4.4.31 · Maths › Multivariable Calculus
Ek line integral ek curve (1D) ke saath quantity ko add karta hai. Ek surface integral 3D space mein rehne wali ek surface (2D) ke upar quantity ko add karta hai.
Scalar surface integral ∬ S f d S : "Agar f ek curved sheet ki density (mass per area) hai, toh uska total mass kya hoga?"
Vector surface integral / flux ∬ S F ⋅ d S : "Agar F kisi fluid ki velocity hai, toh kitna fluid surface ke andar se per second guzarta hai?"
Poora trick yeh hai: ek curved surface mushkil hai, lekin ek flat parameter rectangle easy hai. Hum ek flat ( u , v ) region ko surface pe map karte hain aur dekhte hain ki map area ko kitna stretch karta hai.
Definition Parametrized surface
Ek surface ek vector map hai jo uv -plane ke 2D region D se 3D mein jaata hai:
r ( u , v ) = ( x ( u , v ) , y ( u , v ) , z ( u , v ) ) , ( u , v ) ∈ D .
v ko fixed rakh ke u ko vary karne se surface pe ek curve trace hoti hai; isi tarah u fixed ke saath bhi.
Stretch factor kyun chahiye? Jab hum parameters ko tiny amounts d u , d v se move karte hain, toh surface pe point tangent vectors ke zariye move karta hai
r u = ∂ u ∂ r , r v = ∂ v ∂ r .
Chhota sa parameter square d u d v ek tiny parallelogram mein map ho jaata hai jo r u d u aur r v d v se bana hota hai.
Intuition Parallelogram ka area = cross product ka magnitude
Vectors a aur b se bane parallelogram ka area ∥ a × b ∥ hota hai, kyunki ∥ a × b ∥ = ∥ a ∥∥ b ∥ sin θ = (base)(height).
Toh real surface area ka tiny patch hai
d S = ∥ r u × r v ∥ d u d v .
Yeh ∥ r u × r v ∥ Jacobian ka 2D analogue hai — yeh area scaling factor hai.
Agar f = 1 , toh tumhe surface area ∬ S d S milta hai.
Agar f = density, toh total mass milta hai.
Worked example Graph surface
z = g ( x , y ) — sabse common special case
u = x , v = y se parametrize karo: r ( x , y ) = ( x , y , g ( x , y )) .
r x = ( 1 , 0 , g x ) , r y = ( 0 , 1 , g y ) .
Yeh step kyun? Yeh x - aur y -directions ke saath tangent vectors hain.
r x × r y = ( − g x , − g y , 1 ) ⇒ ∥ r x × r y ∥ = 1 + g x 2 + g y 2 .
Yeh step kyun? Cross product normal deta hai; uski length stretch factor hai.
∬ S f d S = ∬ D f ( x , y , g ) 1 + g x 2 + g y 2 d x d y .
a ke hemisphere ka area
Sphere x 2 + y 2 + z 2 = a 2 , upper half z = a 2 − x 2 − y 2 disk D : x 2 + y 2 ≤ a 2 ke upar.
g x = a 2 − x 2 − y 2 − x , g y = a 2 − x 2 − y 2 − y .
Kyun? g ko differentiate karo; stretch factor ke liye slopes chahiye.
1 + g x 2 + g y 2 = 1 + a 2 − x 2 − y 2 x 2 + y 2 = a 2 − x 2 − y 2 a 2 .
Toh d S = a 2 − x 2 − y 2 a d x d y . Polar switch karo (x 2 + y 2 = ρ 2 ):
=2\pi a\Big[-\sqrt{a^2-\rho^2}\Big]_0^a = 2\pi a^2.$$
*Polar kyun?* Disk aur integrand radially symmetric hain → clean integral. Result $2\pi a^2$ = $4\pi a^2$ ka aadha. ✔
Definition Unit normal aur orientation
Ek orientable surface mein unit normal ka continuous choice hota hai
n ^ = ∥ r u × r v ∥ r u × r v .
n ^ (ya − n ^ ) choose karna surface ko orient karta hai: yeh "positive" side pick karta hai. (Möbius strip non-orientable hai — koi consistent choice exist nahi karti.)
Intuition Flux kya measure karta hai
Socho fluid velocity field F ke saath hai. Area d S aur unit normal n ^ wale ek tiny patch se, sirf F ka component n ^ ke along fluid ko surface ke andar se carry karta hai. Sideways flow saath mein slide karta hai, andar se nahi.
Toh patch se flow rate hai ( F ⋅ n ^ ) d S .
Intuition Magnitude cancellation itni beautiful kyun hai
Scalar integrals mein tumhe square root ∥ r u × r v ∥ compute karni padti hai jo aksar ugly hoti hai. Flux mein tum kabhi woh square root nahi lete — bas F ko directly r u × r v se dot karo. Flux aksar scalar integrals se easier hota hai!
z = g ( x , y ) se flux, upward normal ke saath
r x × r y = ( − g x , − g y , 1 ) (yeh upward point karta hai kyunki iska z -component + 1 > 0 hai).
F = ( P , Q , R ) ke saath:
∬ S F ⋅ d S = ∬ D ( − P g x − Q g y + R ) d x d y .
F = ( x , y , z ) ka unit sphere se outward flux
Parametrize karo: r ( ϕ , θ ) = ( sin ϕ cos θ , sin ϕ sin θ , cos ϕ ) , ϕ ∈ [ 0 , π ] , θ ∈ [ 0 , 2 π ] .
Yeh step kyun? Unit sphere pe r khud outward radial direction hai; F = r , toh flux "sab kuch straight out point karta hua" hona chahiye.
Compute karo r ϕ × r θ = sin ϕ r (outward normal sin ϕ se scale hoa — spherical area element).
Phir F ⋅ ( r ϕ × r θ ) = r ⋅ ( sin ϕ r ) = sin ϕ ∥ r ∥ 2 = sin ϕ (kyunki ∥ r ∥ = 1 ).
∬ S F ⋅ d S = ∫ 0 2 π ∫ 0 π sin ϕ d ϕ d θ = 2 π ⋅ 2 = 4 π .
Divergence Theorem se check karo: ∇ ⋅ F = 3 , unit ball ka volume = 3 4 π , toh flux = 3 ⋅ 3 4 π = 4 π . ✔
Common mistake "Flux ko bhi square root
∥ r u × r v ∥ chahiye."
Kyun sahi lagta hai: d S definition ∬ ( F ⋅ n ^ ) d S mein appear karta hai, aur d S mein square root hai.
Fix: n ^ d S = ∥ ⋯ ∥ r u × r v ⋅ ∥ ⋯ ∥ d u d v = ( r u × r v ) d u d v . Norm cancel ho jaata hai. F ⋅ ( r u × r v ) directly use karo — no root .
Common mistake Yeh bhool jaana ki flux ka ek SIGN hota hai (orientation).
Kyun sahi lagta hai: Scalar integrals ∬ f d S ≥ 0 hote hain f ≥ 0 ke liye, toh tum assume karte ho ki flux bhi aise hi hai.
Fix: Flux negative ho sakta hai. r u × r v ko r v × r u se swap karne par sign flip ho jaata hai. Hamesha check karo ki tumhara normal waise point kar raha hai jaisa problem puchh raha hai (jaise "outward").
F ⋅ ( r u × r v ) ki jagah F ⋅ r use karna.
Kyun sahi lagta hai: Sphere pe r hai normal direction, toh wahan accidentally kaam kar jaata hai.
Fix: Vector area element tangents ka cross product hai, position vector nahi. Sirf luck se sphere pe yeh align hote hain.
Common mistake Parametrization substitute kiye bina
f ( x , y , z ) plug karna.
Kyun sahi lagta hai: Tum f mein x , y , z "dekhte" ho.
Fix: Integrate karne se pehle sab kuch u , v ka function banana hoga: x → x ( u , v ) replace karo, wagera.
Recall Active recall — answers cover karo
Parametrization ke terms mein d S kya hai? → ∥ r u × r v ∥ d u d v .
Flux scalar integral se zyada easy kyun hota hai? → Norm cancel ho jaata hai; koi square root nahi.
Flux physically kya measure karta hai? → Field ka net flow surface ke andar se .
Agar orientation reverse karo toh kya badalta hai? → Flux sign flip ho jaata hai; scalar integral unchanged rehta hai.
Recall Feynman: 12 saal ke bacche ko explain karo
Socho ek bumpy net ek waterfall ke neeche pakdi hui hai. Scalar integral: Agar main poori net paint karna chahta hoon, toh mujhe kitna paint chahiye? Main har chhote square ka area add karta hoon — lekin tilted squares upar se dekhne par bade lagte hain, toh main unhe pehle stretch karta hoon (woh stretch hai ∥ r u × r v ∥ ). Flux: Agar main jaanna chahta hoon ki kitna paani net ke andar se guzarta hai, toh main sirf woh paani count karta hoon jo seedha holes se guzarta hai, net ke saath slide hone wala nahi. Net se nikla hua arrow (n ^ ) mujhe bataata hai "seedha andar se." Net ko flow ke flat rakho aur almost koi paani nahi guzarta — isliye hum normal ke saath dot product use karte hain.
Mnemonic Dono formulas yaad rakho
"Scalar Stretches, Flux Flows."
S calar → S tretch factor ∥ r u × r v ∥ rakho.
F lux → F ield cross product mein dot ho jaata hai, norm F all away kar jaata hai.
Parametrized surface r ( u , v ) ke liye area element d S kya hai? d S = ∥ r u × r v ∥ d u d v
Graph z = g ( x , y ) ke liye ∥ r x × r y ∥ kya hai? Scalar surface integral formula state karo. ∬ S f d S = ∬ D f ( r ) ∥ r u × r v ∥ d u d v
Parameters ke terms mein flux integral formula state karo. ∬ S F ⋅ d S = ∬ D F ( r ) ⋅ ( r u × r v ) d u d v
Flux us square root se kyun bachta hai jo scalar integrals ko chahiye? n ^ d S = ∥ ⋯ ∥ r u × r v ∥ ⋯ ∥ d u d v = ( r u × r v ) d u d v — norm cancel ho jaata hai
Flux integral kaun si physical quantity compute karta hai? Field F ka surface ke andar se net flow (jaise fluid volume per unit time)
Agar surface ki orientation reverse karo toh flux ka kya hota hai? Uska sign flip ho jaata hai (normal reverse ho jaata hai)
Vector area element d S kya hai? d S = n ^ d S = ( r u × r v ) d u d v
Unit sphere se outward F = ( x , y , z ) ka flux? 4 π (div thm se bhi: 3 ⋅ 3 4 π )
Radius a ke sphere ka surface area? 4 π a 2 (har hemisphere 2 π a 2 )
Koi surface non-orientable kyun hoti hai (ek example do)? Unit normal ka koi continuous choice nahi; jaise Möbius strip
Upward normal wale graph ke liye ( P , Q , R ) ka flux kya hai? ∬ D ( − P g x − Q g y + R ) d x d y
magnitude = parallelogram area
Parametrized surface r of u,v
Tangent vectors r_u and r_v
Graph formula sqrt 1+gx^2+gy^2
Line integral over curve 1D