KYA:y=0 par, u=0.
KYUN: Ek real fluid mein viscosity hoti hai, isliye wall se touch karne wala fluid ka layer uske upar slide nahi kar sakta — woh wall ke saath hi move karta hai. Ek stationary wall isliye u(0)=0 deti hai. Yahi no-slip condition hai.
Answer:u(0)=0, no-slip condition se force hota hai.
Recall Solution 1.2
Order:θ<δ∗<δ.
θ sabse chhota KYUN: iska integrand Uu(1−Uu) 0 aur 1 ke beech ke do fractions ka product hai, isliye yeh har jagah us single fraction (1−Uu) se chhota hai jo δ∗ banata hai. Chhota integrand ek chhota integral deta hai.
Recall Solution 1.3
Sirf 0→δ integrate karo. KYUN:δ ke baad fluid free-stream speed par move karta hai, u=U, isliye 1−Uu=0 aur Uu(1−Uu)=0 hota hai. Integrand vanish ho jaata hai, kuch contribute nahi karta — ∞ ek bookkeeping hai "jahan bhi deficit rehta hai" ke liye.
KYA:Uu=δy ko δ∗=∫0δ(1−Uu)dy mein substitute karo.
KYUN substitute karo:δ∗fractional velocity deficit1−u/U ko height par stack karke count karta hai; use add karne ke liye humein woh deficit y ke function ke roop mein chahiye, jo profile humein deti hai.
δ∗=∫0δ(1−δy)dy=[y−2δy2]0δ=δ−2δ=2δKYUN δ/2 aata hai: deficit 1−y/δ seedha 1 (wall par full deficit) se 0 (edge par koi deficit nahi) tak girta hai. Ek base δ par 1 se 0 tak seedhi line ke neeche ka area ek triangle hai — box ka bilkul aadha, isliye δ/2.
Answer:δ∗=2δ=0.5δ.
Recall Solution 2.2
KYUN integrand badalta hai: momentum deficit velocity gap (1−u/U) ko is baat se weight karta hai ki wahan actually kitna mass move kar raha hai, u/U — isliye hum dono ko multiply karte hain, jo δy(1−δy) deta hai.
θ=∫0δδy(1−δy)dy=∫0δ(δy−δ2y2)dy=2δ−3δ=6δKYUN θ<δ∗ yahan: extra factor y/δ ek fraction ≤1 hai, isliye yeh deficit ko har jagah shrink karta hai — integral chhota hi aana chahiye (δ/6<δ/2), jo Exercise 1.2 se consistent hai.
H=θδ∗=δ/6δ/2=3Answer:θ=6δ, H=3.
Recall Solution 2.3
KYUN pehle Rex: Blasius law δ=5x/Rex ko Rex chahiye, aur Rex measure karta hai ki inertia (Ux) viscous diffusion (ν) ko kitna strongly beat karta hai — bada value matlab patli layer.
Rex=νUx=1.5×10−530×0.5=1.5×10−515=106KYUN Blasius law mein plug karo: yeh exact laminar flat-plate result hai; Rex=106=1000 shrink factor hai.
δ=Rex5x=10005×0.5=10002.5=2.5×10−3m=2.5mmAnswer:Rex=106, δ=2.5mm.
KYUN sine? Yeh u=0 wall par aur u=Uy=δ par smoothly satisfy karta hai (iska slope edge par flat ho jaata hai) — true profile ka ek realistic stand-in, unlike kinked linear wale ke.
KYUN sine integrate karo:δ∗ abhi bhi deficit 1−u/U sum karta hai; humein bas ab curved deficit mila hai, isliye humein sin ka antiderivative chahiye.
δ∗=∫0δ(1−sin2δπy)dy=δ−[−π2δcos2δπy]0δKYUN 2δ/π factor:cos(2δπy) par chain rule 2δπ bahar laata hai, isliye jab hum antidifferentiate karte hain toh iska reciprocal π2δ appear hota hai.
Cosine term: y=δ par, cos2π=0; y=0 par, cos0=1. Toh bracket hai −π2δ(0−1)=π2δ.
δ∗=δ−π2δ=δ(1−π2)≈0.3634δAnswer:δ∗=δ(1−π2)≈0.363δ.
Recall Solution 3.2
KYUN do integrals mein split karo:sin(1−sin)=sin−sin2 expand karna ek aisa piece alag karta hai jo humein pehle se pata hai (∫sin) aur ek naya (∫sin2), toh har ek ko ek jaane-maane result se handle kiya ja sakta hai.
θ=∫0δsin2δπy(1−sin2δπy)dy==2δ/π∫0δsin2δπydy−=δ/2∫0δsin22δπydyKYUN identity ki zarurat hai:sin2 ka apna koi elementary antiderivative nahi hai, isliye hum ise sin2ϕ=21−cos2ϕ se rewrite karte hain, jiska is quarter-period par average 21 hai, jo δ/2 deta hai.
θ=π2δ−2δ=δ(π2−21)≈0.1366δH=θδ∗=0.13660.3634≈2.66KYUN 2.59 se compare karo:H ek shape fingerprint hai jo δ se independent hai; sine ka 2.66 exact Blasius 2.59 ke paas land karna iska evidence hai ki sine real profile ko achhi tarah mimic karta hai.
Answer:θ≈0.137δ, H≈2.66 — true Blasius 2.59 ke bahut kareeb, isliye sine profile ek achha approximation hai.
Recall Solution 3.3
KYUN pehle ends check karo: ek candidate profile tab hi physical hai jab woh no-slip se start kare (u=0) aur free stream se mile (u=U) — warna deficit integrals meaningless hain.
Ends check karo.y=0 par: u/U=0 ✓ (no-slip). y=δ par: u/U=2−1=1 ✓.
KYUN substitution η=y/δ: yeh ek δ-cluttered integral ko 0 se 1 tak ek clean number-integral mein badal deta hai, aur δ ka ek factor front mein bahar nikaalta hai (dy=δdη se) — isliye answer ek pure fraction times δ hona chahiye.
δ∗=δ∫01(1−2η+η2)dη=δ[η−η2+3η3]01=δ(1−1+31)=3δAnswer:δ∗=3δ≈0.333δ.
KYUN product expand karo:θ ko Uu(1−Uu) chahiye, aur u/U=2η−η2 ke saath yeh ek polynomial hai — ise multiply out karne se aisi terms milti hain jo hum ek power at a time integrate kar sakte hain.
η=y/δ aur u/U=2η−η2 ke saath:
(2η−η2)(1−2η+η2)=2η−5η2+4η3−η4θ=δ∫01(2η−5η2+4η3−η4)dη=δ[η2−35η3+η4−5η5]01KYUN 15 par collect karo: denominators 1,3,1,5 ka least common multiple 15 hai, isliye common denominator sum ko exact banata hai decimal-rounded ki jagah.
=δ(1−35+1−51)=δ⋅1515−25+15−3=152δH=θδ∗=2δ/15δ/3=615=2.5KYUN H=2.5 sense banata hai: parabola linear line se "fuller" hai, isliye woh kam fluid slow karti hai — linear H=3 se chhota shape factor, bilkul waise jaise opening figure ne predict kiya tha.
Answer:θ=152δ≈0.133δ, H=2.5.
Recall Solution 4.2
Values: linear H=3.00; sine H≈2.66; parabolic H=2.50. True Blasius H≈2.59.
KYUN H sahi yardstick hai: yeh δ ko strip away karta hai aur sirf deficit ki shape capture karta hai, isliye models ko Blasius' 2.59 se compare karna ek fair, size-independent test hai.
Ranking (Blasius ke sabse kareeb pehle): sine (2.66) ≈ parabolic (2.50) > linear (3.00).
Sabse bekar model:linear profile, H=3.00, 2.59 se sabse door hai. KYUN: ek seedhi line y=δ par ek sharp kink rakhti hai (nonzero slope flat free stream se milti hui) aur constant shear — real profiles curve over hoti hain aur smoothly flatten karti hain. Sine aur parabola dono δ ke paas flatten hote hain, jo reality se zyada match karta hai.
Recall Solution 4.3
KYUN δ∗=δ/2, θ=δ/6 reuse karo: woh ratios purely linear profile ki shape se aayi theen, isliye woh har x par hold karti hain — hum bas x-dependent δ feed karte hain.
Exercise 2.1–2.2 se: δ∗=δ/2, θ=δ/6. Toh
δ∗=21⋅Rex5x=Rex2.5x,θ=61⋅Rex5x=Rex0.8333xKYUN numbers instantly follow karte hain:x=0.5 par humne pehle hi δ=2.5mm find kar liya tha (Exercise 2.3), isliye sirf use half aur sixth karna baaki hai.
x=0.5 par: Rex=106, δ=2.5mm.
δ∗=22.5=1.25mm,θ=62.5=0.4167mmAnswer:δ∗=1.25mm, θ≈0.417mm (θ<δ∗<δ confirm hota hai).
KYUN η mein karo:η=y/δ ke saath profile bas η1/n hai aur har integral 0→1 run karta hai, isliye hum ek hi stroke mein sabn ke liye valid formulas paate hain — har pehle special case ki ek synthesis.
δδ∗=∫01(1−η1/n)dη=1−n1+11=1−n+1n=n+11KYUN power-rule step:∫01η1/ndη=n1+11=n+1n; 1 se subtract karne par n+11 bachta hai.
δθ=∫01η1/n(1−η1/n)dη=∫01(η1/n−η2/n)dη=n+1n−n+2n=(n+1)(n+2)nKYUN extra η2/n term:η1/n ko square karne se exponent double hota hai, jo second integral n+2n deta hai; difference ek single fraction mein collapse ho jaata hai.
Shape factor:H=θ/δδ∗/δ=n/[(n+1)(n+2)]1/(n+1)=nn+2.
n=7 ke liye:δδ∗=81=0.125,δθ=8⋅97=727≈0.0972,H=79≈1.286KYUN H≈1.29 "fuller" hai: bada nη1/n ko wall ke paas fast upar le jaata hai — zyada fluid already U ke paas hai, tiny deficit, isliye H laminar values se bahut neeche baithta hai.
Answer:δ∗=δ/(n+1), θ=(n+1)(n+2)nδ, H=nn+2; n=7 par: δ∗=0.125δ, θ≈0.0972δ, H≈1.29.
Recall Solution 5.2
KYUN limit lo: ek parameter ko extreme par push karna ek formula ko physically sane hai ya nahi test karne ka sabse sasta tarika hai — agar yah yahan toota, toh galat hai.
Jaise n→∞, har η>0 ke liye η1/n→1: fluid wall par ek infinitely thin sliver ko chhodkar har jagah full speed U par hai — yeh ek plug (slug) profile hai.
δδ∗=n+11→0,δθ=(n+1)(n+2)n→0,H=nn+2→1Physical sense: jab almost koi slowed fluid nahi hai toh almost koi mass ya momentum deficit nahi hai, isliye δ∗→0 aur θ→0. Aur H→1 theoretical minimum shape factor hai — flow jitna ho sake utna "full" hai, separation se bilkul ulta extreme. ✓
Recall Solution 5.3
KYUN integrands compare karo, integrals nahi: agar ek integrand har height par ≤ doosre ka hai, toh integral woh inequality inherit karta hai — yeh kisi bhi integral compute kiye bina ordering prove karne ka sabse clean tarika hai.
Dono ko same dy ke saath integrals likhein aur f=Uu lo, jo 0≤f≤1 satisfy karta hai:
δ∗=∫0∞(1−f)dy,θ=∫0∞f(1−f)dyKYUN pointwise bound hold karta hai: kyunki 0≤f≤1, factor (1−f)≥0 hai, aur ek non-negative number ko f≤1 se multiply karna use sirf shrink kar sakta hai (ya hold):
f(1−f)≤1⋅(1−f)=(1−f)
Kyunki yeh har height y par hold karta hai, integrate karna inequality preserve karta hai:
θ=∫f(1−f)dy≤∫(1−f)dy=δ∗
Isliye θ≤δ∗, yaani H=δ∗/θ≥1 hamesha. δ∗<δ ke saath combine karke (deficit slab poori layer se pateeli hai), hum θ<δ∗<δ recover karte hain. ■
Recall One-line self-test summary
Linear H=3 ::: parabolic H=2.5 ::: sine H≈2.66 ::: Blasius H≈2.59 ::: 71-power H≈1.29 ::: aur hamesha H≥1.