I was going through my professor's notes about Canonical transformations. He states that a canonical transformation from (q,p) to (Q,P) is one that if which the original coordinates obey Hamilton's canonical equations then so do the transformed coordinates, albeit for a different Hamiltonian. He then considers, as an example the Hamiltonian
H=12p2,
with a transformation:
Q=q, P=√p−√q.
The notes state that this transformation is locally canonical with respect to H, and that in the transformed coordinates the new Hamiltonian is:
K=13(P+√Q)3.
I don't understand how we know that this is locally canonical, or what it really even means to be locally canonical. Also, where do we get K from? Considering that the inverse transformation would be:
q=Q, p=(P+√Q)2,
Why isn't the new Hamiltonian this:
K=12(P+√Q)4,
where all I've done is plug the inverted transformation into the original Hamiltonian?
I'm a bit confused by all this. Would appreciate any help.
Answer
The original coordinates satisfy the equations of motion when the integral of p˙q−H(p,q) is minimized, and the new coordinates satisfy the equations of motion when the integral of P˙Q−K(P,Q) is minimized. There is no requirement that H and K be numerically equal.
The transformation is canonical if the Poisson bracket remains invariant.
The EOMs are
˙p=0
˙q=p
and from the new Hamiltonian, we get
˙P=−(P+√Q)212√Q=−p2√q=ddt(√p−√q)
˙Q=(P+√Q)2=˙q
thus the equations of motion are numerically equal.
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