Bertrand's and Earnshaw's theorems contradiction

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SUMMARY

Bertrand's and Earnshaw's theorems present a fundamental contradiction in classical mechanics regarding stability in gravitational systems. Earnshaw's theorem asserts that static configurations of point masses under a 1/r potential lack stable equilibrium points, while Bertrand's theorem indicates that certain potentials can yield stable orbits. The discussion clarifies that the stability in Bertrand's theorem arises from dynamic conditions, specifically angular momentum, which is absent in the static scenarios described by Earnshaw's theorem. Thus, the introduction of dynamics allows for stable orbits, contrasting with the static limitations of Earnshaw's theorem.

PREREQUISITES
  • Understanding of classical mechanics principles, particularly gravitational forces.
  • Familiarity with Earnshaw's theorem and its implications on static configurations.
  • Knowledge of Bertrand's theorem and its application to orbital stability.
  • Basic concepts of angular momentum and its role in dynamic systems.
NEXT STEPS
  • Study the implications of Earnshaw's theorem in electrostatics and its limitations.
  • Explore the mathematical derivation of Bertrand's theorem and its applications in orbital mechanics.
  • Investigate the role of angular momentum in stabilizing orbits in gravitational systems.
  • Read Griffiths' "Introduction to Electrodynamics" alongside Purcell's "Electricity and Magnetism" for deeper insights into electrostatic equilibrium.
USEFUL FOR

Students and professionals in physics, particularly those focusing on classical mechanics, gravitational systems, and electrostatics, will benefit from this discussion. It is also valuable for educators seeking to clarify the distinctions between static and dynamic stability in physical systems.

Trifis
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I think the title is self-explanatory. The first theorem states that gravitational forces (1/r potentials in general) are able to produce stable orbits, whereas the second excludes stability! Can somebody help me to clear this out?
 
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Trifis said:
I think the title is self-explanatory. The first theorem states that gravitational forces (1/r potentials in general) are able to produce stable orbits, whereas the second excludes stability! Can somebody help me to clear this out?

Earnshaw's theorem talks about static configurations.
 
A.T. said:
Earnshaw's theorem talks about static configurations.

In Earnshaw's theorem there is not a minimum for the potential. In Bertrand's theorem close orbits are excecuted around a point of stability (like the oscillation).

I need something more elaborate please.
 
static = no movement
orbits = movement
 
When an orbit has a stable point then the particle can as well stay at this point point forever without losing its dynamical stability.
 
Trifis said:
When an orbit has a stable point then the particle can as well stay at this point point forever without losing its dynamical stability.
To contradict Earnshaw all involved particles have to remain static, not just a single one. It applies only to point masses/charges which cannot occupy the same point in space.
 
Specifically, Earnshaw's Theorem states that in a static situation for pointlike particles, a 1/r potential does not have any maxima or minina (stable points) in an unoccupied region, since the sources themselves occupy space. When dynamics are added into the mix, there is an effective potential from the angular component which pushes away from the source and falls off as 1/r2. For example, with gravity, the potential is a combination of angular repulsion (\frac{1}{2}\frac{mh^2}{r^2}) and gravitational attraction (\frac{GMm}{r}), which gives a total potential of U=\frac{1}{2}\frac{mh^2}{r^2} - \frac{GMm}{r}, and a minimum at r=\frac{h^2}{GM}.

(h is angular momentum per mass)
 
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Ok therefore it is the extra angular movement which provides the stability of the ORBIT and cannot be found in the static case.

On second thought it can be said that since Earnshaw applies only on 1/r forces (my oscillation argumantion was thereby false) there weren't any equilibrium states Kepler-like orbits first place to debate on in the first place ...
 
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so since Laplace says that there can be no local extrema then a charge at the center of a cube with charges at the 6 corners cannot be in electrostatic equilibrium since then U would be at a minimum? if the potential is like a saddle point for the center charge in a cube then in the xz plane it is at a max and yz it is at a minimum at the same time? (do you calculate the potential by superposition to find the saddle point?)
how do you know that the charge leaks out of every face of the cube?

Griffiths doesn't say that much about this, is it better to read Purcell and Wave Electromagnetics at the same time?
 
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