How Does a Canonical Transformation Relate to Hamilton's Equations of Motion?

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Homework Help Overview

The discussion revolves around canonical transformations in the context of Hamiltonian mechanics, specifically focusing on a generating function and its implications for Hamilton's equations of motion.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants explore the explicit form of the canonical transformation and question the validity of using the Hamiltonian as the generating function. There is discussion about the transformation equations and the implications of small parameters in the context of Hamilton's equations.

Discussion Status

The conversation is ongoing, with participants clarifying the transformation relations and discussing the conditions under which the Hamiltonian can be used as the generating function. Some guidance has been provided regarding the choice of generating functions and their relationship to time evolution in Hamiltonian mechanics.

Contextual Notes

Participants note the importance of neglecting higher-order terms and the smoothness of functions involved in the transformation. There is also mention of the preservation of Poisson brackets in the context of the transformation.

Logarythmic
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Homework Statement



Consider a canonical transformation with generating function

[tex]F_2 (q,P) = qP + \epsilon G_2 (q,P)[/tex],

where [tex]\epsilon[/tex] is a small parameter.
Write down the explicit form of the transformation. Neglecting terms of order [tex]\epsilon^2[/tex] and higher,find a relation between this transformation and Hamilton's equations of motion, by setting [tex]G_2=H[/tex] (why is this allowed?) and [tex]\epsilon = dt[/tex].2. The attempt at a solution

I think the transformation equations are

[tex]\delta p = P - p = -\epsilon \frac{\partial G_2}{\partial q}[/tex]

and

[tex]\delta q =Q-q=\epsilon \frac{\partial G_2}{\partial q}[/tex]
vanesch said:
I guess there's a typo here:
[tex]\delta q =Q-q=\epsilon \frac{\partial G_2}{\partial P}[/tex]

but how can I solve the last part? Can I just say that with the use of H and dt the equations can be written as

[tex]\dot{p}=-\frac{\partial H}{\partial q}[/tex]

and

[tex]\dot{q}=\frac{\partial H}{\partial P}[/tex]

which are the Hamiltonian equations of motion? And why is this allowed?

vanesch said:
The idea is that we work in first order in [tex]\epsilon[/tex], and that you can hence replace everywhere [tex]P[/tex] by [tex]p[/tex] as the difference will introduce only second-order errrors.
 
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Ooops ! :redface: :redface:

I'm terribly sorry, instead of replying, I erroneously edited your post ! :bugeye:
 
Yes it should be a P, not a q. I get the relations

[tex]Q = q + \delta q[/tex]

and

[tex]P = p + \delta p[/tex]

but why is it allowed to use G = H?
 
Logarythmic said:
Yes it should be a P, not a q. I get the relations

[tex]Q = q + \delta q[/tex]

and

[tex]P = p + \delta p[/tex]

but why is it allowed to use G = H?

You have the choice ! Every function G(q,P) (which is smooth enough) will generate a canonical transformation. So you may just as well use H(q,P), and then - that's the whole point - the transformation equations from (q,p) into (Q,P) give you simply the genuine time evolution where epsilon is the small time step. For an arbitrary G that isn't the case of course, you've just transformed your coordinates (q,p) in some other (Q,P). But for G = H, you've transformed the coordinates (q,p) in what they will be, a small moment later !
The reason for that is that your transformation equations you've found for an arbitrary G are what they are, and become the Hamilton equations of motion when you pick G to be equal to H.

Now, strictly speaking we should write H(q,P) instead of H(q,p), but we can replace the P by p here, because they are only a small amount different.
 
and it also preserve the fundamental poisson brackets...

its just a quick calcolus {Q,P}
 

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