Conservation laws
Classical mechanics has several well-known conservation laws. Here we
show how these laws can be derived using Lagrangian formalism.
For an system without external interactions, the Lagrangian cannot
depend on time.
dtdLL˙=i∑(∂qi∂Ldtdqi+∂q˙i∂Ldtdq˙i)=q˙i∂iL+q¨i∂˙iL=0.From the Euler-Lagrange equation we can substitute ∂iL
(dtd∂˙iL)q˙i+q¨i∂˙iL−L˙=dtd(q˙i∂˙iL−L)=0.Assuming L=21mq˙iq˙i−U(q), the conserved quantity is
mq˙iq˙i−(21mq˙iq˙i−U(q))=21mq˙iq˙i+U(q)=:E.So energy is conserved when there are no time-dependent interactions
(varying external potentials).
Another symmetry that follows from postulate 2 of classical mechanics
is spacial invariance. If a system is translated some small amount dx,
Abuse of notation
I’m using Einstein notation here, without caring about up/down indices.
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