is impossible going rarer→denser, so we must set up dense→rare.
Step 2. Increase θ1. Since n1>n2, Snell gives sinθ2=n2n1sinθ1>sinθ1, so θ2>θ1: the ray bends away from the normal.
Why this step? It shows θ2 races ahead of θ1 and will hit 90° first.
Step 3. Define the critical angle as the θ1 for which the refracted ray just grazes the surface: θ2=90°.
Why this step?90° is the last possible refraction angle. Beyond it, no real refracted ray exists.
Step 4. Substitute θ1=θc and θ2=90° into Snell:
n1sinθc=n2sin90°=n2⋅1
Step 5. Solve:
Step 6 (the punchline). For θ1>θc, Snell would demand sinθ2=n2n1sinθ1>1 — impossible. So no refracted ray exists, and 100% of the energy reflects: total internal reflection.
Light must go denser→rarer (n1>n2) AND the incidence angle must exceed the critical angle (θ1>θc).
Derive the critical angle condition from Snell's law.
Set θ2=90° in n1sinθ1=n2sinθ2 → n1sinθc=n2 → sinθc=n2/n1.
Formula for the critical angle?
sinθc=n2/n1 (rarer index over denser index).
For glass (n=1.5) in air, what is θc?
sin−1(1/1.5)≈41.8°.
Why does refraction become impossible beyond θc?
Snell would require sinθ2>1, which has no real solution, so no refracted ray exists and all light reflects.
Does a higher refractive index give a larger or smaller critical angle?
Smaller — that's why diamond (θc≈24°) traps light and sparkles.
How do you get n from a measured critical angle (against air)?
n=1/sinθc.
Recall Feynman: explain to a 12-year-old
Imagine you're underwater looking up. Light can escape into the air, but the more slanted you look, the more the escaping light bends. At one special slant (the critical angle), the light can't escape anymore — it skims flat along the water's surface. Tilt just a bit more and the water acts like a perfect mirror: the light bounces straight back down. That mirror-trick is total internal reflection, and the special slant where it kicks in is the critical angle.
Dekho, jab light ek dense medium (jaise glass, jiska refractive index zyada hai) se rare medium (jaise air) me jaati hai, toh woh normal se door mudti hai. Jaise-jaise tum incidence angle θ1 badhate ho, refracted ray aur zyada flat hoti jaati hai. Ek special angle aata hai jahan refracted ray bilkul surface ke saath-saath chali jaati hai, yaani θ2=90°. Yahi wala incidence angle critical angleθc kehlata hai.
Ab maths bilkul simple hai — sirf Snell's law lagao: n1sinθ1=n2sinθ2. Critical angle pe θ2=90° daalo, toh sin90°=1, aur formula ban jaata hai sinθc=n2/n1. Yaad rakhna: rarer upar, denser neeche (rarer index divided by denser index). Glass-air ke liye yeh 1/1.5=0.667 aata hai, matlab θc≈41.8°.
Asli magic tab hota hai jab θ1>θc. Tab Snell's law bolta hai ki sinθ2 ko 1 se bada hona padega — jo impossible hai! Toh light bahar nikal hi nahi sakti, poori ki poori wapas reflect ho jaati hai. Isi ko Total Internal Reflection kehte hain. Yahi reason hai ki optical fibre me light kilometers tak bina leak hue travel karti hai, aur diamond itna sparkle karta hai (uska θc sirf 24° hai, toh light andar phasi rehti hai).
Ek common galti: students sinθc=n1/n2 likh dete hain — galat! Hamesha derive karke check karo: agar value 1 se zyada aaye toh formula ulta hai. Aur dhyaan rakho TIR sirf dense-to-rare direction me hota hai, ulta kabhi nahi.