Simple Harmonic Motion Inside earth

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SUMMARY

The discussion centers on the analysis of a particle's motion when dropped into a hole drilled through the center of the Earth, assuming uniform density. It establishes that the motion is simple harmonic and calculates the oscillation period to be approximately 84 minutes. The key equation derived is F(x) = -Kx, where K is a constant related to gravitational force and density. The participants emphasize the importance of recognizing that only the mass within the current radius contributes to the net force on the particle.

PREREQUISITES
  • Understanding of Newton's second law of motion
  • Familiarity with gravitational force equations
  • Knowledge of calculus, particularly integration techniques
  • Concept of simple harmonic motion and its characteristics
NEXT STEPS
  • Study the derivation of gravitational force in spherical coordinates
  • Learn about the implications of uniform density in gravitational fields
  • Explore the mathematical foundations of simple harmonic motion
  • Investigate the effects of rotational dynamics on oscillatory motion
USEFUL FOR

Students of physics, particularly those studying mechanics, educators teaching gravitational concepts, and anyone interested in the dynamics of oscillatory systems within gravitational fields.

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Homework Statement


A particle is dropped into a hole drilled straight through the center of the Earth. Neglecting rotational effects, show that the particle's motion is simple harmonic if you assume Earth has uniform density. Show that the period of the oscillation is about 84 min.


Homework Equations


[tex]F = -G m \int_V \frac{\rho(r') e_r}{r^2}dv'[/tex]


The Attempt at a Solution



I was going to use Newton's second law to show that
[tex]m \frac{d^2 r}{dt^2} = -G m \int_V \frac{\rho(r') e_r}{r^2}dv'[/tex]

Where the volume integral should produce some function of r. So, I started off the integration by choosing an arbitrary point in the sphere a distance r' away, and using R as the distance from the origin to the point mass, r as the distance between the arbitrary distance and the distance of the point mass, theta as the asimuthal angle, and phi as the rotational angle I got.

[tex]m \frac{d^2 r}{dt^2} = -G m \int_0^{R} \int_0^\pi \int_0^{2\pi} \frac{\rho r'^2 sin\theta}{r^2}dr' d\theta d\phi[/tex]

integrating with respect to phi brings in a factor of 2π, and now I used law of cosines

[tex]r^2 = r'^2 + R^2 - 2r'Rcos\theta[/tex]

[tex]2r dr = 2r'Rsin\theta d\theta[/tex]

[tex]\frac{sin\theta}{r}d\theta = \frac{dr}{r'R}[/tex]

so the substitute the law of cosines stuff into the force equation

[tex]F = \frac{-2 \pi G m \rho}{R} \int_0^R r'^2 dr \int_{r'-R}^{r'+R} \frac{1}{r}dr[/tex]

doing the r' integral I can see that this ultimately won't give a linear function of R

[tex]\frac{2 \pi}{3} \frac{G m \rho}{R} R^3 \int_{r'-R}^{r'+R} \frac{1}{r}dr[/tex]

Can someone help me out, point out what I did wrong, put me on the right track?

I think that once I find the right equation for force, which I actually know from experience should be [tex]F(r) = -\frac{4 \pi}{3}G m r \rho[/tex], that I can do the differential equation stuff.
 
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You're making it too complicated. Assume that the density of the Earth is a constant function, and realize that because of the character of the 1/r^2 force law, you can turn this into a surface integral. Once you do that, you're golden.
 
At any point in the fall, the only mass exerting a nett force on the test body is that contained inside the current radius because the shell of matter outside the radius has no effect. So the force at point x is

[tex]F(x) = -\frac{4}{3}\pi Gm\rho x^3/x^2[/tex]

which gives

[tex]F(x) = -Kx[/tex]

QED I think. Assuming uniform density.
 
Last edited:

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