← Classical Mechanics
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Symmetry & Conservation Laws

Emmy Noether's theorem is one of the deepest results in physics: every continuous symmetry of the action corresponds to a conserved quantity. Translational symmetry gives momentum conservation; rotational symmetry gives angular momentum conservation; time-translation symmetry gives energy conservation.

Key Concepts

Noether's Theorem
If the Lagrangian is invariant under a continuous one-parameter transformation qq+ϵδqq\to q+\epsilon\delta q, then Q=iLq˙iδqiQ=\sum_i\frac{\partial L}{\partial\dot q_i}\delta q_i is a constant of motion.
Cyclic Coordinate
A coordinate qiq_i that does not appear in LL (only q˙i\dot q_i does). The conjugate momentum pi=L/q˙ip_i=\partial L/\partial\dot q_i is then conserved. This is the simplest application of Noether's theorem.
Energy Conservation
If LL has no explicit time dependence (L/t=0\partial L/\partial t=0), the Hamiltonian H=ipiq˙iLH=\sum_i p_i\dot q_i-L is conserved. This is conservation of energy.
Discrete Symmetries
Parity (spatial reflection) and time reversal are discrete symmetries. Unlike continuous symmetries, they do not generate conserved quantities (Noether's theorem requires continuous transformations), but they impose constraints on allowed interactions.

Key Equations

Noether's conserved charge
Q=iLq˙iδqiQ = \sum_i \frac{\partial L}{\partial \dot{q}_i}\,\delta q_i
Conserved quantity associated with the symmetry transformation δqᵢ.
Energy (Jacobi integral)
E=iq˙iLq˙iLE = \sum_i \dot{q}_i \frac{\partial L}{\partial \dot{q}_i} - L
Conserved when ∂L/∂t = 0; equals T+V for natural systems.
Angular momentum
Lz=m(xy˙yx˙)=mr2ϕ˙L_z = m(x\dot{y} - y\dot{x}) = mr^2\dot{\phi}
Conserved due to rotational symmetry; conjugate to the cyclic angle φ.
Worked Example

Angular Momentum from Rotational Symmetry

Problem

A particle moves in a central potential V(r)V(r). Show that angular momentum is conserved using cyclic coordinates.

Solution

In polar coordinates: T=12m(r˙2+r2ϕ˙2)T=\frac{1}{2}m(\dot r^2+r^2\dot\phi^2), V=V(r)V=V(r).

L=12m(r˙2+r2ϕ˙2)V(r)L = \frac{1}{2}m(\dot r^2 + r^2\dot\phi^2) - V(r)

ϕ\phi is cyclic (L/ϕ=0\partial L/\partial\phi=0), so the conjugate momentum is conserved:

pϕ=Lϕ˙=mr2ϕ˙=l=constp_\phi = \frac{\partial L}{\partial\dot\phi} = mr^2\dot\phi = l = \text{const}

pϕ=lp_\phi=l is the angular momentum — conserved because LL has rotational (ϕ\phi) symmetry.

Answer l=mr2ϕ˙=l=mr^2\dot\phi= const; conservation follows from ϕ\phi being cyclic in LL.
Practice

Exercises

7 problems
1 of 7

A particle in 2D has L=12m(x˙2+y˙2)V(x)L=\frac{1}{2}m(\dot x^2+\dot y^2)-V(x) (no yy in VV). Which momentum is conserved?

(p_y = const)
2 of 7

A particle (m=2.0m=2.0 kg) moves in a circle of radius r=3.0r=3.0 m at ϕ˙=4.0\dot\phi=4.0 rad/s. Find the conserved angular momentum l=mr2ϕ˙l=mr^2\dot\phi (in kg·m²/s).

kg·m²/s
3 of 7

A free particle with L=12mx˙2L=\frac{1}{2}m\dot x^2 has px=5.0p_x=5.0 kg·m/s at t=0t=0. What is pxp_x at t=10t=10 s?

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4 of 7

A spring-mass system has L=12mx˙212kx2L=\frac{1}{2}m\dot x^2-\frac{1}{2}kx^2 with no explicit time dependence. The conserved energy is E=12mx˙2+12kx2E=\frac{1}{2}m\dot x^2+\frac{1}{2}kx^2. For m=1m=1 kg, k=4k=4 N/m, x˙=0\dot x=0, x=3x=3 m, find EE (in J).

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5 of 7

A particle moves in a potential V=V(r)V=V(r) (central force). Using angular momentum l=4.0l=4.0 kg·m²/s and r=2.0r=2.0 m and m=1.0m=1.0 kg, find ϕ˙\dot\phi (in rad/s).

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6 of 7

Under time translation invariance, the Noether charge is energy. A pendulum at angle θ=20°\theta=20° with θ˙=1.0\dot\theta=1.0 rad/s, m=0.5m=0.5 kg, l=1.0l=1.0 m. Find EE (in J).

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7 of 7

For a symmetric top with I1=I2I3I_1=I_2\ne I_3, there are three conserved quantities. One is LzL_z (space-fixed). For I3=0.10I_3=0.10 kg·m², ω3=20\omega_3=20 rad/s, find L3=I3ω3L_3=I_3\omega_3 (in kg·m²/s).

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Key Takeaways

  • Noether's theorem: every continuous symmetry → a conserved quantity. This is the deepest connection between symmetry and dynamics.
  • Cyclic coordinates give conserved momenta directly; explicit time independence gives conserved energy.
  • The three great conservation laws — energy, momentum, angular momentum — each follow from a spacetime symmetry.
  • Discrete symmetries (parity, time reversal) constrain interactions but do not produce conserved charges via Noether.