Finding Conserved Quantities for Analytical Mechanics Exam Questions

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SUMMARY

This discussion focuses on finding conserved quantities from three Hamiltonians in analytical mechanics, specifically in the context of a graduate course based on Arnold's book. The Hamiltonians presented are: (1) a general function of coordinates and momenta, (2) a nested function of coordinates and momenta, and (3) a sum of squared velocities plus a potential dependent on squared coordinates. The participants conclude that while the first and second Hamiltonians primarily conserve the Hamiltonian itself, the third Hamiltonian allows for the conservation of orbital angular momentum when substituting velocities with momenta.

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  • Understanding of Hamiltonian mechanics
  • Familiarity with Hamilton-Jacobi theory
  • Knowledge of generalized coordinates and momenta
  • Basic concepts of conservation laws in physics
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Graduate students in physics, particularly those studying analytical mechanics, as well as educators and researchers looking to deepen their understanding of Hamiltonian systems and conserved quantities.

JorisL
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Hi all,

I am preparing for my "second chance exam" in analytical mechanics.
It is a graduate course i.e. based on geometry. (Our course notes are roughly based on Arnold's book).

I was able to find some old exam questions and one of those has me stumped, completely.
The question gives 3 general Hamiltonians, no details whatsoever and asks to find as many conserved quantities as possible.
*Warning* The second one really hurts my brain.

##\mathcal{H}_1 = \mathcal{H}_1\left( f_1(q^1,p_1), \ldots, f_N(q^N,p_N)\right)##
(1)​
##\mathcal{H}_2 = g_N( g_{N-1}(\ldots g_2(g_1(q^1,p_1),q^2,p_2)\ldots ,q^{N-1},p_{N-1}),q^N,p_N)##
(2)​
##\mathcal{H}_3 = \sum_{i=1}^N \left(\dot{q}^i(t)\right)^2+V\left( \sum_{i=1}^N \left(q^i(t)\right)^2\right)##
(3)​

Hamiltonian (1) isn't terribly complicated at first sight, however without further information about the functions ##f_i## I'm not sure what I can deduce. As far as I can tell, I cannot claim anything to be conserved except the Hamiltonian itself. (Which is easy to see because there is no explicit time-dependence so ##dH_1/dt = \{H,H\} = 0##)

The second Hamiltonian, I don't even understand why the instructor would do such a thing to us. It is horrible and unless someone knows a neat trick or has some cool information about this, I suggest we all pretend that doesn't exist. My guess is that only the conservation of the Hamiltonian follows from this, once again.

Definition (3) seems like a nice expression. But there is a strange thing going on here, we have ##\dot{q}^i## in there but no generalized moments.
I could state that the moments are cyclic but that would be a trap I think.
This Hamiltonian hasn't been "fully transformed" from the Lagrangian.
I believe the "real" Hamiltonian might be invariant under rotations in the coordinates ##\vec{q}##.
My (very short and vague) motivation is that the positions appear squared only, no mixing either.

So does anybody have some general remarks/ideas/resources to help me with this kind of stuff?

-Joris
 
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So I made some 'progress', the first 2 are definitely based on the use of (time independent) Hamilton-Jacobi.
Even though this is not much to go by, I suppose it might help some people with the same problems.

I might come back to this later and go into some detail if I can find the time.
 
JorisL said:
Hi all,

##\mathcal{H}_1 = \mathcal{H}_1\left( f_1(q^1,p_1), \ldots, f_N(q^N,p_N)\right)##
(1)​

Calculate
\dot{ f }_{ i } = \{ H , f_{ i } \} = \sum_{ n = 1 }^{ N } \left( \frac{ \partial H }{ \partial p^{ n } } \frac{ \partial f_{ i } }{ \partial q_{ n } } - \frac{ \partial H }{ \partial q_{ n } } \frac{ \partial f_{ i } }{ \partial p^{ n } } \right) .
Then, use
\frac{ \partial f_{ i } }{ \partial q^{ n } } = \frac{ \partial f_{ i } }{ \partial p^{ n } } = 0 , \ \ \mbox{ for all } \ n \neq i .

##\mathcal{H}_2 = g_N( g_{N-1}(\ldots g_2(g_1(q^1,p_1),q^2,p_2)\ldots ,q^{N-1},p_{N-1}),q^N,p_N)##
(2)​

Try to calculate
\dot{ g }_{ 1 } = \{ H , g_{ 1 } \} .

##\mathcal{H}_3 = \sum_{i=1}^N \left(\dot{q}^i(t)\right)^2+V\left( \sum_{i=1}^N \left(q^i(t)\right)^2\right)##
(3)​

Nothing prevent you from setting \dot{ q }^{ i } = p^{ i }. Then, you can show that the orbital angular momentum is conserved
\frac{ d L_{ i } }{ d t } = \{ H , \epsilon_{ i j k } q^{ j } p^{ k } \} = 0 .
 

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