2.1.9 · D4Analytical Mechanics

Exercises — Noether's theorem — symmetry ↔ conservation law

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The two tools you will reuse constantly:


Level 1 — Recognition

Exercise 1.1 — Spot the cyclic coordinate

A bead slides on a frictionless horizontal table, described in polar coordinates: Which coordinate is cyclic (ignorable), and what conserved quantity does that give?

Recall Solution

WHAT to look for: a coordinate whose symbol does not appear in — only its velocity does. Scan : we see , , — but no bare . So is cyclic. WHY that matters: Euler–Lagrange for reads The conserved quantity is the conjugate momentum This is the angular momentum of the bead. The physical symmetry: rotating the whole system by any angle leaves unchanged (the table has no preferred direction).

Exercise 1.2 — Symmetry → law matchup

For each symmetry, name the conserved quantity: (a) shift the clock's zero, ; (b) shift every particle by the same vector, ; (c) rotate everything about by .

Recall Solution

(a) Time-translation invariance ( has no explicit ) → energy conserved. (b) Space-translation invariance → total linear momentum conserved. (c) Rotation invariance → total angular momentum conserved. The pattern: a "doesn't-matter" in a continuous knob freezes one number.


Level 2 — Application

Exercise 2.1 — Turn the Noether crank on a rotation

Free particle in a plane, . Apply the infinitesimal rotation . Confirm and compute the Noether charge .

Recall Solution

Step 1 — WHAT the transformation does to velocities. Differentiate the shifts in time: . Step 2 — check invariance (WHY ). Step 3 — build the charge. So rotation ↔ , exactly as the parent §5 promised.

Read the figure below to see WHY geometrically. The black arrow is the vector ; the red arrow is where the rotation sends it. Notice the red push is perpendicular to the black arrow (their dot product is ). A push at right angles to a vector rotates it without stretching it — so the length is frozen, which is exactly why the kinetic energy (built from that length, for the velocity vector) does not change. That perpendicular-push picture is the geometric heart of "rotation is a symmetry," and the conserved charge it produces is .

Figure — Noether's theorem — symmetry ↔ conservation law

Exercise 2.2 — Central-force energy and angular momentum

A planet moves under gravity, . Write the two conserved quantities and their numerical form for , on a circular orbit of radius .

Recall Solution

Angular momentum (from cyclic , as in Ex 1.1): . Energy (no explicit ): . On a circular orbit , and balancing forces gives , so , .

  • .
  • . So and (bound orbit, hence ).

Level 3 — Analysis

Exercise 3.1 — When is energy NOT conserved?

A particle sits in a potential that is being slowly cranked: with . Is the energy function conserved? Prove it with a direct computation of .

Recall Solution

First derive the master identity — don't just quote it. Start from with , and differentiate in time using the product rule and chain rule: Now expand by the chain rule (remember depends on , , and explicitly on ): Substitute this in: The bracket vanishes by Euler–Lagrange (). What survives is So energy changes only through the explicit time dependence of — that is the precise Noether statement "time-translation symmetry ⇒ energy conserved." Apply it here. Only the potential carries : , so Energy leaks in at rate : you are doing work on the system by turning the knob . Symmetry broken → charge not conserved, exactly as Noether's converse warns.

Exercise 3.2 — A symmetry that changes by a total derivative

For the free particle , consider a Galilean boost (every point gets pushed forward by a small constant velocity as time passes). Show for some , and find the corrected conserved charge .

Recall Solution

Step 1 — velocity shift. . Step 2 — vary . . So it is a total time derivative with . The action is still invariant (boundary term), so Noether still applies — but with the correction. Step 3 — corrected charge. Check it is constant: because a free particle has . ✓ Physically , encoding the initial position — the conserved charge of Galilean boosts. This is the case the parent flagged: but still gives a law.


Level 4 — Synthesis

Exercise 4.1 — Two particles, relative coordinate, and total momentum

Two particles interact through a potential depending only on their separation: Show that translation invariance () makes total momentum conserved, and verify numerically for with velocities that is fixed while an individual momentum need not be.

Recall Solution

WHY can't stop translation: depends on ; under the difference is unchanged, so , and kinetic terms only see velocities. Hence . Noether charge: Take : — a fixed number even though and can change through the force. The moral: the center-of-mass coordinate is cyclic; the relative coordinate carries all the interaction.

Exercise 4.2 — Building energy from the time-shift charge

For a 1-D particle , use (the parent's prescription for a time shift) with the boundary correction to reconstruct the energy , and evaluate it for .

Recall Solution

Step 1 — the corrected charge for a time shift: That is exactly . So "shift the clock" ↔ energy, cleanly derived, not assumed. Step 2 — number: .


Level 5 — Mastery

Exercise 5.1 — Runge–Lenz vector as a hidden symmetry

The Kepler problem has, beyond energy and angular momentum, an extra conserved vector — the Laplace–Runge–Lenz vector Verify using Newton's law and . (This corresponds to a symmetry that is not a simple point transformation — a hint of the deeper Noether world.)

Recall Solution

Step 1 — differentiate, using that is constant. Step 2 — set up plane-polar unit vectors. Motion is in a plane; use (radial) and (tangential), with . Their time derivatives are the standard results and . Angular momentum is . Step 3 — expand the first term explicitly (no black box). Insert and : Now use the right-handed relation (since ). Therefore Step 4 — expand the second term. Step 5 — combine and cancel. Every -dependence cancelled because the two terms produced the same -vector — that is the special algebra of the potential. Meaning: points along the orbit's major axis with length (eccentricity ); its constancy is why Kepler ellipses don't precess. The associated symmetry lives in a rotation group in 4 dimensions — see Symmetry Groups & Lie Algebras.

Exercise 5.2 — Scaling symmetry of the free-particle action

The free particle is invariant under the scaling . Show the action integral is strictly invariant (the overall factor is exactly ), then confirm it on the concrete path over an interval .

Recall Solution

Step 1 — how each ingredient scales. Under and , the velocity is a ratio: The time measure scales as . Step 2 — assemble the action. The factor from the velocity and from the measure cancel exactly — the action is strictly invariant. This is a genuine symmetry of the action. Step 3 — concrete numerical check (reconciled step by step). Take for the original path : Now apply the scaling with . The transformed path is expressed at scaled time ; eliminating gives , i.e. the new velocity is (matching Step 1), and the new interval is . Compute the scaled action directly: — the shrunken velocity-squared () is exactly compensated by the four-times-longer time interval (). The invariance is demonstrated on real numbers, not just symbols.


Recall Quick self-test (cloze)

A coordinate missing from is called ::: cyclic (ignorable), and its conjugate momentum is conserved. Energy is conserved exactly when has no explicit dependence on ::: time . The Noether charge for a symmetry with is ::: . Rotation invariance conserves ::: angular momentum .

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