1D three-body problem (with spherical shell)

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SUMMARY

The discussion centers on the 1D three-body problem involving two point masses, m1 and m2, and a spherical shell with mass M. The initial conditions specify that both h1 and H start at h0, while h2 begins at 0, with all derivatives equal to zero at time t=0. The equations of motion are defined using Newton's law of gravitation, leading to a system of differential equations that describe the interactions between the masses. The primary inquiry is whether this system can be solved to demonstrate that mass m1 remains at the center of the spherical shell over time.

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Let's suppose that we have two point particles with masses m1,m2 and the spherical shell with mass M, placed in a line, at distances h1,h2 and H from 0 in that line (0 is the center of some inertial frame of reference). The initial conditions and the equations of motion are the following:

h_1(0)=H(0)=h_0

h_2(0)=0

h_1'(0)=h_2'(0)=H'(0)=0 (time derivative)

(the mass m1 is in the center of the spherical shell at time t=0, but I'm trying to prove that for every t)\frac{d^2h_1(t)}{dt^2}=-G\frac{m_2}{(h_1-h_2)^2}

\frac{d^2h_2(t)}{dt^2}=G\frac{m_1}{(h_1-h_2)^2}+G\frac{M}{(H-h_2)^2}

\frac{d^2H(t)}{dt^2}=-G\frac{m_2}{(H-h_2)^2}

Is there any way to solve this problem (to find the positions of the masses as functions of the time)?
 
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Αnyone? At least tell me if this problem is solvable or not.
It seems quiet easy but the system off differential equantions is hard to solve. Is there any other way to solve it?

Actually what i am trying to prove is \frac{d^2 h_1(t)}{dt^2}=\frac{d^2 H(t)}{dt^2} and that the mass m1 will remain in the center of spherical shell.
 

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