Particle falling inside a sphere due to gravity

AI Thread Summary
The discussion centers on calculating the time it takes for a particle to fall through a drilled hole from one side of the Earth to the other, influenced by Earth's radius and density. The gravitational field inside a sphere is described by the equation g = (4πGρ/3)r, leading to the velocity function v(r) = r√(4πGρ). The motion is identified as oscillatory, represented by a second-order differential equation, allowing the derivation of the period T = √(3π/(Gρ)). This period does not depend on the radius of the sphere, although density plays a crucial role. Interestingly, the period for the particle's motion matches that of a theoretical satellite orbiting Earth at its surface.
Robin04
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Homework Statement


We drill a hole from the surface of the Earth to the other side through the center, drop a test particle and measure the time it takes to come back. How does this time depend on the radius and density of the Earth?

Homework Equations

The Attempt at a Solution


The gravitation field inside a sphere is ##g=\frac{4\pi G\rho}{3}r##, where ##G## is the gravitational constant, ##\rho## is the density, ##r## is the distance from the center.
Now I have to find the function ##r(t)##. I already found ##v(r)=r\sqrt{4\pi G \rho}## (the initial velocity is zero). How can I bring time into the equation?
 
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Robin04 said:

Homework Statement


We drill a hole from the surface of the Earth to the other side through the center, drop a test particle and measure the time it takes to come back. How does this time depend on the radius and density of the Earth?

Homework Equations

The Attempt at a Solution


The gravitation field inside a sphere is ##g=\frac{4\pi G\rho}{3}r##, where ##G## is the gravitational constant, ##\rho## is the density, ##r## is the distance from the center.
Now I have to find the function ##r(t)##. I already found ##v(r)=r\sqrt{4\pi G \rho}## (the initial velocity is zero). How can I bring time into the equation?

Since the motion is oscillatory motion, you can think a form of Second order DE, such that

$$d^2r/dt^2+ω^2r=0$$ where ##ω## will be the anguler frequency or ##w=2π/T##
 
Arman777 said:
Since the motion is oscillatory motion, you can think a form of Second order DE, such that

$$d^2r/dt^2+ω^2r=0$$ where ##ω## will be the anguler frequency or ##w=2π/T##
So I could say ##g+\omega^2r=0##, from which ##T=\sqrt{\frac{3\pi}{G\rho}}## Is this correct? It doesn't depend on the radius of the sphere.
 
Robin04 said:
So I could say ##g+\omega^2r=0##, from which ##T=\sqrt{\frac{3\pi}{G\rho}}## Is this correct? It doesn't depend on the radius of the sphere.
It's true yes. I don't think we can get the density and the radius in the same equation. For the radius dependence put the ##ρ## value in the equation that you find and you ll see that it depends also on radius in some other aspect.
 
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Arman777 said:
It's true yes. I don't think we can get the density and the radius in the same equation. For the radius dependence put the ##ρ## value in the equation that you find and you ll see that it depends also on radius in some other aspect.
Thank you! :)
 
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A bit of trivia: the period for your particle is the same as for a (theoretical) satellite orbiting the Earth at its surface.
 
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