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
Key Equations
Angular Momentum from Rotational Symmetry
A particle moves in a central potential . Show that angular momentum is conserved using cyclic coordinates.
In polar coordinates: , .
is cyclic (), so the conjugate momentum is conserved:
is the angular momentum — conserved because has rotational () symmetry.
Exercises
7 problemsA particle in 2D has (no in ). Which momentum is conserved?
A particle ( kg) moves in a circle of radius m at rad/s. Find the conserved angular momentum (in kg·m²/s).
A free particle with has kg·m/s at . What is at s?
Unlock Exercise 3
Subscribe to PhysWeb Pro to access all exercises and track your progress.
Upgrade to Pro →A spring-mass system has with no explicit time dependence. The conserved energy is . For kg, N/m, , m, find (in J).
Unlock Exercise 4
Subscribe to PhysWeb Pro to access all exercises and track your progress.
Upgrade to Pro →A particle moves in a potential (central force). Using angular momentum kg·m²/s and m and kg, find (in rad/s).
Unlock Exercise 5
Subscribe to PhysWeb Pro to access all exercises and track your progress.
Upgrade to Pro →Under time translation invariance, the Noether charge is energy. A pendulum at angle with rad/s, kg, m. Find (in J).
Unlock Exercise 6
Subscribe to PhysWeb Pro to access all exercises and track your progress.
Upgrade to Pro →For a symmetric top with , there are three conserved quantities. One is (space-fixed). For kg·m², rad/s, find (in kg·m²/s).
Unlock Exercise 7
Subscribe to PhysWeb Pro to access all exercises and track your progress.
Upgrade to Pro →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.