Motion in a Central Gravitational Force

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SUMMARY

The discussion centers on the motion of a particle influenced by a central inverse-square-law force field, specifically described by the equation F(r) = -k/r² - λ/r³, where k and λ are positive constants. Participants emphasize the need to derive the motion's characteristics, particularly demonstrating that it results in a precessing ellipse. The differential equation (d²/dθ²)(1/r) + (1/r) = -μr²F(r)/l² is highlighted as a critical starting point for analysis, although participants express uncertainty in manipulating the left-hand side of the equation.

PREREQUISITES
  • Understanding of central force motion and inverse-square laws
  • Familiarity with differential equations and their applications in physics
  • Knowledge of orbital mechanics and precession concepts
  • Proficiency in LaTeX for mathematical expressions
NEXT STEPS
  • Derive the motion equations for central force problems using LaTeX
  • Study the properties of precessing orbits in gravitational fields
  • Explore the implications of superimposed forces on particle motion
  • Learn about the applications of differential equations in classical mechanics
USEFUL FOR

Students and educators in physics, particularly those studying classical mechanics and orbital dynamics, will benefit from this discussion. It is also valuable for anyone interested in the mathematical modeling of forces and motion.

Macykc2
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Homework Statement


Discuss the motion of a particle in a central inverse-square-law force field for a superimposed force whose magnitude is inversely proportional to the cube of the distance from the particle to the force center, that is:
F(r) = -k/r2 - λ/r3 and k,λ>0​
Show that the motion is described by a precessing ellipse.

Homework Equations


The one given in the question

The Attempt at a Solution


I honestly don't know where to begin, we derived an equation in class that we could find the force law if a particular known orbit r=r(θ), and I was thinking of using it:
(d2/dθ2)(1/r) + (1/r) = -μr2F(r)/l2
but I don't know what to do with the left hand side, but again it's just a guess as to what to start with.
Sorry for not using the math commands, they didn't want to work for some reason.
 
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You need to solve the differential equation.

For equations, you can type out LaTeX markup directly.

You may want to back up a bit and make sure you understand the motivation for deriving the equation you used in the first place... see if the same approach still applies here.
 

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