How to Derive Equations of Motion for Colliding Masses in a Central Field?

PhysStudent81
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Homework Statement



I have two masses of finite width, m_1 and m_2. The force is Newton's gravity, so U = k/r. I want to work out their relevant equations of motions r_1(t) and r_2(t) as they start off from rest and collide. I don't want to consider any rotational motion.


Homework Equations



U = \frac{k}{r}
r = r_{1}(t) - r_{2}(t)

0.5μ\dot{r}^2 = E_{tot} - \frac{k}{r}

dt = \frac{μ}{2}∫\frac{dr}{\sqrt{E_{tot} - \frac{k}{r}}}

The Attempt at a Solution



I try to integrate the above equation it gives me something very complicated (I end up integrating cosec^3 after making the substitution \frac{1}{r} = \sin^{2}(\theta)) which gives me t = t(r), but I can't invert this to give me r = r(t).

Am I doing something wrong? Is there another way of doing it that doesn't involve lagrangian or hamiltonian dynamics (which I haven't studied).

Another way would be to solve the the 2nd order differential equation directly:

\frac{dr^{2}}{dt^{2}} = \frac{k}{r^{2}}

but I can't seem to do this (I fee I'm missing something very simple here). I know that if I let r = At^{\frac{2}{3}} this is a solution but it doesn't have enough constants.

Any pointers?

Thanks,

Rob
 
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PhysStudent81 said:
I try to integrate the above equation it gives me something very complicated (I end up integrating cosec^3 after making the substitution \frac{1}{r} = \sin^{2}(\theta)) which gives me t = t(r), but I can't invert this to give me r = r(t).

Am I doing something wrong?

I think what you are doing is correct. Did you allow for the fact that both k and Etot are negative numbers? Anyway, as you say, you can get an expression for t(r). I agree that the result looks too complicated to invert for r(t).
 
So strange that for such seemingly simple problem there is no closed form result for r(t). t(r) is actually all I wanted so that's ok!
 
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