Answer
Be aware that there exist various definitions of a canonical transformation (CT) in the literature:
Firstly, Refs. 1 and 2 define a CT as a transformation1 (qi,pi) ↦ (Qi(q,p,t),Pi(q,p,t))
[together with a choice of a Hamiltonian H(q,p,t) and a Kamiltonian K(Q,P,t); and where t is the time parameter] that satisfies (n∑i=1pidqi−Hdt)−(n∑i=1PidQi−Kdt) = dFfor some generating function F.Secondly, Wikipedia (October 2015) calls a transformation (1) [together with a choice of H(q,p,t) and K(Q,P,t)] a CT if it transforms the Hamilton's eqs. into Kamilton's eqs. This is called a canonoid transformation in Ref. 3.
Thirdly, Ref. 3 calls a transformation (1) a CT if ∀H(q,p,t)∃K(Q,P,t) such that the transformation (1) transforms the Hamilton's eqs. into Kamilton's eqs.
Fourthly, some authors (e.g. Ref. 4) use the word CT as just another word for a symplectomorphism f:M→M [which may depend on a parameter t] on a symplectic manifold (M,ω), i.e. f∗ω=ω.
Here ω is the symplectic two-form, which in local Darboux/canonical coordinates reads ω=∑ni=1dpi∧dqi.Fifthly, Ref. 1 defines an extended canonical transformation (ECT) as a transformation (1) [together with a choice of H(q,p,t) and K(Q,P,t)] that satisfies λ(n∑i=1pidqi−Hdt)−(n∑i=1PidQi−Kdt) = dF
for some parameter λ≠0 and for some generating function F.
Now let us discuss some of the relationships between the above five different definitions.
The first definition is an ECT with λ=1. An ECT satisfies the second definition, but not necessarily vice-versa, cf. e.g. this and this Phys.SE post.
The first definition is a symplectomorphism (by forgetting about H and K). Conversely, there may be global obstructions for a symplectomorphism to satisfy the first definition. However, a symplectomorphism sufficiently close to the identity map and defined within a single Darboux coordinate chart does satisfy the parts of the first definition that do not concern H and K. See also e.g. my Phys.SE answer here.
An ECT is not necessarily a symplectomorphism. Counterexample: Q = λq,P=pK = λH,F = 0,
where λ∉{0,1} is a constant different from zero and one, so that the Poisson bracket is not preserved {Q,P}PB = λ{q,p}PB ≠ {q,p}PB = 1.
References:
H. Goldstein, Classical Mechanics; Chapter 9. See text under eq. (9.11).
L.D. Landau and E.M. Lifshitz, Mechanics; §45. See text between eqs. (45.5-6).
J.V. Jose & E.J. Saletan, Classical Dynamics: A Contemporary Approach, 1998; Subsection 5.3.1, p. 233.
V.I. Arnold, Mathematical Methods of Classical Mechanics, 2nd eds., 1989; See §44E and footnote 76 on p. 241.
--
1 Although Ref. 1 and Ref. 2 don't bother to mention this explicitly, it is implicitly assumed that the map (1) is a sufficiently smooth bijection, e.g., a diffeomorphism [which depends smoothly on the time parameter t]. Similar smoothness conditions are implicitly assumed about H, K, and F.
No comments:
Post a Comment