WHY T−V and not T+V? Energy conservation (T+V) is constant along the true path — it carries no information distinguishing paths. The differenceT−V is what gets "balanced" over time: the system trades kinetic for potential and the integral of the trade-off is extremized.
We want: whichq(t) kills δS? Perturb the true path:
q(t)→q(t)+εη(t),η(t1)=η(t2)=0,
where η is an arbitrary smooth "wiggle" that vanishes at the fixed endpoints (WHY zero there? endpoints are held fixed — we don't get to vary them).
The action becomes a function of ε:
S(ε)=∫t1t2L(q+εη,q˙+εη˙,t)dt.
Stationary means dεdSε=0=0. Differentiate under the integral (chain rule):
dεdS0=∫t1t2(∂q∂Lη+∂q˙∂Lη˙)dt.
Why this step? Each path-component picks up a derivative of L; η multiplies the q-slot, η˙ the q˙-slot.
Now integrate the second term by parts to free η˙ into η:
∫t1t2∂q˙∂Lη˙dt==0(η vanishes at ends)[∂q˙∂Lη]t1t2−∫t1t2dtd(∂q˙∂L)ηdt.
Why this step? The boundary term dies because η(t1)=η(t2)=0 — this is exactly why fixed endpoints matter. Substituting back:
dεdS0=∫t1t2(∂q∂L−dtd∂q˙∂L)η(t)dt=0.
This must hold for every wiggle η. By the Fundamental Lemma of Calculus of Variations (if ∫fηdt=0 for all η, then f≡0), the bracket must vanish:
WHY this recovers Newton: for L=21mx˙2−V(x):
∂x˙∂L=mx˙, so dtd(mx˙)=mx¨; and ∂x∂L=−V′(x)=F.
Euler–Lagrange gives mx¨−F=0⇒F=mx¨. Newton's law falls out for free.
Imagine you must walk from your house to a friend's house and you'll be graded by a weird "tiredness score" added up over the whole trip. Nature plays the same game with every moving thing: it adds up a score (the action) along each possible route. The route that the ball, planet, or pendulum actually takes is the one where you couldn't make the score any better by nudging the route a tiny bit — it's perfectly balanced. So instead of asking "what force pushes it now?", you ask "which whole path is the smartest overall?" Both questions give the same answer, but the path-question is often much easier.
Dekho, idea bahut elegant hai. Newton bolta hai "har pal force lagao, F=ma solve karo." Hamilton ek doosra angle deta hai: kisi bhi object ke saare possible raaste socho jo start point se end point tak jaate hain. Har raaste ke liye ek number nikaalo jise actionS=∫(T−V)dt kehte hain — yaani kinetic energy minus potential energy ka time ke upar integral. Asli raasta wahi hota hai jahan ye action stationary ho jaye, matlab thoda sa path hilao to S change na ho (first order me). Isko δS=0 likhte hain.
Ab WHY T−V? Kyunki T+V (total energy) to constant rehti hai, woh paths ko distinguish nahi karti. T−V ka time-average balance hota hai, aur usi balance se asli trajectory decide hoti hai. Jab hum is condition ko maths se solve karte hain (path ko thoda perturb karo q+εη, integrate by parts, endpoints pe wiggle zero hone se boundary term mar jaata hai, phir fundamental lemma), to Euler–Lagrange equation nikalti hai: dtd∂q˙∂L=∂q∂L. Aur agar L=21mx˙2−V daalo to seedha mx¨=−V′(x), yaani Newton ka law! Toh dono same physics, bas dekhne ka tareeka alag.
Practical fayda: pendulum ya complicated systems me forces aur tensions resolve karna painful hota hai. Lekin agar aap sirf T aur V angle θ me likh do, geometry apne aap handle ho jaati hai — koi free-body diagram nahi. Ek important warning: "least action" naam se lagta hai hamesha minimum, par actually stationary hota hai, kabhi-kabhi saddle bhi. Isliye exam me "principle of stationary action" bolna safe hai. Yaad rakho mantra: Wiggle karo, integrate by parts, ends phenk do, lemma se bracket zero.