Regular vs stable orbits in spherically symmetric potentials

In summary, classical mechanics can be summarized as follows: canonical transformations, angle-action variables, invariant tori in phase space, and quasiperiodic motion in Cartesian coordinates. If there are less than 3 integrals of motion, then some (if not all) orbits are chaotic. If a potential has a local maximum, then the law of physics is unpredictable about what will happen next.
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ZelchJ
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TL;DR Summary
Are chaotic orbits possible in central force fields?
I am struggling with Hamiltonian formulation of classical mechanics. I think I have grasped the idea of canonical transformations, including the idea of angle-action variables and invariant tori in phase space. Still, few points seem to elude my understanding...

Let's talk about a particle moving in a 3D potential, so its phase-space is 6D. If I understand it right, if this potential has at least 3 integrals of motion, then the system is said to be integrable, and the particle's orbit in phase space is confined to the surface of a three-dimensional torus, and its motion in Cartesian coordinates is quasiperiodic. If, on the other hand, there are less than 3 integrals of motion, then some (if not all) orbits are chaotic (irregular).

Now, any static spherically symmetric potential has four integrals of motion - energy and three components of the angular momentum. Is this enough to state that chaotic orbits are impossible in static spherically symmetric potentials? In other words, that all orbits are regular in any static central force field?

If yes, then how does this match with the fact that unstable orbits are possible in central force field? (e.g., https://physics.stackexchange.com/questions/183726/what-makes-an-orbit-stable-or-unstable). In my understanding, regular orbits are basically a synonym for stable orbits: because regular orbits are not chaotic, two near-by orbits on two near-by tori don't ever diverge as chaotic orbits do. Isn't it the same as stability?
 
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ZelchJ said:
If yes, then how does this match with the fact that unstable orbits are possible in central force field? (e.g., https://physics.stackexchange.com/questions/183726/what-makes-an-orbit-stable-or-unstable). In my understanding, regular orbits are basically a synonym for stable orbits: because regular orbits are not chaotic, two near-by orbits on two near-by tori don't ever diverge as chaotic orbits do. Isn't it the same as stability?
Stability here means orbits that are closed, i.e., that do not converge (diverge) to 0 (infinity).
 
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Suppose that one uses a potential that has a local maximum. Further, assume that the potential is shaped so that a particle can approach the point of the maximum and arrive within finite time with zero remaining kinetic energy. Then the laws of physics are impredictive about what happens next. The particle can stay there indefinitely. Or it can depart at any time in either direction.

If my memory does not betray me, the function ##f(x) = -e^{-1/x^2}## for x not equal to zero and ##f(x) = 0## for ##x = 0## qualifies as such a potential. One could tweak it to put a potential barrier at the ends so that escape is made impossible.
 
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Of course, for this potential the analysis in terms of a power series around ##x=0## must fail, because there is an essential singularity when considered as a complex function, and thus there's no power series or, more precisely, the power series has convergence radius 0.
 
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Thank you all for the replies. But I still can't see how this relates to the notion of regular orbits in phase-space of Hamiltonian formulation.
 

FAQ: Regular vs stable orbits in spherically symmetric potentials

What is the difference between regular and stable orbits in spherically symmetric potentials?

Regular orbits refer to orbits that are predictable and follow a smooth, repeating path, often described by closed curves in phase space. Stable orbits, on the other hand, are those that remain bounded and do not diverge over time when subjected to small perturbations. In a spherically symmetric potential, regular orbits are typically also stable, but not all stable orbits are necessarily regular.

How does the concept of spherical symmetry affect the nature of orbits?

Spherical symmetry implies that the potential depends only on the distance from the center and not on the direction. This symmetry simplifies the equations of motion and leads to the conservation of angular momentum. Consequently, the orbits lie in a plane, and the effective potential can be analyzed in one dimension, making it easier to identify regular and stable orbits.

Can you provide examples of spherically symmetric potentials and their typical orbits?

Common examples of spherically symmetric potentials include the gravitational potential of a point mass (Newtonian potential) and the harmonic oscillator potential. In the Newtonian potential, typical orbits are elliptical (Keplerian orbits), which are both regular and stable. In the harmonic oscillator potential, orbits are closed ellipses centered on the origin, and they are also regular and stable.

What role does angular momentum play in determining the stability of orbits?

Angular momentum plays a crucial role in the stability of orbits in spherically symmetric potentials. It acts as a centrifugal barrier, preventing the orbiting object from falling into the center. Higher angular momentum generally leads to more stable orbits because the effective potential has a stronger repulsive component at small radii, which stabilizes the motion against perturbations.

How do perturbations affect regular and stable orbits in spherically symmetric potentials?

Perturbations can affect regular and stable orbits differently. For regular orbits, small perturbations typically result in slight deviations that do not alter the overall predictable and repeating nature of the orbit. For stable orbits, as long as the perturbations are small, the orbit will remain bounded and not diverge over time. However, large perturbations can destabilize an orbit, potentially leading to chaotic behavior or escape from the potential well.

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