Can the Gauss Law for Gravitation be used to prove the Shell Theorem?

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SUMMARY

The discussion centers on using Gauss's Law for Gravitation to prove the Shell Theorem, which states that an object inside a uniformly dense spherical shell experiences no net gravitational force from the shell. The participants explore the mathematical setup involving gravitational force equations, specifically F = GmM/r², and consider the implications of uniform density on gravitational calculations. The approach involves integrating the gravitational contributions from differential mass elements of the shell, leading to the conclusion that the net force is zero within the shell.

PREREQUISITES
  • Understanding of Gauss's Law for Gravitation
  • Familiarity with gravitational force equations, specifically F = GmM/r²
  • Basic knowledge of calculus for integration of differential mass elements
  • Concept of uniform density in spherical shells
NEXT STEPS
  • Study the derivation of the Shell Theorem in classical mechanics
  • Learn about the applications of Gauss's Law in gravitational fields
  • Explore integration techniques for calculating gravitational forces from continuous mass distributions
  • Examine examples of gravitational interactions in astrophysics involving spherical symmetry
USEFUL FOR

Students of physics, particularly those studying classical mechanics, as well as educators and anyone interested in gravitational theory and its applications in real-world scenarios.

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Homework Statement


Prove that an object within a spherically symmetric shell with uniform density will feel no gravitational force due to the mass of the shell. Let the density of the shell be ρ, the mass of the object be m, the radii to the inner and outer surfaces be r1 and r2 respectively, and let the mass of the shell be M.

Homework Equations


F = GmM/r^2

The Attempt at a Solution



so far I've drawn my setup. I tried to emulate the wikipedia article's drawing so that now I have two shells basically. I'm not exactly sure where I should go from here.

I have:

dFR = GmdM/(s^{2}_{1})cos(\varphi_{1}) + GmdM/(s^{2}_{2})cos(\varphi_{2})

but... can't I just take the distance and angle right in the middle of those two? I'll call them x and \alpha

so that I have

dFR = GmdM/(x^{2})cos(\alpha)

where x = (s1 + s2)/2

and \alpha = (\varphi_{1} + \varphi_{2})/2

?

if so that would make things a lot easier

I think that it would be okay to do that because it says that the shell has uniform density
 

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I think you would like to use the ' Gauss Law for Gravitation '.
 

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