Bertrand's and Earnshaw's theorems contradiction

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Discussion Overview

The discussion revolves around the apparent contradiction between Bertrand's theorem and Earnshaw's theorem, particularly in the context of gravitational forces and their implications for stability in orbits versus static configurations. Participants explore the nature of stability in dynamic versus static systems, focusing on the characteristics of 1/r potentials.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants note that Bertrand's theorem allows for stable orbits under gravitational forces, while Earnshaw's theorem suggests that static configurations cannot achieve stability.
  • Earnshaw's theorem is described as applying to static situations where pointlike particles do not have stable points in an unoccupied region due to the absence of minima or maxima in the potential.
  • Others argue that the dynamics introduced by angular momentum in Bertrand's theorem create effective potentials that can lead to stability, which is absent in the static case described by Earnshaw's theorem.
  • One participant emphasizes that for Earnshaw's theorem to contradict Bertrand's theorem, all involved particles must remain static, highlighting the limitations of Earnshaw's theorem to point masses or charges.
  • There is a discussion about the implications of local extrema in electrostatic configurations, questioning the equilibrium of charges in specific arrangements and the calculation of potential using superposition.

Areas of Agreement / Disagreement

Participants express differing views on the implications of Earnshaw's theorem and Bertrand's theorem, with no consensus reached on how these theorems interact or resolve the apparent contradiction. The discussion remains unresolved regarding the implications of static versus dynamic systems.

Contextual Notes

Limitations include the dependence on definitions of stability and equilibrium, as well as the unresolved nature of how dynamic effects alter the conclusions drawn from Earnshaw's theorem.

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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