In plain words
Write kinetic energy minus potential energy in coordinates that suit the constraints, and the equations follow mechanically. Constraint forces never appear, which is the entire reason for the method.
The recipe
- Choose generalised coordinates degrees of freedom = 3N − constraints).
- Write T (kinetic) and V (potential) in terms of q, q̇.
- L = T − V.
- Euler–Lagrange: d/dṫ.
Conservation laws (Noether)
| Symmetry | Conserved |
|---|---|
| L independent of cyclic) | ̇ |
| L independent of t | energy ̇ |
| translation invariance | linear momentum |
| rotation invariance | angular momentum |
Standard systems
| System | L |
|---|---|
| Simple pendulum, length | ½̇ mg |
| Particle in a central field | ½m(ṙ̇ cyclic ⇒ angular momentum mṙ conserved |
| Bead on a rotating wire | ½m(ṙ |
| Atwood machine | ½ẋgx |
| Cycloid | T = mȧ mga |
For the cycloid: d/dt[2mȧ] = mȧ mga gives ̈ ̇ — note the mass cancels.
Constraints
- Holonomic f(q, t) = 0: eliminate a coordinate, or use a multiplier which is the constraint force).
- Non-holonomic constraints (e.g. rolling without slipping) need multipliers; they cannot be eliminated.
Key takeaways
- Count degrees of freedom first; that is how many equations you will write.
- Cyclic coordinate ⇒ conserved conjugate momentum, instantly.
- Mass often cancels for constrained gravity problems — a useful sanity check.