Traps tackle karne se pehle, boundary khud dekho — kyunki neeche ke almost har trap mein actually is ek picture ki galat reading hai.
Figure ko left se right padhо. Sabse left panel mein incidence angle θ1 chhota hai: light rarer medium mein cross karti hai aur normal se door bend hoti hai, isliye θ2>θ1. Jaise-jaise tum θ1 upar slide karte ho (middle panel), refracted ray surface ki taraf aur aur tip karti jaati hai. Right panel mein θ1 exactly us value par pahunch gaya hai jahan refracted ray boundary ke saath flat lie karti hai — yahi θ2=90° hai, aur yahi incidence angle θc hai.
Formula kahan se aata hai — ek wavefront argument, koi memorised rule nahi. Snell's law n1sinθ1=n2sinθ2 sirf yeh statement hai ki wavefronts boundary ke along continuous rehti hain (dekho Snell's Law). Grazing condition θ2=90° plug karo, jiske liye sin90°=1:
n1sinθc=n2⋅1⟹sinθc=n1n2
Toh formula bas itna hi hai ki "refracted ray ke paas bend karne ki jagah khatam ho gayi." Kyunki hamein n1>n2 chahiye (dense→rare), right side hamesha 1 se kam hoti hai, aur yahi reason hai ki ek valid angle exist karta hai. Yeh panel dimaag mein rakho — "flat refracted ray" picture neeche har item ka anchor hai.
TIR tab ho sakta hai jab light rarer medium se denser medium mein travel kare.
False — n1<n2 ke saath sinθ2=n2n1sinθ1<1 har θ1 ke liye hota hai, isliye ek real refracted ray hamesha exist karti hai aur refraction kabhi cease nahi hoti.
Exactly θ1=θc par, saari light already totally internally reflect ho chuki hoti hai.
False — exactly θc par refracted ray abhi bhi exist karti hai lekin surface ke saath θ2=90° par graze karti hai; TIR (100% reflection) sirf tab shuru hota hai jab θ1, θc se strictly greater ho.
Denser medium ka bada refractive index ek bada critical angle deta hai.
False — sinθc=n2/n1, isliye n1 badhane se fraction chhota hota hai aur isliye θc bhi; yahi reason hai ki diamond (n=2.42, θc≈24°) glass se kahin zyada aasaani se light trap karta hai.
Critical angle sirf denser medium ke index par depend karta hai.
False — yeh ration2/n1 par depend karta hai; same glass ka air ke against ek θc hota hai aur water ke against bilkul alag.
Critical angle se neeche, boundary par koi bhi light reflect nahi hoti.
False — kuch light hamesha reflect hoti hai (partial reflection har boundary par hota hai); θc se neeche zyaadatar energy transmit hoti hai, aur reflected fraction sirf badhta hai jaise-jaise θ1, θc ke paas pahunchta hai.
Agar do media ke refractive indices equal hain, toh koi critical angle nahi hoga.
True — n1=n2 ke saath, sinθc=1 isliye θc=90°; light kabhi bend nahi hoti aur kabhi trap nahi ho sakti, isliye TIR effectively occur nahi kar sakta.
TIR sirf kuch light reflect karta hai; kuch hamesha leak hoti rehti hai.
False — θc se aage 100% energy reflect hoti hai (ideally); koi ordinary refracted ray time-averaged energy carry nahi karta, aur yahi "total" ka matlab hai.
Critical angle se aage electromagnetic field boundary ke dusri taraf exactly zero hota hai.
False — surface ke baad ek non-propagating evanescent field exist karta hai, jo wavelength ke fraction par exponentially decay karta hai; yeh boundary ke across koi net energy carry nahi karta, isliye reflection abhi bhi total hai (edge-case section dekho).
Total internal reflection aur metal mirror se reflection ek hi phenomenon hai.
False — ek metal mirror har bounce par kuch percent absorb karta hai, jabki TIR essentially lossless hai; yahi reason hai ki fibre optics aur prisms TIR use karte hain na ki metallic coatings.
"sinθc=n1/n2, kyunki incident medium pehle likha jaata hai."
Ratio flip hai. n1sinθc=n2sin90° mein θ2=90° set karne par sinθc=n2/n1 milta hai — rarer over denser, jo correctly 1 se kam hai.
"Air se glass mein jaane wali light TIR undergo kar sakti hai agar angle kaafi steep ho."
Direction ulta hai. Air→glass rarer→denser hai, isliye us side koi critical angle exist nahi karta; TIR ke liye light ko denser medium ke andar hona chahiye boundary hit karte waqt.
"Critical angle woh hai jahan reflected ray exactly 90° incident ray se hoti hai."
Yeh Brewster's condition describe karta hai — θB par reflected aur refracted rays perpendicular hoti hain (θB+θ2=90°), jo reflection ko polarize karta hai. Critical angle alag hai: isse refracted ray ke θ2=90° par grazing se define kiya jaata hai, yeh refraction cease hone ka statement hai, polarization ka nahi (dekho Brewster's Angle).
"Kyunki sinθc=n2/n1, ek fibre core jiska n=1.0 hai air ke against light perfectly trap karega."
n1=1.0=n2 ke saath fraction 1 hai aur θc=90°; kuch bhi trap nahi hota. Ek working fibre ko ek core chahiye jo uski cladding se denser ho (dekho Optical Fibres).
"θc=sin−1(1.4/1.2) light ke liye jo n1=1.2 se n2=1.4 mein jaati hai."
Argument 1.4/1.2>1 ka koi valid arcsine nahi hai — yeh sign hai ki yeh direction (rarer→denser) koi critical angle allow hi nahi karta, isliye setup invalid hai.
"θc ke aage bhi refraction hoti rehti hai, bas 90° se zyada bend hoti hai."
Transmitted ray ke liye "90° se zyada" bend jaisi koi cheez nahi hoti — woh use incident side par wapas rakh deta. Snell demand karta hai sinθ2>1, jo impossible hai, isliye refraction genuinely ruk jaati hai (dekho Refraction of Light).
Kyun refracted ray 90° par pahunch jaati hai pehle incident ray se, jaise-jaise θ1 badhta hai?
Kyunki dense→rare mein sinθ2=n2n1sinθ1 hota hai jisme n1/n2>1, isliye θ2>θ1 hamesha; θ2 aage bhaagta hai aur 90° ki ceiling ko hit karta hai jabki θ1 abhi bhi chhota hota hai.
Kyun θ2=90° ko θc ke liye defining condition choose kiya jaata hai?
Kyunki 90°sabse bada possible refraction angle hai — ray surface ke saath flat lie karti hai (figure ka rightmost panel). Kisi bhi bade θ2 ki demand geometrically impossible hai, isliye yahi exact tipping point hai jahan refraction exist nahi kar sakti.
Kyun diamonds same cut ke glass gems se zyada sparkle karte hain?
Diamond ka high index (2.42) ek chhota θc≈24° deta hai, isliye zyaadatar internal rays ise exceed karti hain aur escape se pehle andar kai baar bounce karti hain, light ko concentrate aur delay karti hain.
Kyun sinθc ek valid critical angle ke liye hamesha 1 se kam aana chahiye?
Kyunki sinθc=n2/n1 aur TIR ke liye n1>n2 chahiye (denser to rarer); ≥1 ki value signal karti hai ki ya toh ratio flip ho gaya ya galat direction choose kiya (dekho Refractive Index).
Kyun binoculars aur periscopes ke andar silvered mirrors ki jagah TIR prefer kiya jaata hai?
TIR essentially 100% light reflect karta hai bina kisi metallic absorption ke, isliye images bright rehti hain; ek 45° prism angle comfortably glass ke θc≈42° se exceed karta hai (dekho Prisms and Total Internal Reflection).
Kyun garmi ke din ek road door se geeli, reflective surface jaisi dikhti hai?
Garmi ki road ke paas ki hawa ek continuous index gradient banati hai (surface par sabse rarer); har thin layer sky-light ko thoda aur refract karti hai jab tak ek ray wapas upar bend nahi ho jaati. Yeh ek single sharp interface nahi hai, isliye strictly yeh gradient refraction hai, textbook TIR nahi — though trapping effect similar lagta hai (dekho Mirage and Atmospheric Refraction).
θc kya hoga jab do media identical hain (n1=n2)?
sinθc=1, isliye θc=90°; light seedhi nikal jaati hai bina kisi bending ke aur kabhi trap nahi ho sakti — TIR impossible hai.
Jaise n2→n1 neeche se, critical angle ka kya hoga?
n2/n1→1, isliye θc→90°; "trapping window" (θc,90°) kuch nahi tak sir jaati hai, matlab jaise indices ek doosre ke paas aate hain TIR achieve karna mushkil hota jaata hai.
Jaise n1, n2 ki tulna mein bahut bada hota jaata hai, θc kya approach karta hai?
n2/n1→0, isliye θc→0°; incidence ka almost koi bhi angle light ko trap kar leta hai, jo lossless light-piping ke liye ideal limit hai.
Exactly θ1=θc par kya hota hai — boundary mirror hai ya window?
Na poora ek, na poora doosra — refracted ray exist karti hai lekin surface ke saath skim karti hai (θ2=90°), ek knife-edge case; true mirror behaviour sirf is angle se thoda aage switch on hota hai.
Agar light dense→rare setup mein θ1=0° (seedha) par boundary hit kare, toh kya TIR hoga?
Nahi — normally-incident ray seedhi nikal jaati hai θ2=0° ke saath; kyunki 0°<θc, refraction freely hoti hai aur koi trapping nahi hoti.
Kya TIR ho sakta hai agar incident medium vacuum ho?
Nahi — vacuum ka sabse kam possible index hai (n=1), isliye koi rarer medium nahi hai jisme light jaaye; TIR ke liye destination se kisi denser cheez mein shuru karna zaroori hai.
θc ke aage, kya koi bhi energy rarer medium mein cross kar sakti hai?
Flat boundary akele se nahi — wahan field evanescent hai, penetration depth ∼λ/(2π) ke saath exponentially decay karti hai aur across koi net energy carry nahi karti. Lekin agar ek doosra dense medium us decay distance ke andar laaya jaaye, toh light gap ke across "tunnel" kar sakti hai (frustrated TIR) — quantum tunnelling ka wave equivalent.
θ1>θc par evanescent field surface ke aage kitni deep tak jaata hai?
Sirf wavelength ke fraction tak — uski amplitude roughly λ/(2π) boundary ke andar 1/e tak fall ho jaati hai, yahi reason hai ki "total" reflection genuinely total hai jab tak surface ke bilkul saath koi aur medium nahi rakh diya jaata.