2.5.15 · D3 · Physics › Optics › Diffraction grating — condition for maxima
Intuition Yeh page kis liye hai
Parent note Diffraction grating — condition for maxima ne tumhe wo ek rule diya jo sab kuch chalata hai:
d sin θ m = mλ .
Yahan θ m ka matlab bas itna hai — "us maximum ka angle θ jiska order m hai" — hum chhota sa subscript m isliye lagate hain taaki yaad rahe ki hum kis bright spot ki taraf point kar rahe hain (m = 1 wala, m = 2 wala, wagera). Jab koi ambiguity nahi hoti toh subscript hata dete hain aur seedha θ likhte hain.
Yahan hum naya physics nahi seekhte — hum har tarah ke questions dhundte hain jo us rule se nikl sakte hain, aur ek-ek ka solve karte hain. Agar tum yeh sab kar sako, toh koi bhi grating problem tumhe surprise nahi kar sakti.
Shuru karne se pehle, aao har symbol ko dobara samjhein taaki koi bhi reader seedha aa ke follow kar sake:
d = do neighbouring slits ke beech ki centre-to-centre distance , metres mein measure ki gayi. Ek fence mein do tiny gaps socho; d us gap-to-gap ka step hai.
θ = angle jo outgoing ray straight-ahead direction se banati hai ("normal", yaani grating ke perpendicular line). Seedha aage θ = 0 hai; side mein hard turn θ = 9 0 ∘ hai. Subscript ke saath, θ m m -ve maximum ka angle hai.
λ (lambda) = wavelength , light ki ek poori crest-to-crest ripple ki length. Dekho Wavelength and the visible spectrum .
m = order , ek poora counting number 0 , ± 1 , ± 2 , … . Yeh count karta hai ki kitne poore wavelengths ka extra path neighbouring rays ko alag karta hai.
sin θ = ek right triangle ka "opposite over hypotenuse". Hum yeh use karte hain (na ki tan ya cos ) kyunki ek ray jo extra path travel karti hai woh ek right triangle ki woh side hai jo angle θ ke opposite hoti hai, d hypotenuse ke saath — exactly wahi jo parent note ne draw kiya tha.
Intuition Signs, negative orders aur arcsine ke do answers
Har worked example neeche positive θ ke liye solve karta hai, lekin physics left–right symmetric hai, isliye signs ke baare mein honest rehna zaroori hai:
Negative orders. Kyunki m ka range 0 , ± 1 , ± 2 , … hai, har positive maximum ka ek mirror twin hota hai. Agar m = + 1 angle + θ par hai, toh m = − 1 angle − θ par hai — wahi angle doosri taraf centre se. Isliye counting problems (Cell D) mein hamesha ek odd total 2 m m a x + 1 milta hai.
Arcsine ke do answers. Jab tum θ = sin − 1 ( x ) likhte ho, yaad rakho ki sin usi value par θ aur 18 0 ∘ − θ dono par equal hota hai. Ek grating ke liye hum sirf − 9 0 ∘ ≤ θ ≤ + 9 0 ∘ wali branch rakhte hain, kyunki grating se nikalna ray ko forward half-space mein point karna chahiye (woh grating ke through peeche nahi ja sakti). Isliye hum hamesha "principal" arcsine lete hain, kabhi obtuse partner nahi.
The ceiling. sin θ kabhi 1 se zyada ya − 1 se kam nahi ho sakta, isliye − 9 0 ∘ ≤ θ ≤ + 9 0 ∘ poora physically allowed range hai. Koi bhi m jo ∣ mλ / d ∣ > 1 force kare uska koi real angle nahi hota — woh order simply exist hi nahi karta.
Yeh dhyan mein rakho: jab bhi hum likhein "θ 1 = 19. 3 ∘ ", toh m = − 1 ke liye silently ek matching − 19. 3 ∘ bhi hota hai.
Har grating question in cells mein se ek (ya blend) hoti hai. Har worked example neeche us cell ke saath tagged hai jise woh solve karta hai.
Cell
Kya ise alag banata hai
Example
A. Forward — angle nikalo
d , λ , m diya; θ solve karo
Ex 1
B. Backward — d nikalo
θ , λ , m diya; spacing / lines-per-mm solve karo
Ex 2
C. Backward — λ nikalo
θ , d , m diya; wavelength solve karo
Ex 3
D. Orders count karo
Kitne maxima fit hote hain; sin θ ≤ 1 aur ± m symmetry use karo
Ex 4
E. Degenerate: m = 0
Zero order — sab colours overlap karte hain, koi dispersion nahi
Ex 5
F. Limiting: order exactly 9 0 ∘ par
sin θ = 1 boundary; "just barely fits / just fails" wala case
Ex 6
G. Do wavelengths / dispersion
Ek hi order mein do colours ka angular separation
Ex 7
H. Real-world word problem
Starlight spectrometer, numbers extract karni padegi
Ex 8
I. Exam twist — overlapping orders
Ek colour ka order m same angle par land karta hai jahan doosre colour ka order m ′ hai
Ex 9
Cells covered: A B C D E F G H I — sab ke sab.
Worked example Example 1 (Cell A)
Green light, λ = 550 nm , 600 lines/mm ki grating par padti hai. First-order (m = 1 ) maximum kahan hai?
Forecast: Jab d sirf kuch wavelengths jitna wide hai, kya tum ek tiny angle (kuch degrees) expect karte ho ya ek bada wala (tens of degrees)? Pehle guess karo, phir padhte jao.
Step 1 — d metres mein nikalo.
d = 600 mm − 1 1 = 600 1 mm = 1.667 × 1 0 − 6 m .
Yeh step kyun? Equation ko physical spacing chahiye, na ki "lines per mm". Hum invert karte hain, aur mm→m convert karte hain taaki d aur λ SI units share karein (parent note mein "lines vs spacing" wali galti dekho).
Step 2 — grating rule ko sin θ ke liye rearrange karo.
sin θ 1 = d mλ = 1.667 × 1 0 − 6 1 ⋅ 550 × 1 0 − 9 = 0.330.
Yeh step kyun? θ unknown hai; sin θ isolate karna hi ek zaruri algebra hai. Neeche step figure dekho — mλ / d literally "opposite ÷ hypotenuse" ratio hai.
Step 3 — sine undo karo.
θ 1 = sin − 1 ( 0.330 ) = 19. 3 ∘ .
Yeh step kyun? sin − 1 (arcsine) jawab deta hai "kis angle ka sine yeh hai?" — yeh sine ko undo karke angle reveal karta hai. Hum principal value [ − 9 0 ∘ , + 9 0 ∘ ] mein rakhte hain; twin maximum m = − 1 angle − 19. 3 ∘ par hoga.
Verify: Plug back karo: d sin θ = 1.667 × 1 0 − 6 × sin ( 19. 3 ∘ ) = 1.667 × 1 0 − 6 × 0.330 = 5.5 × 1 0 − 7 m = 550 nm = 1 ⋅ λ . ✓ Angle bada hai (tens of degrees) — small-angle shortcut fail ho jaata.
Worked example Example 2 (Cell B)
Ek red laser, λ = 633 nm , apna third-order maximum θ = 35. 0 ∘ par produce karta hai. Grating spacing d aur lines per mm nikalo.
Forecast: Modest angle par higher order ka matlab hai ki slits relatively... wide hain ya narrow? Guess karo.
Step 1 — rule ko d ke liye solve karo.
d = s i n θ mλ = s i n 3 5 ∘ 3 ⋅ 633 × 1 0 − 9 .
Yeh step kyun? Ab d unknown hai, isliye dono sides ko sin θ se divide karte hain.
Step 2 — evaluate karo.
sin 3 5 ∘ = 0.5736 , d = 0.5736 1.899 × 1 0 − 6 = 3.31 × 1 0 − 6 m .
Yeh step kyun? Symbolic answer ko number mein badalna hai: calculator se sin 3 5 ∘ compute karo, numerator mλ = 3 × 633 nm banao, phir divide karo, taaki physical spacing padh sakein.
Step 3 — lines per mm mein convert karo.
lines/mm = d 1 = 3.31 × 1 0 − 3 mm 1 ≈ 302 lines/mm .
Yeh step kyun? Lines-per-mm spacing ka reciprocal hota hai, mm mein expressed.
Verify: d sin θ = 3.31 × 1 0 − 6 × 0.5736 = 1.90 × 1 0 − 6 m , aur mλ = 3 × 633 × 1 0 − 9 = 1.90 × 1 0 − 6 m . ✓ Slits fairly wide hain (≈300/mm), isliye order 3 modest 35° par baitha hai.
Worked example Example 3 (Cell C)
Ek unknown spectral line second order (m = 2 ) par appear hoti hai, θ = 28. 0 ∘ par, 400 lines/mm ki grating par. Wavelength kya hai, aur kya yeh visible hai?
Forecast: Visible light ~400–700 nm tak hoti hai. Kya tumhara answer us band ke andar land karega?
Step 1 — d nikalo.
d = 400 mm − 1 1 = 2.5 × 1 0 − 6 m .
Yeh step kyun? Equation physical spacing d ke terms mein likhi hai, lekin data "lines per mm" ke roop mein aaya hai; hum invert karte hain taaki us ruling density ko metre-scale gap mein convert karein jisse d aur λ SI units share karein.
Step 2 — rule ko λ ke liye solve karo.
λ = m d s i n θ = 2 2.5 × 1 0 − 6 × s i n 2 8 ∘ .
Yeh step kyun? λ ab unknown hai; path difference d sin θ ko order m se divide karo.
Step 3 — evaluate karo.
sin 2 8 ∘ = 0.4695 , λ = 2 2.5 × 1 0 − 6 × 0.4695 = 5.87 × 1 0 − 7 m = 587 nm .
Verify: 587 nm visible spectrum ke yellow mein hai — yeh famous sodium line hai. Plug back: d sin θ = 2.5 × 1 0 − 6 × 0.4695 = 1.174 × 1 0 − 6 ; mλ = 2 × 5.87 × 1 0 − 7 = 1.174 × 1 0 − 6 . ✓
Worked example Example 4 (Cell D)
Blue light λ = 450 nm 800 lines/mm ki grating par. Total kitne bright maxima appear hote hain?
Forecast: Compute karne se pehle total guess karo. (Yaad rakho maxima dono sides par appear hote hain!)
Step 1 — d nikalo.
d = 800 mm − 1 1 = 1.25 × 1 0 − 6 m .
Yeh step kyun? Counting formula physical spacing d use karta hai; data lines/mm mein ruling density hai, isliye hum invert karte hain (aur metres mein padhte hain) taaki woh gap nikale jo actually d / λ mein enter karta hai.
Step 2 — sabse bada possible order nikalo.
λ d = 450 × 1 0 − 9 1.25 × 1 0 − 6 = 2.78.
Yeh step kyun? sin θ ko uski physical ceiling 1 par set karne se m m a x = ⌊ d / λ ⌋ milta hai; koi bhi bada m demand karta hai sin θ > 1 , jo koi real angle supply nahi kar sakta.
Step 3 — floor lo aur dono sides count karo.
m m a x = ⌊ 2.78 ⌋ = 2.
Orders present: m = − 2 , − 1 , 0 , + 1 , + 2 → 5 maxima .
Yeh step kyun? Pattern centre ke baare mein symmetric hai: har positive order + m ka negative twin − m mirror angle par hai, aur m = 0 ek akela central spot hai — yahi 2 m m a x + 1 deta hai.
Verify: Check karo order 2 real hai: sin θ 2 = 2 × 450 × 1 0 − 9 /1.25 × 1 0 − 6 = 0.72 ≤ 1 . ✓ Check karo order 3 impossible hai: 3 × 450/1250 = 1.08 > 1 → koi solution nahi. ✓ Count = 2 × 2 + 1 = 5 . ✓
Worked example Example 5 (Cell E)
White light (sab wavelengths 400–700 nm) kisi bhi grating par padti hai. Zero-order (m = 0 ) maximum kahan hai, aur uska colour kya hai?
Forecast: Kya zero-order angle colour par depend karta hai? Haan ya nahi guess karo.
Step 1 — m = 0 rule mein daalo.
d sin θ 0 = 0 ⋅ λ = 0 ⇒ sin θ 0 = 0 ⇒ θ 0 = 0 ∘ .
Yeh step kyun? Zero extra path difference ke saath, har wavelength seedha aage constructively interfere karti hai.
Step 2 — colour ke baare mein soco.
Kyunki θ 0 = 0 λ se independent hai, sab colours ek hi jagah land karte hain aur recombine ho jaate hain.
Yeh step kyun? Koi wavelength bend nahi hoti, isliye centre par koi dispersion nahi hoti.
Figure mein kya dekhna hai: seedha aage wala red arrow m = 0 ray hai — notice karo yeh ek single arrow hai jo har colour ko ek saath carry karta hai, kyunki sab wavelengths θ = 0 par pile ho jaati hain. Ab upar aur neeche fan karte black arrows follow karo: woh m = ± 1 rays hain, aur yahan colours alag ho jaate hain (blue centre ke qareeb, red zyada door) kyunki m ≥ 1 ke liye angle finally λ par depend karta hai. Picture is cell ka poora point hai: centre white hai; fans coloured hain.
Verify: Equation θ 0 = 0 deta hai λ = 400 nm ke liye bhi aur λ = 700 nm ke liye bhi, isliye unke beech spread 0 ∘ hai — ek single white central maximum. ✓ (Sirf m ≥ 1 ke liye colours spectra mein fan out karte hain.)
Worked example Example 6 (Cell F)
Ek grating ka spacing d = 1200 nm hai. λ = 600 nm ke liye, kya second-order maximum exist karta hai? Woh kahan appear hota hai, aur kya hoga agar tum λ thoda bada kar do?
Forecast: d / λ = 2 exactly — ek razor-edge case. Kya order 2 visible hoga, invisible hoga, ya edge par grazing hoga?
Step 1 — sin θ 2 compute karo.
sin θ 2 = d mλ = 1200 2 × 600 = 1.000.
Yeh step kyun? Hum order ko ceiling sin θ ≤ 1 ke against test kar rahe hain.
Step 2 — sin θ = 1 interpret karo.
θ 2 = sin − 1 ( 1 ) = 9 0 ∘ .
Yeh step kyun? θ = 9 0 ∘ ka matlab hai ray grating surface ke saath saath skim karti hai — mathematically exist karti hai lekin infinitely spread hai aur aage screen tak kabhi nahi pahunchti. Yeh visibility ki exact boundary hai.
Step 3 — wavelength nudge karo.
λ = 610 nm ke liye: sin θ 2 = 2 × 610/1200 = 1.017 > 1 . Koi real angle nahi — order 2 gayab ho jaata hai.
Yeh step kyun? Yeh dikhata hai ki boundary ek genuine cliff hai: d / λ = m se thoda sa aage jaate hi woh order disappear ho jaata hai.
Verify: λ = 600 nm par, m m a x = ⌊ 1200/600 ⌋ = 2 (edge counts). λ = 610 nm par, ⌊ 1200/610 ⌋ = ⌊ 1.97 ⌋ = 1 — order 2 gone. ✓
Worked example Example 7 (Cell G)
500 lines/mm ki grating par do lines se light padti hai: λ 1 = 486 nm (blue) aur λ 2 = 656 nm (red), dono hydrogen se. First order mein in do lines ka angular separation nikalo.
Forecast: Kaun sa colour zyada bend hoga — shorter blue ya longer red? Compute karne se pehle guess karo.
Step 1 — d nikalo.
d = 500 mm − 1 1 = 2.0 × 1 0 − 6 m .
Step 2 — har colour ka angle (m = 1 ).
sin θ 1 , blue = 2.0 × 1 0 − 6 486 × 1 0 − 9 = 0.243 ⇒ θ = 14.0 6 ∘ .
sin θ 1 , red = 2.0 × 1 0 − 6 656 × 1 0 − 9 = 0.328 ⇒ θ = 19.1 4 ∘ .
Yeh step kyun? Same equation do baar apply ki; sirf λ badla, isliye longer wavelength ko bada angle milna chahiye.
Step 3 — subtract karo.
Δ θ = 19.1 4 ∘ − 14.0 6 ∘ = 5.0 8 ∘ .
Yeh step kyun? "Angular separation" literally do directions ke beech ka gap hai, isliye hum do coloured spots kitne door hain yeh nikalne ke liye chhote angle ko bade se subtract karte hain.
Verify: Red (656 ) blue (486 ) se zyada bend karta hai kyunki sin θ ∝ λ — yeh consistent hai ki grating red ko sabse door fan karta hai, raindrop se opposite lekin yahan correct. Separation ≈ 5. 1 ∘ aasani se resolvable hai; yahi Resolving power and spectrometers ka basis hai. ✓
Worked example Example 8 (Cell H)
Ek astronomer starlight ko ek spectrometer mein feed karta hai jiskin grating mein 1200 lines/mm hai. Ek calcium absorption line first order mein measured angle θ = 28. 4 ∘ par appear hoti hai. Wavelength kya hai, aur kya yeh known Ca II K line ≈ 393.4 nm se match karti hai?
Forecast: 1200 lines/mm ek fine grating hai (small d ). Near-UV light ke liye first order small angle par hoga ya large angle par? Guess karo.
Step 1 — numbers extract karo. Maano N ℓ = 1200 lines/mm ruling density hai (grating ke liye quoted "lines per mm"), m = 1 , θ = 28. 4 ∘ .
Yeh step kyun? Word problems variables ko prose mein chhupaate hain — pehle unhe name karo. Note karo N ℓ lines per length hai; spacing d uska reciprocal hai, exactly jaise har example mein upar.
Step 2 — d nikalo.
d = N ℓ 1 = 1200 mm − 1 1 = 8.333 × 1 0 − 7 m .
Step 3 — λ ke liye solve karo.
λ = m d s i n θ = 1 8.333 × 1 0 − 7 × s i n 28. 4 ∘ .
sin 28. 4 ∘ = 0.4756 , λ = 8.333 × 1 0 − 7 × 0.4756 = 3.96 × 1 0 − 7 m = 396 nm .
Verify: 396 nm violet/near-UV mein hai. Yeh Ca II H line ≈ 396.8 nm ke sabse qareeb hai, K line 393.4 nm ke nahi — yeh genuinely useful distinction hai, kyunki H aur K lines do famous calcium absorption features hain aur sirf ≈ 3 nm apart hain. Plug back: d sin θ = 8.333 × 1 0 − 7 × 0.4756 = 3.96 × 1 0 − 7 m = 1 ⋅ λ . ✓
Worked example Example 9 (Cell I)
Ek grating par, red light λ R = 700 nm apne second order mein ek shorter wavelength λ x ke third order ke saath overlap karti hai (same angle). λ x kya hai, aur uska colour kya hai?
Forecast: Same angle ke liye, kya higher order ko longer ya shorter wavelength chahiye? Guess karo.
Step 1 — overlap condition likho.
Same d , same θ , isliye d sin θ ki value dono rays ke liye identical hai. Har ray ke liye grating rule ek baar likhte hain:
d sin θ = m R λ R and d sin θ = m x λ x ,
isliye left-hand sides match karte hain aur
m R λ R = m x λ x ⇒ 2 × 700 = 3 × λ x .
Yeh step kyun? "Same angle" ka matlab hai d sin θ dono ke liye common hai — do mλ products equal set karo. d aur sin θ cancel ho jaate hain, isliye grating spacing kabhi enter hi nahi karta!
Step 2 — solve karo.
λ x = 3 2 × 700 = 466.7 nm .
Yeh step kyun? Seedha algebra: known product m R λ R ko doosre order m x = 3 se divide karo.
Step 3 — identify karo.
466.7 nm visible band mein blue hai.
Yeh step kyun? Bare number ko physical colour mein convert karte hain taaki answer meaningful ho, sirf arithmetic nahi.
Verify: Equal path difference check karo — koi bhi grating lo, maano d = 2000 nm. Red order 2: sin θ = 2 × 700/2000 = 0.700 . Blue order 3: sin θ = 3 × 466.7/2000 = 0.700 . Identical angle ✓. Higher order ko shorter wavelength chahiye — jaise forecast mein check kiya.
Common mistake Overlap problems:
d mat laao
Kyun sahi lagta hai: Har doosra grating problem d maangta hai, isliye students yahan bhi dhundne lagte hain. Fix: Jab do maxima same angle share karte hain, quantity d sin θ dono rays ke liye common hai. Har ke liye grating rule likho (d sin θ = m 1 λ 1 aur d sin θ = m 2 λ 2 ), dekho left-hand sides equal hain, aur m 1 λ 1 = m 2 λ 2 set karo. d sin θ completely cancel ho jaata hai, isliye tum unknown wavelength (ya order) spacing jaane bina solve karte ho — jaisa Example 9 dikhata hai.
Common mistake Count karte waqt negative orders bhoolna
Kyun sahi lagta hai: Tum ek angle ke liye solve karte ho, ek bright spot dekhte ho, aur wahi count report karte ho. Fix: Har order + m ke liye ek mirror order − m hai − θ par (upar signs wala intuition dekho). Total 2 m m a x + 1 hota hai, hamesha odd kyunki single m = 0 centre ka koi twin nahi hota.
Recall Poora matrix self-test karo
Yeh kaunse cell honge? "Measured angle se lines/mm nikalo" ::: Cell B (backward for d ).
"Screen par kitne spots hain?" ::: Cell D (counting orders, ± m yaad rakho).
"Kya order 4 exist karta hai?" ::: Cell F (limiting / boundary at sin θ ≤ 1 ).
"Do spectral lines ka angular gap" ::: Cell G (dispersion).
"Colour x order 3 red order 2 se overlap karta hai" ::: Cell I (overlapping orders).
Har cell same equation hai ek alag letter ke liye solve ki gayi: "d sin θ = mλ — jo letter chahiye use cover karo, uske liye solve karo." Angle → sin − 1 ( mλ / d ) . Spacing → mλ / sin θ . Wavelength → d sin θ / m . Count → 2 ⌊ d / λ ⌋ + 1 .