2.1.9 · D4 · HinglishAnalytical Mechanics

ExercisesNoether's theorem — symmetry ↔ conservation law

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2.1.9 · D4 · Physics › Analytical Mechanics › Noether's theorem — symmetry ↔ conservation law

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Level 1 — Recognition

Exercise 1.1 — Cyclic coordinate dhundo

Ek bead ek frictionless horizontal table par slide kar rahi hai, polar coordinates mein describe ki gayi: Kaun sa coordinate cyclic (ignorable) hai, aur usse kaunsa conserved quantity milti hai?

Recall Solution

Kya dhundna hai: wo coordinate jiska symbol mein appear na kare — sirf uski velocity ho. scan karo: hum dekhte hain , , — lekin koi bare nahi. To cyclic hai. Iska matlab kyun important hai: ke liye Euler–Lagrange kuch yun likhta hai Conserved quantity conjugate momentum hai Ye bead ki angular momentum hai. Physical symmetry: poore system ko kisi bhi angle se rotate karne par unchanged rehta hai (table ki koi preferred direction nahi hai).

Exercise 1.2 — Symmetry → law matchup

Har symmetry ke liye, conserved quantity ka naam batao: (a) clock ka zero shift karo, ; (b) har particle ko same vector se shift karo, ; (c) sab kuch ke around se rotate karo.

Recall Solution

(a) Time-translation invariance ( mein koi explicit nahi) → energy conserved. (b) Space-translation invariance → total linear momentum conserved. (c) Rotation invariance → total angular momentum conserved. Pattern ye hai: ek continuous knob mein "doesn't-matter" hona ek number ko freeze kar deta hai.


Level 2 — Application

Exercise 2.1 — Rotation par Noether crank ghoomao

Ek plane mein free particle, . Infinitesimal rotation apply karo. Confirm karo aur Noether charge compute karo.

Recall Solution

Step 1 — transformation velocities ke saath KIYA karta hai. Shifts ko time mein differentiate karo: . Step 2 — invariance check (WHY ). Step 3 — charge banao. To rotation ↔ , bilkul waisa hi jैसा parent §5 ne promise kiya tha.

Neeche diya figure padho taaki geometrically samjho WHY hai. Kala arrow vector hai; lal arrow dikhata hai rotation use kahan bhejti hai. Notice karo ki lal push kale arrow ke perpendicular hai (unka dot product hai). Ek vector ke right angles par push karna use bina stretch kiye rotate karta hai — isliye length freeze ho jaati hai, aur exactly isliye kinetic energy (jo us velocity vector ki length se bani hai) change nahi hoti. Ye perpendicular-push picture "rotation is a symmetry" ka geometric heart hai, aur jo conserved charge ye produce karta hai wo hai.

Figure — Noether's theorem — symmetry ↔ conservation law

Exercise 2.2 — Central-force energy aur angular momentum

Ek planet gravity ke under move kar raha hai, . Do conserved quantities likho aur , radius ke circular orbit ke liye unki numerical value nikalo.

Recall Solution

Angular momentum (cyclic se, jaise Ex 1.1 mein): . Energy (koi explicit nahi): . Circular orbit par , aur forces balance karne se , to , .

  • .
  • . To aur (bound orbit, isliye ).

Level 3 — Analysis

Exercise 3.1 — Energy conserved kab NAHI hoti?

Ek particle ek aisi potential mein hai jo slowly change ho rahi hai: jahan . Kya energy function conserved hai? ki direct computation se prove karo.

Recall Solution

Pehle master identity derive karo — ise sirf quote mat karo. se shuru karo jahan , aur time mein product rule aur chain rule use karke differentiate karo: Ab ko chain rule se expand karo (yaad raho depend karta hai , , aur explicitly par): Ise substitute karo: Bracket Euler–Lagrange se vanish ho jaata hai (). Jo bachta hai wo hai To energy sirf ke explicit time dependence se change hoti hai — ye precise Noether statement hai "time-translation symmetry ⇒ energy conserved." Yahan apply karo. Sirf potential mein hai: , to Energy rate se leak ho rahi hai: tum knob ghumaa ke system par kaam kar rahe ho. Symmetry broken → charge not conserved, bilkul waisa hi jaisa Noether ka converse warn karta hai.

Exercise 3.2 — Ek symmetry jo ko total derivative se change karti hai

Free particle ke liye, ek Galilean boost consider karo (har point ko time ke saath ek small constant velocity se aage push kiya jaata hai). Dikhao ki kisi ke liye, aur corrected conserved charge nikalo.

Recall Solution

Step 1 — velocity shift. . Step 2 — vary karo. . To ye ke saath total time derivative hai. Action abhi bhi invariant hai (boundary term), isliye Noether abhi bhi apply hota hai — lekin correction ke saath. Step 3 — corrected charge. Check karo ki ye constant hai: kyunki free particle mein hota hai. ✓ Physically hai, initial position encode karta hai — Galilean boosts ka conserved charge. Ye wahi case hai jo parent ne flag kiya tha: lekin abhi bhi ek law deta hai.


Level 4 — Synthesis

Exercise 4.1 — Do particles, relative coordinate, aur total momentum

Do particles sirf apne separation par depend karne wali potential se interact karte hain: Dikhao ki translation invariance () total momentum conserve karti hai, aur ke saath velocities ke liye numerically verify karo ki fixed hai jabki ek individual momentum zaroor nahi.

Recall Solution

WHY translation rok nahi sakti: depend karta hai par; ke under difference unchanged rehta hai, to , aur kinetic terms sirf velocities dekhte hain. Isliye . Noether charge: lo: — ek fixed number, bhaley hi aur force ke through change ho sakein. Moral: center-of-mass coordinate cyclic hai; relative coordinate saari interaction carry karta hai.

Exercise 4.2 — Time-shift charge se energy banana

Ek 1-D particle ke liye, time shift ke liye parent ka prescription use karo aur boundary correction ke saath energy reconstruct karo, aur ise ke liye evaluate karo.

Recall Solution

Step 1 — time shift ke liye corrected charge: Ye exactly hai. To "clock shift karo" ↔ energy, cleanly derived, assumed nahi. Step 2 — number: .


Level 5 — Mastery

Exercise 5.1 — Runge–Lenz vector as a hidden symmetry

Kepler problem mein, energy aur angular momentum ke alawa, ek extra conserved vector hai — Laplace–Runge–Lenz vector Newton's law aur use karke verify karo. (Ye ek aisi symmetry correspond karta hai jo simple point transformation nahi hai — deeper Noether world ka ek hint.)

Recall Solution

Step 1 — differentiate karo, is baat ka use karke ki constant hai. Step 2 — plane-polar unit vectors set up karo. Motion ek plane mein hai; (radial) aur (tangential) use karo, jahan . Unke time derivatives standard results hain aur . Angular momentum hai . Step 3 — pehla term explicitly expand karo (koi black box nahi). aur insert karo: Ab right-handed relation use karo (kyunki ). Isliye Step 4 — doosra term expand karo. Step 5 — combine aur cancel karo. Saari -dependence cancel ho gayi kyunki dono terms ne same -vector produce kiya — ye potential ka special algebra hai. Meaning: orbit ke major axis ke along point karta hai length (eccentricity ) ke saath; uski constancy isliye hai ki Kepler ellipses precess nahi karti. Associated symmetry 4 dimensions mein ek rotation group mein rehti hai — dekho Symmetry Groups & Lie Algebras.

Exercise 5.2 — Free-particle action ki scaling symmetry

Free particle scaling ke under invariant hai. Dikhao ki action integral strictly invariant hai (overall factor exactly hai), phir ise concrete path par interval ke liye confirm karo.

Recall Solution

Step 1 — har ingredient kaise scale karta hai. aur ke under, velocity ek ratio hai: Time measure scale hota hai . Step 2 — action assemble karo. Velocity se factor aur measure se factor exactly cancel ho jaate hain — action strictly invariant hai. Ye action ki genuine symmetry hai. Step 3 — concrete numerical check (step by step reconciled). lo original path ke liye: Ab ke saath scaling apply karo. Transformed path hai jo scaled time par express ki gayi; eliminate karne par milta hai, yaani nayi velocity hai (Step 1 se match karta hai), aur naya interval hai. Scaled action directly compute karo: — shrunken velocity-squared () exactly four-times-longer time interval () se compensate ho jaati hai. Invariance real numbers par demonstrate ki gayi, sirf symbols par nahi.


Recall Quick self-test (cloze)

Wo coordinate jo se missing ho use ::: cyclic (ignorable) kehte hain, aur uska conjugate momentum conserved hota hai. Energy exactly tab conserved hoti hai jab ka ::: time par koi explicit dependence na ho. Symmetry ke saath ke liye Noether charge hai ::: . Rotation invariance ::: angular momentum conserve karti hai.

Back to the parent topic · related: Conservation of Energy, Conservation of Momentum, Angular Momentum, Hamiltonian Mechanics.