Pieces chunno. Sirf ek coordinate hai, y. Velocity y˙ hai, toh kinetic energy hai
T=21my˙2.
Gravity neeche pull karti hai; potential energy height ke saath badhti hai:
V=mgy⇒L=T−V=21my˙2−mgy.Machine chalao. Euler-Lagrange machine ke do ingredients:
∂y˙∂L=my˙⇒dtd(my˙)=my¨,∂y∂L=−mg.
Subtract karo:
my¨−(−mg)=0⇒my¨+mg=0⇒y¨=−g.
Acceleration gneeche ki taraf hai — bilkul Newton ki tarah. ✓
x=ℓsinθ,y=−ℓcosθ ke saath, speed ℓθ˙ hai, toh
T=21mℓ2θ˙2,V=−mgℓcosθ,L=21mℓ2θ˙2+mgℓcosθ.∂θ˙∂L=mℓ2θ˙⇒dtd=mℓ2θ¨,∂θ∂L=−mgℓsinθ.
EL: mℓ2θ¨+mgℓsinθ=0⇒θ¨=−ℓgsinθ.Small angles:sinθ≈θ, toh θ¨=−ℓgθ. Ye SHM hai with
ω=ℓg,Tperiod=2πgℓ.
Position (angle from bottom): x=Rsinθ,y=−Rcosθ (bottom y=−R par hai). Ye form mein pendulum se identical hai ℓ→R ke saath — hoop wahi rigid constraint provide karta hai jo rod karta tha, aur normal force radius ke along point karti hai, allowed (tangential) motion ke perpendicular, isliye ye no virtual work karti hai aur kabhi appear nahi hoti.
T=21mR2θ˙2,V=−mgRcosθ.θ¨=−Rgsinθ.
Same physics, nayi geometry. ✓
Bead ki velocity mein ek radial part r˙ aur ek tangential part rω (wire ke spinning se) hai. Ye perpendicular hain, toh
T=21m(r˙2+r2ω2),V=0.
Yahan r2ω2 depends on r karta hai, toh ∂T/∂r=0 — yahi poora point hai.
∂r˙∂T=mr˙⇒dtd=mr¨,∂r∂T=mrω2.
EL (Qr=0): mr¨−mrω2=0⇒r¨=ω2r.
Positive sign ka matlab hai bead baahir ki taraf jaati hai — centrifugal effect automatically ∂T/∂r se nikal aaya. Solution r(t)=Aeωt+Be−ωt: exponential escape. ✓
Agar m1x se neeche jaata hai, toh m2x se upar jaata hai (string inextensible hai — ye constraint hai). Dono x˙ speed se chalte hain:
T=21(m1+m2)x˙2.
Heights: m1 at −x, m2 at −(ℓ−x)=x−ℓ. Toh
V=−m1gx+m2g(x−ℓ)=(m2−m1)gx−m2gℓ.∂x˙∂L=(m1+m2)x˙⇒dtd=(m1+m2)x¨,∂x∂L=−(m2−m1)g=(m1−m2)g.
EL: (m1+m2)x¨−(m1−m2)g=0⇒x¨=m1+m2(m1−m2)g.
Tension kabhi appear nahi hui — ye internal constraint force hai, single coordinate x choose karne se khatam ho gayi. ✓
T=21MX˙2+21mx˙2,V=21k(x−X)2.L=21MX˙2+21mx˙2−21k(x−X)2.X ke liye equation:∂X˙∂L=MX˙,∂X∂L=−21k⋅2(x−X)⋅(−1)=k(x−X).⇒MX¨−k(x−X)=0⇒MX¨=k(x−X).x ke liye equation:∂x˙∂L=mx˙,∂x∂L=−k(x−X).⇒mx¨=−k(x−X).
Newton's third law dikh raha hai: dono forces equal aur opposite hain. ✓
Bob position (pivot at height yp):
x=ℓsinθ,y=yp−ℓcosθ.
Velocities: x˙=ℓθ˙cosθ, y˙=y˙p+ℓθ˙sinθ.
x˙2+y˙2=ℓ2θ˙2+y˙p2+2ℓθ˙y˙psinθ.T=21m(ℓ2θ˙2+y˙p2+2ℓθ˙y˙psinθ),V=mgy=mg(yp−ℓcosθ).y˙p2 aur mgyp pieces sirf time par depend karti hain, θ ya θ˙ par nahi, toh ye EL derivatives se drop ho jaati hain. Relevant parts rakho:
∂θ˙∂L=mℓ2θ˙+mℓy˙psinθ.dtd∂θ˙∂L=mℓ2θ¨+mℓy¨psinθ+mℓy˙pθ˙cosθ.∂θ∂L=mℓθ˙y˙pcosθ−mgℓsinθ.
Subtract karo; mℓy˙pθ˙cosθ terms cancel ho jaate hain:
mℓ2θ¨+mℓy¨psinθ+mgℓsinθ=0.y¨p=−aΩ2cos(Ωt) ke saath:
θ¨=−ℓ1(g−aΩ2cosΩt)sinθ.
Drive ek time-varying effective gravitygeff(t)=g−aΩ2cosΩt ki tarah act karta hai. (Ye famous inverted-pendulum stabilization ka seed hai.) ✓
Koi potential nahi, toh dtd∂x˙∂T−∂x∂T=Qx use karo.
T=21mx˙2,Qx=F⋅∂x∂r=F(t)⋅1=F0sin(Ωt).mx¨=F0sin(Ωt)⇒x¨=mF0sin(Ωt).
Ek baar integrate karo (x˙(0)=0):
x˙=mΩF0(1−cosΩt).
Dobara integrate karo (x(0)=0):
x(t)=mΩF0(t−ΩsinΩt).
Bead drift karta hai (t term) saath mein wiggle karte hue — ek oscillating force se net secular motion. ✓
T=21mx˙2+21Iϕ˙2,V=0(level ground).
Constraint x˙−Rϕ˙=0 non-holonomic hai (ismein velocities hain); δqiindependent nahi hain, toh hum multiplier terms append karte hain. Modified equations hain dtd∂q˙i∂L−∂qi∂L=λai, jahan ax=1,aϕ=−R constraint axx˙+aϕϕ˙=0 se aate hain.
x equation:mx¨=λ.
ϕ equation:Iϕ¨=−λR⇒21mR2ϕ¨=−λR⇒21mRϕ¨=−λ.Constraint (differentiated):x¨=Rϕ¨.
ϕ equation mein ϕ¨=x¨/R substitute karo: 21mR⋅x¨/R=−λ⇒21mx¨=−λ.
mx¨=λ ke saath combine karo:
21(λ)=−λ⇒23λ=0⇒λ=0,x¨=0.
Level ground par bina kisi driving ke, friction (constraint) force λzero hai aur hoop constant speed par roll karta hai — friction sirf tab zaroori hoti hai jab kuch rolling change karne ki koshish kare. Multiplier λwahi friction force hai. Dekho Lagrange multipliers for non-holonomic constraints. ✓
Recall Self-test: tool ko situation se match karo
Constraint force explicitly chahiye, non-holonomic ::: Lagrange multiplier λ (raw form with λai)
Force −∂V/∂q hai, holonomic ::: standard L=T−V Euler-Lagrange
Explicit time-dependent driving force, no potential ::: raw form with generalized force QiL mein qi nahi hai (sirf q˙i) ::: cyclic coordinate, ∂L/∂q˙i conserved