Particle oscillating around equilibrium radius

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SUMMARY

The discussion centers on the oscillatory motion of a particle of mass m, influenced by gravitational forces, described by the equation m\ddot{r}=-\frac{k}{r^{2}}+\frac{l^{2}}{mr^{3}}. The equilibrium radius r_{0} can be derived in terms of constants k, l, and m. When the particle is perturbed near this equilibrium radius (r=r_{0}+\epsilon), it exhibits oscillatory behavior, and the frequency of oscillation is determined using the effective potential approach, specifically through the relation \omega=\sqrt{\frac{1}{m}\frac{d^2U_{eff}}{dr^2}}. The method involves substituting r=r_0+\epsilon into the motion equation and applying a Taylor expansion.

PREREQUISITES
  • Understanding of classical mechanics, particularly gravitational forces.
  • Familiarity with differential equations and their applications in motion.
  • Knowledge of angular momentum and its role in radial motion.
  • Experience with Taylor series expansions in mathematical physics.
NEXT STEPS
  • Study the derivation of effective potential in gravitational systems.
  • Learn about oscillatory motion in classical mechanics.
  • Explore the application of Taylor series in physics problems.
  • Investigate the relationship between angular momentum and radial motion in three dimensions.
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Students of classical mechanics, physicists analyzing gravitational systems, and anyone interested in the dynamics of oscillatory motion in multi-dimensional spaces.

AbigailM
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Homework Statement


A particle of mass m moving in three dimensions is attracted to the origin by the gravitational force of a much heavier object. It can be shown that the radial motion is governed by the following equation
[itex]m\ddot{r}=-\frac{k}{r^{2}}+\frac{l^{2}}{mr^{3}}[/itex]

where k is a constant and l is the angular momentum. Determine an equilibrium radius [itex]r_{0}[/itex] in terms of k, l, and m. If the particle is put near that equilibrium radius, [itex]r=r_{0}+\epsilon[/itex](where [itex]\epsilon << r_{0}[/itex]), it will have an oscillatory radial motion about [itex]r_{0}[/itex]. What will be the frequency of that oscillation?

The Attempt at a Solution


Attached to thread as I'm horribly slow at typing latex.
 

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Your final answer looks correct, but I'm not quite sure what it is you've done to get it. Specifically, why do you assert that [itex]\omega=\sqrt{\frac{1}{m}\frac{d^2U_{eff}}{dr^2}}[/itex]? Is the RHS of this equation even a constant?

The method I would suggest is to just plug [itex]r=r_0+\epsilon[/itex] into your equation of motion and Taylor expand the RHS of it in powers of [itex]\frac{\epsilon}{r_0}[/itex] (since you know that it is much smaller than one).
 

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