How to characterize a power law field?

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SUMMARY

This discussion focuses on characterizing power law fields defined by the equation F = -K/r^n, where 'u' is the radial vector. The conversation highlights methods for recognizing these fields through the analysis of trajectories of moving material points, emphasizing that n=2 and n=-1 yield closed non-circular orbits. Additionally, it explores the use of theoretical models, such as Van der Waals forces, to determine the power coefficient 'n' and discusses applications in cosmology and particle interactions at infinitesimal scales.

PREREQUISITES
  • Understanding of central force fields in classical mechanics
  • Familiarity with the mathematical representation of power laws
  • Knowledge of trajectory analysis in physics
  • Basic concepts of cosmology and quantum mechanics
NEXT STEPS
  • Study the mathematical derivation of trajectories in power law fields
  • Research Van der Waals forces and their applications in theoretical models
  • Explore the implications of power law fields in cosmological models
  • Investigate quantum mechanics effects on particle interactions at small scales
USEFUL FOR

Physicists, students of classical mechanics, cosmologists, and researchers interested in the dynamics of central force fields and their applications in both macroscopic and microscopic contexts.

Moleculmol
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Hello, as part of the study of fields with central forces, I came across with fields called power law, defined by F = - K/r ^ n u
(u is radial vector passing through the origin O)
I would like to dismiss case n = 2, which refers to the Newtonian fields whose study was exhaustively conducted in class. My questions are:
-How to recognize a power law field from the trajectory of a moving material point in this field?
- Once the nature of the field identified (power law), the determination of the power n can be conjectured by reasoning on heuristic considerations, however are there any situations where one can resort to theoretical models to find this coefficient (I think for example to VanderWalls force but I would like another example).
- An example of application of these methods to a concrete physical situation, in cosmology (movement of the stars) or interactions between particles at infinitesimal scale.
Thank you in advance.
 
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Moleculmol said:
Summary: In classic mechanics, central forces with the form -k/r^n are often introduced to model actions that are directed along the line joining the object and the origin.

-How to recognize a power law field from the trajectory of a moving material point in this field?
Calculate how the motion will look like for different powers, then do the opposite if you have a given trajectory. n=2 and n=-1 are the only cases that lead to closed non-circular orbits.
Moleculmol said:
- An example of application of these methods to a concrete physical situation, in cosmology (movement of the stars) or interactions between particles at infinitesimal scale.
Well, on large scales these are all n=2, on small scales you probably have to consider quantum mechanics and things get more complicated.
 

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